---
_id: '14852'
abstract:
- lang: eng
  text: The physical conditions giving rise to high escape fractions of ionizing radiation
    (LyC fesc) in star-forming galaxies – most likely protagonists of cosmic reionization
    – are not yet fully understood. Using the VLT/MUSE observations of ∼1400 Ly α
    emitters at 2.9 &amp;lt; z &amp;lt; 6.7, we compare stacked rest-frame UV spectra
    of candidates for LyC leakers and non-leakers selected based on their Ly α profiles.
    We find that the stacks of potential LyC leakers, i.e. galaxies with narrow, symmetric
    Ly α profiles with small peak separation, generally show (i) strong nebular O iii]λ1666,
    [Si iii]λ1883, and [C iii]λ1907 +C iii]λ1909 emission, indicating a high-ionization
    state of the interstellar medium (ISM); (ii) high equivalent widths of He iiλ1640
    (∼1 − 3 Å), suggesting the presence of hard ionizing radiation fields; (iii) Si ii*λ1533
    emission, revealing substantial amounts of neutral hydrogen off the line of sight;
    (iv) high C ivλλ1548,1550 to [C iii]λ1907 +C iii]λ1909 ratios (C iv/C iii] ≳0.75)
    , signalling the presence of low column density channels in the ISM. In contrast,
    the stacks with broad, asymmetric Ly α profiles with large peak separation show
    weak nebular emission lines, low He iiλ1640 equivalent widths (≲1 Å), and low
    C iv/C iii] (≲0.25), implying low-ionization states and high-neutral hydrogen
    column densities. Our results suggest that C iv/C iii] might be sensitive to the
    physical conditions that govern LyC photon escape, providing a promising tool
    for identification of ionizing sources among star-forming galaxies in the epoch
    of reionization.
acknowledgement: 'We thank the anonymous referee for the constructive feedback that
  helped to improve the manuscript. We thank Michael Maseda, Daniel Schaerer, Charlotte
  Simmonds, and Rashmi Gottumukkala for useful comments and productive discussions.
  We also thank the organizers and participants of the 24th MUSE Science Busy Week
  in Leiden. IGK acknowledges an Excellence Master Fellowship granted by the Faculty
  of Science of the University of Geneva. This work has received funding from the
  Swiss State Secretariat for Education, Research and Innovation (SERI) under contract
  number MB22.00072, as well as from the Swiss National Science Foundation (SNSF)
  through project grant number 200020_207349 and SNSF Professorship grant number 190079.
  The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation
  under grant number 140. This paper is based on observations collected at the European
  Organisation for Astronomical Research in the Southern Hemisphere under ESO programmes
  094.A-0289(B), 095.A-0010(A), 096.A-0045(A), 096.A-0045(B), 094.A-0205, 095.A-0240,
  096.A-0090, 097.A-0160, and 098.A-0017. We made extensive use of several open-source
  software packages and we are thankful to the respective authors for sharing their
  work: NUMPY (Harris et al. 2020), ASTROPY (Astropy Collaboration 2022), MATPLOTLIB
  (Hunter 2007), IPYTHON (Perez & Granger 2007), and TOPCAT (Taylor 2005).'
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Ivan
  full_name: Kramarenko, Ivan
  id: 9a9394cb-3200-11ee-973b-f5ba2a8b16e4
  last_name: Kramarenko
- first_name: J
  full_name: Kerutt, J
  last_name: Kerutt
- first_name: A
  full_name: Verhamme, A
  last_name: Verhamme
- first_name: P A
  full_name: Oesch, P A
  last_name: Oesch
- first_name: L
  full_name: Barrufet, L
  last_name: Barrufet
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: H
  full_name: Kusakabe, H
  last_name: Kusakabe
- first_name: I
  full_name: Goovaerts, I
  last_name: Goovaerts
- first_name: T T
  full_name: Thai, T T
  last_name: Thai
citation:
  ama: Kramarenko I, Kerutt J, Verhamme A, et al. Linking UV spectral properties of
    MUSE Ly α emitters at <i>z</i> ≳ 3 to Lyman continuum escape. <i>Monthly Notices
    of the Royal Astronomical Society</i>. 2024;527(4):9853-9871. doi:<a href="https://doi.org/10.1093/mnras/stad3853">10.1093/mnras/stad3853</a>
  apa: Kramarenko, I., Kerutt, J., Verhamme, A., Oesch, P. A., Barrufet, L., Matthee,
    J. J., … Thai, T. T. (2024). Linking UV spectral properties of MUSE Ly α emitters
    at <i>z</i> ≳ 3 to Lyman continuum escape. <i>Monthly Notices of the Royal Astronomical
    Society</i>. Oxford University Press. <a href="https://doi.org/10.1093/mnras/stad3853">https://doi.org/10.1093/mnras/stad3853</a>
  chicago: Kramarenko, Ivan, J Kerutt, A Verhamme, P A Oesch, L Barrufet, Jorryt J
    Matthee, H Kusakabe, I Goovaerts, and T T Thai. “Linking UV Spectral Properties
    of MUSE Ly α Emitters at <i>z</i> ≳ 3 to Lyman Continuum Escape.” <i>Monthly Notices
    of the Royal Astronomical Society</i>. Oxford University Press, 2024. <a href="https://doi.org/10.1093/mnras/stad3853">https://doi.org/10.1093/mnras/stad3853</a>.
  ieee: I. Kramarenko <i>et al.</i>, “Linking UV spectral properties of MUSE Ly α
    emitters at <i>z</i> ≳ 3 to Lyman continuum escape,” <i>Monthly Notices of the
    Royal Astronomical Society</i>, vol. 527, no. 4. Oxford University Press, pp.
    9853–9871, 2024.
  ista: Kramarenko I, Kerutt J, Verhamme A, Oesch PA, Barrufet L, Matthee JJ, Kusakabe
    H, Goovaerts I, Thai TT. 2024. Linking UV spectral properties of MUSE Ly α emitters
    at <i>z</i> ≳ 3 to Lyman continuum escape. Monthly Notices of the Royal Astronomical
    Society. 527(4), 9853–9871.
  mla: Kramarenko, Ivan, et al. “Linking UV Spectral Properties of MUSE Ly α Emitters
    at <i>z</i> ≳ 3 to Lyman Continuum Escape.” <i>Monthly Notices of the Royal Astronomical
    Society</i>, vol. 527, no. 4, Oxford University Press, 2024, pp. 9853–71, doi:<a
    href="https://doi.org/10.1093/mnras/stad3853">10.1093/mnras/stad3853</a>.
  short: I. Kramarenko, J. Kerutt, A. Verhamme, P.A. Oesch, L. Barrufet, J.J. Matthee,
    H. Kusakabe, I. Goovaerts, T.T. Thai, Monthly Notices of the Royal Astronomical
    Society 527 (2024) 9853–9871.
date_created: 2024-01-22T08:22:17Z
date_published: 2024-02-01T00:00:00Z
date_updated: 2024-01-23T12:33:50Z
day: '01'
ddc:
- '520'
department:
- _id: GradSch
- _id: JoMa
doi: 10.1093/mnras/stad3853
external_id:
  arxiv:
  - '2305.07044'
file:
- access_level: open_access
  checksum: 9d02df4035c4951cf63dee0db1e462e9
  content_type: application/pdf
  creator: dernst
  date_created: 2024-01-23T12:30:45Z
  date_updated: 2024-01-23T12:30:45Z
  file_id: '14879'
  file_name: 2024_MNAstronomSoc_Kramarenko.pdf
  file_size: 4521738
  relation: main_file
  success: 1
file_date_updated: 2024-01-23T12:30:45Z
has_accepted_license: '1'
intvolume: '       527'
issue: '4'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
license: https://creativecommons.org/licenses/by/4.0/
month: '02'
oa: 1
oa_version: Published Version
page: 9853-9871
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
  eissn:
  - 1365-2966
  issn:
  - 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
status: public
title: Linking UV spectral properties of MUSE Ly α emitters at <i>z</i> ≳ 3 to Lyman
  continuum escape
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 527
year: '2024'
...
---
_id: '15053'
abstract:
- lang: eng
  text: Atom-based quantum simulators have had many successes in tackling challenging
    quantum many-body problems, owing to the precise and dynamical control that they
    provide over the systems' parameters. They are, however, often optimized to address
    a specific type of problem. Here, we present the design and implementation of
    a 6Li-based quantum gas platform that provides wide-ranging capabilities and is
    able to address a variety of quantum many-body problems. Our two-chamber architecture
    relies on a robust combination of gray molasses and optical transport from a laser-cooling
    chamber to a glass cell with excellent optical access. There, we first create
    unitary Fermi superfluids in a three-dimensional axially symmetric harmonic trap
    and characterize them using in situ thermometry, reaching temperatures below 20
    nK. This allows us to enter the deep superfluid regime with samples of extreme
    diluteness, where the interparticle spacing is sufficiently large for direct single-atom
    imaging. Second, we generate optical lattice potentials with triangular and honeycomb
    geometry in which we study diffraction of molecular Bose-Einstein condensates,
    and show how going beyond the Kapitza-Dirac regime allows us to unambiguously
    distinguish between the two geometries. With the ability to probe quantum many-body
    physics in both discrete and continuous space, and its suitability for bulk and
    single-atom imaging, our setup represents an important step towards achieving
    a wide-scope quantum simulator.
acknowledgement: We thank Clara Bachorz, Darby Bates, Markus Bohlen, Valentin Crépel,
  Yann Kiefer, Joanna Lis, Mihail Rabinovic, and Julian Struck for experimental assistance
  in the early stages of this project, and Sebastian Will for a critical reading of
  the manuscript. This work has been supported by Agence Nationale de la Recherche
  (Grant No. ANR-21-CE30-0021), the European Research Council (Grant No. ERC-2016-ADG-743159),
  CNRS (Tremplin@INP 2020), and Région Ile-de-France in the framework of DIM SIRTEQ
  (Super2D and SISCo) and DIM QuanTiP.
article_number: '013158'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Shuwei
  full_name: Jin, Shuwei
  last_name: Jin
- first_name: Kunlun
  full_name: Dai, Kunlun
  last_name: Dai
- first_name: Joris
  full_name: Verstraten, Joris
  last_name: Verstraten
- first_name: Maxime
  full_name: Dixmerias, Maxime
  last_name: Dixmerias
- first_name: Ragheed
  full_name: Al Hyder, Ragheed
  id: d1c405be-ae15-11ed-8510-ccf53278162e
  last_name: Al Hyder
- first_name: Christophe
  full_name: Salomon, Christophe
  last_name: Salomon
- first_name: Bruno
  full_name: Peaudecerf, Bruno
  last_name: Peaudecerf
- first_name: Tim
  full_name: de Jongh, Tim
  last_name: de Jongh
- first_name: Tarik
  full_name: Yefsah, Tarik
  last_name: Yefsah
citation:
  ama: Jin S, Dai K, Verstraten J, et al. Multipurpose platform for analog quantum
    simulation. <i>Physical Review Research</i>. 2024;6(1). doi:<a href="https://doi.org/10.1103/physrevresearch.6.013158">10.1103/physrevresearch.6.013158</a>
  apa: Jin, S., Dai, K., Verstraten, J., Dixmerias, M., Al Hyder, R., Salomon, C.,
    … Yefsah, T. (2024). Multipurpose platform for analog quantum simulation. <i>Physical
    Review Research</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevresearch.6.013158">https://doi.org/10.1103/physrevresearch.6.013158</a>
  chicago: Jin, Shuwei, Kunlun Dai, Joris Verstraten, Maxime Dixmerias, Ragheed Al
    Hyder, Christophe Salomon, Bruno Peaudecerf, Tim de Jongh, and Tarik Yefsah. “Multipurpose
    Platform for Analog Quantum Simulation.” <i>Physical Review Research</i>. American
    Physical Society, 2024. <a href="https://doi.org/10.1103/physrevresearch.6.013158">https://doi.org/10.1103/physrevresearch.6.013158</a>.
  ieee: S. Jin <i>et al.</i>, “Multipurpose platform for analog quantum simulation,”
    <i>Physical Review Research</i>, vol. 6, no. 1. American Physical Society, 2024.
  ista: Jin S, Dai K, Verstraten J, Dixmerias M, Al Hyder R, Salomon C, Peaudecerf
    B, de Jongh T, Yefsah T. 2024. Multipurpose platform for analog quantum simulation.
    Physical Review Research. 6(1), 013158.
  mla: Jin, Shuwei, et al. “Multipurpose Platform for Analog Quantum Simulation.”
    <i>Physical Review Research</i>, vol. 6, no. 1, 013158, American Physical Society,
    2024, doi:<a href="https://doi.org/10.1103/physrevresearch.6.013158">10.1103/physrevresearch.6.013158</a>.
  short: S. Jin, K. Dai, J. Verstraten, M. Dixmerias, R. Al Hyder, C. Salomon, B.
    Peaudecerf, T. de Jongh, T. Yefsah, Physical Review Research 6 (2024).
date_created: 2024-03-04T07:42:52Z
date_published: 2024-02-13T00:00:00Z
date_updated: 2024-03-04T07:55:29Z
day: '13'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1103/physrevresearch.6.013158
external_id:
  arxiv:
  - '2304.08433'
file:
- access_level: open_access
  checksum: ba2ae3e3a011f8897d3803c9366a67e2
  content_type: application/pdf
  creator: dernst
  date_created: 2024-03-04T07:53:08Z
  date_updated: 2024-03-04T07:53:08Z
  file_id: '15054'
  file_name: 2024_PhysicalReviewResearch_Jin.pdf
  file_size: 4025988
  relation: main_file
  success: 1
file_date_updated: 2024-03-04T07:53:08Z
has_accepted_license: '1'
intvolume: '         6'
issue: '1'
keyword:
- General Physics and Astronomy
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
publication: Physical Review Research
publication_identifier:
  issn:
  - 2643-1564
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Multipurpose platform for analog quantum simulation
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 6
year: '2024'
...
---
_id: '12165'
abstract:
- lang: eng
  text: It may come as a surprise that a phenomenon as ubiquitous and prominent as
    the transition from laminar to turbulent flow has resisted combined efforts by
    physicists, engineers and mathematicians, and remained unresolved for almost one
    and a half centuries. In recent years, various studies have proposed analogies
    to directed percolation, a well-known universality class in statistical mechanics,
    which describes a non-equilibrium phase transition from a fluctuating active phase
    into an absorbing state. It is this unlikely relation between the multiscale,
    high-dimensional dynamics that signify the transition process in virtually all
    flows of practical relevance, and the arguably most basic non-equilibrium phase
    transition, that so far has mainly been the subject of model studies, which I
    review in this Perspective.
article_processing_charge: No
article_type: original
author:
- first_name: Björn
  full_name: Hof, Björn
  id: 3A374330-F248-11E8-B48F-1D18A9856A87
  last_name: Hof
  orcid: 0000-0003-2057-2754
citation:
  ama: Hof B. Directed percolation and the transition to turbulence. <i>Nature Reviews
    Physics</i>. 2023;5:62-72. doi:<a href="https://doi.org/10.1038/s42254-022-00539-y">10.1038/s42254-022-00539-y</a>
  apa: Hof, B. (2023). Directed percolation and the transition to turbulence. <i>Nature
    Reviews Physics</i>. Springer Nature. <a href="https://doi.org/10.1038/s42254-022-00539-y">https://doi.org/10.1038/s42254-022-00539-y</a>
  chicago: Hof, Björn. “Directed Percolation and the Transition to Turbulence.” <i>Nature
    Reviews Physics</i>. Springer Nature, 2023. <a href="https://doi.org/10.1038/s42254-022-00539-y">https://doi.org/10.1038/s42254-022-00539-y</a>.
  ieee: B. Hof, “Directed percolation and the transition to turbulence,” <i>Nature
    Reviews Physics</i>, vol. 5. Springer Nature, pp. 62–72, 2023.
  ista: Hof B. 2023. Directed percolation and the transition to turbulence. Nature
    Reviews Physics. 5, 62–72.
  mla: Hof, Björn. “Directed Percolation and the Transition to Turbulence.” <i>Nature
    Reviews Physics</i>, vol. 5, Springer Nature, 2023, pp. 62–72, doi:<a href="https://doi.org/10.1038/s42254-022-00539-y">10.1038/s42254-022-00539-y</a>.
  short: B. Hof, Nature Reviews Physics 5 (2023) 62–72.
date_created: 2023-01-12T12:10:18Z
date_published: 2023-01-01T00:00:00Z
date_updated: 2023-08-01T12:50:48Z
day: '01'
department:
- _id: BjHo
doi: 10.1038/s42254-022-00539-y
external_id:
  isi:
  - '000890148700002'
intvolume: '         5'
isi: 1
keyword:
- General Physics and Astronomy
language:
- iso: eng
month: '01'
oa_version: None
page: 62-72
publication: Nature Reviews Physics
publication_identifier:
  eissn:
  - 2522-5820
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Directed percolation and the transition to turbulence
type: journal_article
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 5
year: '2023'
...
---
_id: '12723'
abstract:
- lang: eng
  text: 'Lead halide perovskites enjoy a number of remarkable optoelectronic properties.
    To explain their origin, it is necessary to study how electromagnetic fields interact
    with these systems. We address this problem here by studying two classical quantities:
    Faraday rotation and the complex refractive index in a paradigmatic perovskite
    CH3NH3PbBr3 in a broad wavelength range. We find that the minimal coupling of
    electromagnetic fields to the k⋅p Hamiltonian is insufficient to describe the
    observed data even on the qualitative level. To amend this, we demonstrate that
    there exists a relevant atomic-level coupling between electromagnetic fields and
    the spin degree of freedom. This spin-electric coupling allows for quantitative
    description of a number of previous as well as present experimental data. In particular,
    we use it here to show that the Faraday effect in lead halide perovskites is dominated
    by the Zeeman splitting of the energy levels and has a substantial beyond-Becquerel
    contribution. Finally, we present general symmetry-based phenomenological arguments
    that in the low-energy limit our effective model includes all basis coupling terms
    to the electromagnetic field in the linear order.'
article_number: '106901'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Artem
  full_name: Volosniev, Artem
  id: 37D278BC-F248-11E8-B48F-1D18A9856A87
  last_name: Volosniev
  orcid: 0000-0003-0393-5525
- first_name: Abhishek
  full_name: Shiva Kumar, Abhishek
  id: 5e9a6931-eb97-11eb-a6c2-e96f7058d77a
  last_name: Shiva Kumar
- first_name: Dusan
  full_name: Lorenc, Dusan
  id: 40D8A3E6-F248-11E8-B48F-1D18A9856A87
  last_name: Lorenc
- first_name: Younes
  full_name: Ashourishokri, Younes
  id: e32c111f-f6e0-11ea-865d-eb955baea334
  last_name: Ashourishokri
- first_name: Ayan A.
  full_name: Zhumekenov, Ayan A.
  last_name: Zhumekenov
- first_name: Osman M.
  full_name: Bakr, Osman M.
  last_name: Bakr
- first_name: Mikhail
  full_name: Lemeshko, Mikhail
  id: 37CB05FA-F248-11E8-B48F-1D18A9856A87
  last_name: Lemeshko
  orcid: 0000-0002-6990-7802
- first_name: Zhanybek
  full_name: Alpichshev, Zhanybek
  id: 45E67A2A-F248-11E8-B48F-1D18A9856A87
  last_name: Alpichshev
  orcid: 0000-0002-7183-5203
citation:
  ama: Volosniev A, Shiva Kumar A, Lorenc D, et al. Spin-electric coupling in lead
    halide perovskites. <i>Physical Review Letters</i>. 2023;130(10). doi:<a href="https://doi.org/10.1103/physrevlett.130.106901">10.1103/physrevlett.130.106901</a>
  apa: Volosniev, A., Shiva Kumar, A., Lorenc, D., Ashourishokri, Y., Zhumekenov,
    A. A., Bakr, O. M., … Alpichshev, Z. (2023). Spin-electric coupling in lead halide
    perovskites. <i>Physical Review Letters</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevlett.130.106901">https://doi.org/10.1103/physrevlett.130.106901</a>
  chicago: Volosniev, Artem, Abhishek Shiva Kumar, Dusan Lorenc, Younes Ashourishokri,
    Ayan A. Zhumekenov, Osman M. Bakr, Mikhail Lemeshko, and Zhanybek Alpichshev.
    “Spin-Electric Coupling in Lead Halide Perovskites.” <i>Physical Review Letters</i>.
    American Physical Society, 2023. <a href="https://doi.org/10.1103/physrevlett.130.106901">https://doi.org/10.1103/physrevlett.130.106901</a>.
  ieee: A. Volosniev <i>et al.</i>, “Spin-electric coupling in lead halide perovskites,”
    <i>Physical Review Letters</i>, vol. 130, no. 10. American Physical Society, 2023.
  ista: Volosniev A, Shiva Kumar A, Lorenc D, Ashourishokri Y, Zhumekenov AA, Bakr
    OM, Lemeshko M, Alpichshev Z. 2023. Spin-electric coupling in lead halide perovskites.
    Physical Review Letters. 130(10), 106901.
  mla: Volosniev, Artem, et al. “Spin-Electric Coupling in Lead Halide Perovskites.”
    <i>Physical Review Letters</i>, vol. 130, no. 10, 106901, American Physical Society,
    2023, doi:<a href="https://doi.org/10.1103/physrevlett.130.106901">10.1103/physrevlett.130.106901</a>.
  short: A. Volosniev, A. Shiva Kumar, D. Lorenc, Y. Ashourishokri, A.A. Zhumekenov,
    O.M. Bakr, M. Lemeshko, Z. Alpichshev, Physical Review Letters 130 (2023).
date_created: 2023-03-14T13:11:59Z
date_published: 2023-03-10T00:00:00Z
date_updated: 2023-08-01T13:39:04Z
day: '10'
department:
- _id: GradSch
- _id: ZhAl
- _id: MiLe
doi: 10.1103/physrevlett.130.106901
external_id:
  arxiv:
  - '2203.09443'
  isi:
  - '000982435900002'
intvolume: '       130'
isi: 1
issue: '10'
keyword:
- General Physics and Astronomy
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2203.09443
month: '03'
oa: 1
oa_version: Preprint
publication: Physical Review Letters
publication_identifier:
  eissn:
  - 1079-7114
  issn:
  - 0031-9007
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Spin-electric coupling in lead halide perovskites
type: journal_article
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 130
year: '2023'
...
---
_id: '13197'
abstract:
- lang: eng
  text: "Nominally identical materials exchange net electric charge during contact
    through a mechanism that is still debated. ‘Mosaic models’, in which surfaces
    are presumed to consist of a random patchwork of microscopic donor/acceptor sites,
    offer an appealing explanation for this phenomenon. However, recent experiments
    have shown that global differences persist even between same-material samples,
    which the standard mosaic framework does not account for. Here, we expand the
    mosaic framework by incorporating global differences in the densities of donor/acceptor
    sites. We develop\r\nan analytical model, backed by numerical simulations, that
    smoothly connects the global and deterministic charge transfer of different materials
    to the local and stochastic mosaic picture normally associated with identical
    materials. Going further, we extend our model to explain the effect of contact
    asymmetries during sliding, providing a plausible explanation for reversal of
    charging sign that has been observed experimentally."
acknowledgement: "This project has received funding from the European Research Council
  Grant Agreement No. 949120 and from\r\nthe European Union’s Horizon 2020 research
  and innovation program under the Marie Sklodowska-Curie Grant\r\nAgreement No. 754411. "
article_number: '065601'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Galien M
  full_name: Grosjean, Galien M
  id: 0C5FDA4A-9CF6-11E9-8939-FF05E6697425
  last_name: Grosjean
  orcid: 0000-0001-5154-417X
- first_name: Scott R
  full_name: Waitukaitis, Scott R
  id: 3A1FFC16-F248-11E8-B48F-1D18A9856A87
  last_name: Waitukaitis
  orcid: 0000-0002-2299-3176
citation:
  ama: 'Grosjean GM, Waitukaitis SR. Asymmetries in triboelectric charging: Generalizing
    mosaic models to different-material samples and sliding contacts. <i>Physical
    Review Materials</i>. 2023;7(6). doi:<a href="https://doi.org/10.1103/physrevmaterials.7.065601">10.1103/physrevmaterials.7.065601</a>'
  apa: 'Grosjean, G. M., &#38; Waitukaitis, S. R. (2023). Asymmetries in triboelectric
    charging: Generalizing mosaic models to different-material samples and sliding
    contacts. <i>Physical Review Materials</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevmaterials.7.065601">https://doi.org/10.1103/physrevmaterials.7.065601</a>'
  chicago: 'Grosjean, Galien M, and Scott R Waitukaitis. “Asymmetries in Triboelectric
    Charging: Generalizing Mosaic Models to Different-Material Samples and Sliding
    Contacts.” <i>Physical Review Materials</i>. American Physical Society, 2023.
    <a href="https://doi.org/10.1103/physrevmaterials.7.065601">https://doi.org/10.1103/physrevmaterials.7.065601</a>.'
  ieee: 'G. M. Grosjean and S. R. Waitukaitis, “Asymmetries in triboelectric charging:
    Generalizing mosaic models to different-material samples and sliding contacts,”
    <i>Physical Review Materials</i>, vol. 7, no. 6. American Physical Society, 2023.'
  ista: 'Grosjean GM, Waitukaitis SR. 2023. Asymmetries in triboelectric charging:
    Generalizing mosaic models to different-material samples and sliding contacts.
    Physical Review Materials. 7(6), 065601.'
  mla: 'Grosjean, Galien M., and Scott R. Waitukaitis. “Asymmetries in Triboelectric
    Charging: Generalizing Mosaic Models to Different-Material Samples and Sliding
    Contacts.” <i>Physical Review Materials</i>, vol. 7, no. 6, 065601, American Physical
    Society, 2023, doi:<a href="https://doi.org/10.1103/physrevmaterials.7.065601">10.1103/physrevmaterials.7.065601</a>.'
  short: G.M. Grosjean, S.R. Waitukaitis, Physical Review Materials 7 (2023).
date_created: 2023-07-07T12:48:01Z
date_published: 2023-06-13T00:00:00Z
date_updated: 2023-08-02T06:34:47Z
day: '13'
ddc:
- '537'
department:
- _id: ScWa
doi: 10.1103/physrevmaterials.7.065601
ec_funded: 1
external_id:
  arxiv:
  - '2304.12861'
  isi:
  - '001019565900002'
file:
- access_level: open_access
  checksum: 75584730d9cdd50eeccb4c52c509776d
  content_type: application/pdf
  creator: ggrosjea
  date_created: 2023-07-07T12:49:51Z
  date_updated: 2023-07-07T12:49:51Z
  file_id: '13198'
  file_name: Mosaic_asymmetries.pdf
  file_size: 1127040
  relation: main_file
  success: 1
file_date_updated: 2023-07-07T12:49:51Z
has_accepted_license: '1'
intvolume: '         7'
isi: 1
issue: '6'
keyword:
- Physics and Astronomy (miscellaneous)
- General Materials Science
language:
- iso: eng
month: '06'
oa: 1
oa_version: Submitted Version
project:
- _id: 0aa60e99-070f-11eb-9043-a6de6bdc3afa
  call_identifier: H2020
  grant_number: '949120'
  name: 'Tribocharge: a multi-scale approach to an enduring problem in physics'
- _id: 260C2330-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '754411'
  name: ISTplus - Postdoctoral Fellowships
publication: Physical Review Materials
publication_identifier:
  issn:
  - 2475-9953
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
status: public
title: 'Asymmetries in triboelectric charging: Generalizing mosaic models to different-material
  samples and sliding contacts'
type: journal_article
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 7
year: '2023'
...
---
_id: '13274'
abstract:
- lang: eng
  text: Viscous flows through pipes and channels are steady and ordered until, with
    increasing velocity, the laminar motion catastrophically breaks down and gives
    way to turbulence. How this apparently discontinuous change from low- to high-dimensional
    motion can be rationalized within the framework of the Navier-Stokes equations
    is not well understood. Exploiting geometrical properties of transitional channel
    flow we trace turbulence to far lower Reynolds numbers (Re) than previously possible
    and identify the complete path that reversibly links fully turbulent motion to
    an invariant solution. This precursor of turbulence destabilizes rapidly with
    Re, and the accompanying explosive increase in attractor dimension effectively
    marks the transition between deterministic and de facto stochastic dynamics.
acknowledgement: We thank Baofang Song as well as the developers of Channelflow for
  sharing their numerical codes, and Mukund Vasudevan and Holger Kantz for fruitful
  discussions. This work was supported by a grant from the Simons Foundation (662960,
  B. H.).
article_number: '034002'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Chaitanya S
  full_name: Paranjape, Chaitanya S
  id: 3D85B7C4-F248-11E8-B48F-1D18A9856A87
  last_name: Paranjape
- first_name: Gökhan
  full_name: Yalniz, Gökhan
  id: 66E74FA2-D8BF-11E9-8249-8DE2E5697425
  last_name: Yalniz
  orcid: 0000-0002-8490-9312
- first_name: Yohann
  full_name: Duguet, Yohann
  last_name: Duguet
- first_name: Nazmi B
  full_name: Budanur, Nazmi B
  id: 3EA1010E-F248-11E8-B48F-1D18A9856A87
  last_name: Budanur
  orcid: 0000-0003-0423-5010
- first_name: Björn
  full_name: Hof, Björn
  id: 3A374330-F248-11E8-B48F-1D18A9856A87
  last_name: Hof
  orcid: 0000-0003-2057-2754
citation:
  ama: Paranjape CS, Yalniz G, Duguet Y, Budanur NB, Hof B. Direct path from turbulence
    to time-periodic solutions. <i>Physical Review Letters</i>. 2023;131(3). doi:<a
    href="https://doi.org/10.1103/physrevlett.131.034002">10.1103/physrevlett.131.034002</a>
  apa: Paranjape, C. S., Yalniz, G., Duguet, Y., Budanur, N. B., &#38; Hof, B. (2023).
    Direct path from turbulence to time-periodic solutions. <i>Physical Review Letters</i>.
    American Physical Society. <a href="https://doi.org/10.1103/physrevlett.131.034002">https://doi.org/10.1103/physrevlett.131.034002</a>
  chicago: Paranjape, Chaitanya S, Gökhan Yalniz, Yohann Duguet, Nazmi B Budanur,
    and Björn Hof. “Direct Path from Turbulence to Time-Periodic Solutions.” <i>Physical
    Review Letters</i>. American Physical Society, 2023. <a href="https://doi.org/10.1103/physrevlett.131.034002">https://doi.org/10.1103/physrevlett.131.034002</a>.
  ieee: C. S. Paranjape, G. Yalniz, Y. Duguet, N. B. Budanur, and B. Hof, “Direct
    path from turbulence to time-periodic solutions,” <i>Physical Review Letters</i>,
    vol. 131, no. 3. American Physical Society, 2023.
  ista: Paranjape CS, Yalniz G, Duguet Y, Budanur NB, Hof B. 2023. Direct path from
    turbulence to time-periodic solutions. Physical Review Letters. 131(3), 034002.
  mla: Paranjape, Chaitanya S., et al. “Direct Path from Turbulence to Time-Periodic
    Solutions.” <i>Physical Review Letters</i>, vol. 131, no. 3, 034002, American
    Physical Society, 2023, doi:<a href="https://doi.org/10.1103/physrevlett.131.034002">10.1103/physrevlett.131.034002</a>.
  short: C.S. Paranjape, G. Yalniz, Y. Duguet, N.B. Budanur, B. Hof, Physical Review
    Letters 131 (2023).
date_created: 2023-07-24T09:43:59Z
date_published: 2023-07-21T00:00:00Z
date_updated: 2023-12-13T11:40:19Z
day: '21'
department:
- _id: GradSch
- _id: BjHo
doi: 10.1103/physrevlett.131.034002
external_id:
  arxiv:
  - '2306.05098'
  isi:
  - '001052929900004'
intvolume: '       131'
isi: 1
issue: '3'
keyword:
- General Physics and Astronomy
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2306.05098
month: '07'
oa: 1
oa_version: Preprint
project:
- _id: 238598C6-32DE-11EA-91FC-C7463DDC885E
  grant_number: '662960'
  name: 'Revisiting the Turbulence Problem Using Statistical Mechanics: Experimental
    Studies on Transitional and Turbulent Flows'
publication: Physical Review Letters
publication_identifier:
  eissn:
  - 1079-7114
  issn:
  - 0031-9007
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
status: public
title: Direct path from turbulence to time-periodic solutions
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 131
year: '2023'
...
---
_id: '13278'
abstract:
- lang: eng
  text: We present a numerical analysis of spin-1/2 fermions in a one-dimensional
    harmonic potential in the presence of a magnetic point-like impurity at the center
    of the trap. The model represents a few-body analogue of a magnetic impurity in
    the vicinity of an s-wave superconductor. Already for a few particles we find
    a ground-state level crossing between sectors with different fermion parities.
    We interpret this crossing as a few-body precursor of a quantum phase transition,
    which occurs when the impurity "breaks" a Cooper pair. This picture is further
    corroborated by analyzing density-density correlations in momentum space. Finally,
    we discuss how the system may be realized with existing cold-atoms platforms.
article_number: '006'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Lukas
  full_name: Rammelmüller, Lukas
  last_name: Rammelmüller
- first_name: David
  full_name: Huber, David
  last_name: Huber
- first_name: Matija
  full_name: Čufar, Matija
  last_name: Čufar
- first_name: Joachim
  full_name: Brand, Joachim
  last_name: Brand
- first_name: Hans-Werner
  full_name: Hammer, Hans-Werner
  last_name: Hammer
- first_name: Artem
  full_name: Volosniev, Artem
  id: 37D278BC-F248-11E8-B48F-1D18A9856A87
  last_name: Volosniev
  orcid: 0000-0003-0393-5525
citation:
  ama: Rammelmüller L, Huber D, Čufar M, Brand J, Hammer H-W, Volosniev A. Magnetic
    impurity in a one-dimensional few-fermion system. <i>SciPost Physics</i>. 2023;14(1).
    doi:<a href="https://doi.org/10.21468/scipostphys.14.1.006">10.21468/scipostphys.14.1.006</a>
  apa: Rammelmüller, L., Huber, D., Čufar, M., Brand, J., Hammer, H.-W., &#38; Volosniev,
    A. (2023). Magnetic impurity in a one-dimensional few-fermion system. <i>SciPost
    Physics</i>. SciPost Foundation. <a href="https://doi.org/10.21468/scipostphys.14.1.006">https://doi.org/10.21468/scipostphys.14.1.006</a>
  chicago: Rammelmüller, Lukas, David Huber, Matija Čufar, Joachim Brand, Hans-Werner
    Hammer, and Artem Volosniev. “Magnetic Impurity in a One-Dimensional Few-Fermion
    System.” <i>SciPost Physics</i>. SciPost Foundation, 2023. <a href="https://doi.org/10.21468/scipostphys.14.1.006">https://doi.org/10.21468/scipostphys.14.1.006</a>.
  ieee: L. Rammelmüller, D. Huber, M. Čufar, J. Brand, H.-W. Hammer, and A. Volosniev,
    “Magnetic impurity in a one-dimensional few-fermion system,” <i>SciPost Physics</i>,
    vol. 14, no. 1. SciPost Foundation, 2023.
  ista: Rammelmüller L, Huber D, Čufar M, Brand J, Hammer H-W, Volosniev A. 2023.
    Magnetic impurity in a one-dimensional few-fermion system. SciPost Physics. 14(1),
    006.
  mla: Rammelmüller, Lukas, et al. “Magnetic Impurity in a One-Dimensional Few-Fermion
    System.” <i>SciPost Physics</i>, vol. 14, no. 1, 006, SciPost Foundation, 2023,
    doi:<a href="https://doi.org/10.21468/scipostphys.14.1.006">10.21468/scipostphys.14.1.006</a>.
  short: L. Rammelmüller, D. Huber, M. Čufar, J. Brand, H.-W. Hammer, A. Volosniev,
    SciPost Physics 14 (2023).
date_created: 2023-07-24T10:48:23Z
date_published: 2023-01-24T00:00:00Z
date_updated: 2023-12-13T11:39:32Z
day: '24'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.21468/scipostphys.14.1.006
external_id:
  arxiv:
  - '2204.01606'
  isi:
  - '001000325800008'
file:
- access_level: open_access
  checksum: ffdb70b9ae7aa45ea4ea6096ecbd6431
  content_type: application/pdf
  creator: dernst
  date_created: 2023-07-31T08:44:38Z
  date_updated: 2023-07-31T08:44:38Z
  file_id: '13328'
  file_name: 2023_SciPostPhysics_Rammelmueller.pdf
  file_size: 1163444
  relation: main_file
  success: 1
file_date_updated: 2023-07-31T08:44:38Z
has_accepted_license: '1'
intvolume: '        14'
isi: 1
issue: '1'
keyword:
- General Physics and Astronomy
language:
- iso: eng
month: '01'
oa: 1
oa_version: Published Version
publication: SciPost Physics
publication_identifier:
  issn:
  - 2542-4653
publication_status: published
publisher: SciPost Foundation
quality_controlled: '1'
scopus_import: '1'
status: public
title: Magnetic impurity in a one-dimensional few-fermion system
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 14
year: '2023'
...
---
_id: '13346'
abstract:
- lang: eng
  text: The self-assembly of nanoparticles driven by small molecules or ions may produce
    colloidal superlattices with features and properties reminiscent of those of metals
    or semiconductors. However, to what extent the properties of such supramolecular
    crystals actually resemble those of atomic materials often remains unclear. Here,
    we present coarse-grained molecular simulations explicitly demonstrating how a
    behavior evocative of that of semiconductors may emerge in a colloidal superlattice.
    As a case study, we focus on gold nanoparticles bearing positively charged groups
    that self-assemble into FCC crystals via mediation by citrate counterions. In
    silico ohmic experiments show how the dynamically diverse behavior of the ions
    in different superlattice domains allows the opening of conductive ionic gates
    above certain levels of applied electric fields. The observed binary conductive/nonconductive
    behavior is reminiscent of that of conventional semiconductors, while, at a supramolecular
    level, crossing the “band gap” requires a sufficient electrostatic stimulus to
    break the intermolecular interactions and make ions diffuse throughout the superlattice’s
    cavities.
article_processing_charge: No
article_type: original
author:
- first_name: Chiara
  full_name: Lionello, Chiara
  last_name: Lionello
- first_name: Claudio
  full_name: Perego, Claudio
  last_name: Perego
- first_name: Andrea
  full_name: Gardin, Andrea
  last_name: Gardin
- first_name: Rafal
  full_name: Klajn, Rafal
  id: 8e84690e-1e48-11ed-a02b-a1e6fb8bb53b
  last_name: Klajn
- first_name: Giovanni M.
  full_name: Pavan, Giovanni M.
  last_name: Pavan
citation:
  ama: Lionello C, Perego C, Gardin A, Klajn R, Pavan GM. Supramolecular semiconductivity
    through emerging ionic gates in ion–nanoparticle superlattices. <i>ACS Nano</i>.
    2023;17(1):275-287. doi:<a href="https://doi.org/10.1021/acsnano.2c07558">10.1021/acsnano.2c07558</a>
  apa: Lionello, C., Perego, C., Gardin, A., Klajn, R., &#38; Pavan, G. M. (2023).
    Supramolecular semiconductivity through emerging ionic gates in ion–nanoparticle
    superlattices. <i>ACS Nano</i>. American Chemical Society. <a href="https://doi.org/10.1021/acsnano.2c07558">https://doi.org/10.1021/acsnano.2c07558</a>
  chicago: Lionello, Chiara, Claudio Perego, Andrea Gardin, Rafal Klajn, and Giovanni
    M. Pavan. “Supramolecular Semiconductivity through Emerging Ionic Gates in Ion–Nanoparticle
    Superlattices.” <i>ACS Nano</i>. American Chemical Society, 2023. <a href="https://doi.org/10.1021/acsnano.2c07558">https://doi.org/10.1021/acsnano.2c07558</a>.
  ieee: C. Lionello, C. Perego, A. Gardin, R. Klajn, and G. M. Pavan, “Supramolecular
    semiconductivity through emerging ionic gates in ion–nanoparticle superlattices,”
    <i>ACS Nano</i>, vol. 17, no. 1. American Chemical Society, pp. 275–287, 2023.
  ista: Lionello C, Perego C, Gardin A, Klajn R, Pavan GM. 2023. Supramolecular semiconductivity
    through emerging ionic gates in ion–nanoparticle superlattices. ACS Nano. 17(1),
    275–287.
  mla: Lionello, Chiara, et al. “Supramolecular Semiconductivity through Emerging
    Ionic Gates in Ion–Nanoparticle Superlattices.” <i>ACS Nano</i>, vol. 17, no.
    1, American Chemical Society, 2023, pp. 275–87, doi:<a href="https://doi.org/10.1021/acsnano.2c07558">10.1021/acsnano.2c07558</a>.
  short: C. Lionello, C. Perego, A. Gardin, R. Klajn, G.M. Pavan, ACS Nano 17 (2023)
    275–287.
date_created: 2023-08-01T09:30:29Z
date_published: 2023-01-10T00:00:00Z
date_updated: 2023-08-02T06:51:15Z
day: '10'
doi: 10.1021/acsnano.2c07558
extern: '1'
intvolume: '        17'
issue: '1'
keyword:
- General Physics and Astronomy
- General Engineering
- General Materials Science
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1021/acsnano.2c07558
month: '01'
oa: 1
oa_version: Published Version
page: 275-287
publication: ACS Nano
publication_identifier:
  eissn:
  - 1936-086X
  issn:
  - 1936-0851
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Supramolecular semiconductivity through emerging ionic gates in ion–nanoparticle
  superlattices
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 17
year: '2023'
...
---
_id: '13443'
abstract:
- lang: eng
  text: 'The ages of solar-like stars have been at the center of many studies such
    as exoplanet characterization or Galactic-archeology. While ages are usually computed
    from stellar evolution models, relations linking ages to other stellar properties,
    such as rotation and magnetic activity, have been investigated. With the large
    catalog of 55,232 rotation periods, Prot, and photometric magnetic activity index,
    Sph from Kepler data, we have the opportunity to look for such magneto-gyro-chronology
    relations. Stellar ages are obtained with two stellar evolution codes that include
    treatment of angular momentum evolution, hence using Prot as input in addition
    to classical atmospheric parameters. We explore two different ways of predicting
    stellar ages on three subsamples with spectroscopic observations: solar analogs,
    late-F and G dwarfs, and K dwarfs. We first perform a Bayesian analysis to derive
    relations between Sph and ages between 1 and 5 Gyr, and other stellar properties.
    For late-F and G dwarfs, and K dwarfs, the multivariate regression favors the
    model with Prot and Sph with median differences of 0.1% and 0.2%, respectively.
    We also apply Machine Learning techniques with a Random Forest algorithm to predict
    ages up to 14 Gyr with the same set of input parameters. For late-F, G and K dwarfs
    together, predicted ages are on average within 5.3% of the model ages and improve
    to 3.1% when including Prot. These are very promising results for a quick age
    estimation for solar-like stars with photometric observations, especially with
    current and future space missions.'
acknowledgement: 'This paper includes data collected by the Kepler mission and obtained
  from the MAST data archive at the Space Telescope Science Institute (STScI). Funding
  for the Kepler mission is provided by the NASA Science Mission Directorate. STScI
  is operated by the Association of Universities for Research in Astronomy, Inc.,
  under NASA contract NAS 5–26555. We acknowledge that this research was supported
  in part by the National Science Foundation under grant No. NSF PHY-1748958. S.M.
  acknowledges support from the Spanish Ministry of Science and Innovation (MICINN)
  with the Ramón y Cajal fellowship No. RYC-2015-17697, the grant No. PID2019-107061GB-C66,
  and through AEI under the Severo Ochoa Centres of Excellence Programme 2020–2023
  (CEX2019-000920-S). S.M. and D.G.R. acknowledge support from the Spanish Ministry
  of Science and Innovation (MICINN) with the grant No. PID2019-107187GB-I00. Z.R.C.
  acknowledges support from National Aeronautics and Space Administration via the
  TESS Guest Investigator Program (grant No. 80NSSC18K18584). The work presented here
  was partially supported by the NASA grant NNX17AF27G. A.R.G.S. acknowledges the
  support by FCT through national funds and by FEDER through COMPETE2020 by the following
  grants: UIDB/04434/2020 and UIDP/04434/2020. A.R.G.S. is supported by FCT through
  the work contract No. 2020.02480.CEECIND/CP1631/CT0001. R.A.G., L.A., and S.N.B.
  acknowledge the support from PLATO and GOLF CNES grants. S.N.B. acknowledges support
  from PLATO ASI-INAF agreement No. 2015-019-R.1-2018.'
article_number: '131'
article_processing_charge: Yes
article_type: original
author:
- first_name: Savita
  full_name: Mathur, Savita
  last_name: Mathur
- first_name: Zachary R.
  full_name: Claytor, Zachary R.
  last_name: Claytor
- first_name: Ângela R. G.
  full_name: Santos, Ângela R. G.
  last_name: Santos
- first_name: Rafael A.
  full_name: García, Rafael A.
  last_name: García
- first_name: Louis
  full_name: Amard, Louis
  last_name: Amard
- first_name: Lisa Annabelle
  full_name: Bugnet, Lisa Annabelle
  id: d9edb345-f866-11ec-9b37-d119b5234501
  last_name: Bugnet
  orcid: 0000-0003-0142-4000
- first_name: Enrico
  full_name: Corsaro, Enrico
  last_name: Corsaro
- first_name: Alfio
  full_name: Bonanno, Alfio
  last_name: Bonanno
- first_name: Sylvain N.
  full_name: Breton, Sylvain N.
  last_name: Breton
- first_name: Diego
  full_name: Godoy-Rivera, Diego
  last_name: Godoy-Rivera
- first_name: Marc H.
  full_name: Pinsonneault, Marc H.
  last_name: Pinsonneault
- first_name: Jennifer
  full_name: van Saders, Jennifer
  last_name: van Saders
citation:
  ama: Mathur S, Claytor ZR, Santos ÂRG, et al. Magnetic activity evolution of solar-like
    stars. I. Sph–age relation derived from Kepler observations. <i>The Astrophysical
    Journal</i>. 2023;952(2). doi:<a href="https://doi.org/10.3847/1538-4357/acd118">10.3847/1538-4357/acd118</a>
  apa: Mathur, S., Claytor, Z. R., Santos, Â. R. G., García, R. A., Amard, L., Bugnet,
    L. A., … van Saders, J. (2023). Magnetic activity evolution of solar-like stars.
    I. Sph–age relation derived from Kepler observations. <i>The Astrophysical Journal</i>.
    American Astronomical Society. <a href="https://doi.org/10.3847/1538-4357/acd118">https://doi.org/10.3847/1538-4357/acd118</a>
  chicago: Mathur, Savita, Zachary R. Claytor, Ângela R. G. Santos, Rafael A. García,
    Louis Amard, Lisa Annabelle Bugnet, Enrico Corsaro, et al. “Magnetic Activity
    Evolution of Solar-like Stars. I. Sph–Age Relation Derived from Kepler Observations.”
    <i>The Astrophysical Journal</i>. American Astronomical Society, 2023. <a href="https://doi.org/10.3847/1538-4357/acd118">https://doi.org/10.3847/1538-4357/acd118</a>.
  ieee: S. Mathur <i>et al.</i>, “Magnetic activity evolution of solar-like stars.
    I. Sph–age relation derived from Kepler observations,” <i>The Astrophysical Journal</i>,
    vol. 952, no. 2. American Astronomical Society, 2023.
  ista: Mathur S, Claytor ZR, Santos ÂRG, García RA, Amard L, Bugnet LA, Corsaro E,
    Bonanno A, Breton SN, Godoy-Rivera D, Pinsonneault MH, van Saders J. 2023. Magnetic
    activity evolution of solar-like stars. I. Sph–age relation derived from Kepler
    observations. The Astrophysical Journal. 952(2), 131.
  mla: Mathur, Savita, et al. “Magnetic Activity Evolution of Solar-like Stars. I.
    Sph–Age Relation Derived from Kepler Observations.” <i>The Astrophysical Journal</i>,
    vol. 952, no. 2, 131, American Astronomical Society, 2023, doi:<a href="https://doi.org/10.3847/1538-4357/acd118">10.3847/1538-4357/acd118</a>.
  short: S. Mathur, Z.R. Claytor, Â.R.G. Santos, R.A. García, L. Amard, L.A. Bugnet,
    E. Corsaro, A. Bonanno, S.N. Breton, D. Godoy-Rivera, M.H. Pinsonneault, J. van
    Saders, The Astrophysical Journal 952 (2023).
date_created: 2023-08-01T14:19:16Z
date_published: 2023-08-01T00:00:00Z
date_updated: 2023-12-13T12:00:15Z
day: '01'
ddc:
- '520'
department:
- _id: LiBu
doi: 10.3847/1538-4357/acd118
external_id:
  isi:
  - '001034185700001'
file:
- access_level: open_access
  checksum: f12452834d7ed6748dbf5ace18af4723
  content_type: application/pdf
  creator: dernst
  date_created: 2023-08-02T07:42:26Z
  date_updated: 2023-08-02T07:42:26Z
  file_id: '13448'
  file_name: 2023_AstrophysicalJour_Mathur.pdf
  file_size: 4192386
  relation: main_file
  success: 1
file_date_updated: 2023-08-02T07:42:26Z
has_accepted_license: '1'
intvolume: '       952'
isi: 1
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
month: '08'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
  eissn:
  - 1538-4357
  issn:
  - 0004-637X
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
status: public
title: Magnetic activity evolution of solar-like stars. I. Sph–age relation derived
  from Kepler observations
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 952
year: '2023'
...
---
_id: '13449'
abstract:
- lang: eng
  text: Stars strongly impact their environment, and shape structures on all scales
    throughout the universe, in a process known as "feedback." Due to the complexity
    of both stellar evolution and the physics of larger astrophysical structures,
    there remain many unanswered questions about how feedback operates and what we
    can learn about stars by studying their imprint on the wider universe. In this
    white paper, we summarize discussions from the Lorentz Center meeting "Bringing
    Stellar Evolution and Feedback Together" in 2022 April and identify key areas
    where further dialog can bring about radical changes in how we view the relationship
    between stars and the universe they live in.
article_number: '021001'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Sam
  full_name: Geen, Sam
  last_name: Geen
- first_name: Poojan
  full_name: Agrawal, Poojan
  last_name: Agrawal
- first_name: Paul A.
  full_name: Crowther, Paul A.
  last_name: Crowther
- first_name: B. W.
  full_name: Keller, B. W.
  last_name: Keller
- first_name: Alex
  full_name: de Koter, Alex
  last_name: de Koter
- first_name: Zsolt
  full_name: Keszthelyi, Zsolt
  last_name: Keszthelyi
- first_name: Freeke
  full_name: van de Voort, Freeke
  last_name: van de Voort
- first_name: Ahmad A.
  full_name: Ali, Ahmad A.
  last_name: Ali
- first_name: Frank
  full_name: Backs, Frank
  last_name: Backs
- first_name: Lars
  full_name: Bonne, Lars
  last_name: Bonne
- first_name: Vittoria
  full_name: Brugaletta, Vittoria
  last_name: Brugaletta
- first_name: Annelotte
  full_name: Derkink, Annelotte
  last_name: Derkink
- first_name: Sylvia
  full_name: Ekström, Sylvia
  last_name: Ekström
- first_name: Yvonne A.
  full_name: Fichtner, Yvonne A.
  last_name: Fichtner
- first_name: Luca
  full_name: Grassitelli, Luca
  last_name: Grassitelli
- first_name: Ylva Louise Linsdotter
  full_name: Götberg, Ylva Louise Linsdotter
  id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
  last_name: Götberg
  orcid: 0000-0002-6960-6911
- first_name: Erin R.
  full_name: Higgins, Erin R.
  last_name: Higgins
- first_name: Eva
  full_name: Laplace, Eva
  last_name: Laplace
- first_name: Kong
  full_name: You Liow, Kong
  last_name: You Liow
- first_name: Marta
  full_name: Lorenzo, Marta
  last_name: Lorenzo
- first_name: Anna F.
  full_name: McLeod, Anna F.
  last_name: McLeod
- first_name: Georges
  full_name: Meynet, Georges
  last_name: Meynet
- first_name: Megan
  full_name: Newsome, Megan
  last_name: Newsome
- first_name: G.
  full_name: André Oliva, G.
  last_name: André Oliva
- first_name: Varsha
  full_name: Ramachandran, Varsha
  last_name: Ramachandran
- first_name: Martin P.
  full_name: Rey, Martin P.
  last_name: Rey
- first_name: Steven
  full_name: Rieder, Steven
  last_name: Rieder
- first_name: Emilio
  full_name: Romano-Díaz, Emilio
  last_name: Romano-Díaz
- first_name: Gautham
  full_name: Sabhahit, Gautham
  last_name: Sabhahit
- first_name: Andreas A. C.
  full_name: Sander, Andreas A. C.
  last_name: Sander
- first_name: Rafia
  full_name: Sarwar, Rafia
  last_name: Sarwar
- first_name: Hanno
  full_name: Stinshoff, Hanno
  last_name: Stinshoff
- first_name: Mitchel
  full_name: Stoop, Mitchel
  last_name: Stoop
- first_name: Dorottya
  full_name: Szécsi, Dorottya
  last_name: Szécsi
- first_name: Maxime
  full_name: Trebitsch, Maxime
  last_name: Trebitsch
- first_name: Jorick S.
  full_name: Vink, Jorick S.
  last_name: Vink
- first_name: Ethan
  full_name: Winch, Ethan
  last_name: Winch
citation:
  ama: 'Geen S, Agrawal P, Crowther PA, et al. Bringing stellar evolution and feedback
    together: Summary of proposals from the Lorentz Center workshop. <i>Publications
    of the Astronomical Society of the Pacific</i>. 2023;135(1044). doi:<a href="https://doi.org/10.1088/1538-3873/acb6b5">10.1088/1538-3873/acb6b5</a>'
  apa: 'Geen, S., Agrawal, P., Crowther, P. A., Keller, B. W., de Koter, A., Keszthelyi,
    Z., … Winch, E. (2023). Bringing stellar evolution and feedback together: Summary
    of proposals from the Lorentz Center workshop. <i>Publications of the Astronomical
    Society of the Pacific</i>. IOP Publishing. <a href="https://doi.org/10.1088/1538-3873/acb6b5">https://doi.org/10.1088/1538-3873/acb6b5</a>'
  chicago: 'Geen, Sam, Poojan Agrawal, Paul A. Crowther, B. W. Keller, Alex de Koter,
    Zsolt Keszthelyi, Freeke van de Voort, et al. “Bringing Stellar Evolution and
    Feedback Together: Summary of Proposals from the Lorentz Center Workshop.” <i>Publications
    of the Astronomical Society of the Pacific</i>. IOP Publishing, 2023. <a href="https://doi.org/10.1088/1538-3873/acb6b5">https://doi.org/10.1088/1538-3873/acb6b5</a>.'
  ieee: 'S. Geen <i>et al.</i>, “Bringing stellar evolution and feedback together:
    Summary of proposals from the Lorentz Center workshop,” <i>Publications of the
    Astronomical Society of the Pacific</i>, vol. 135, no. 1044. IOP Publishing, 2023.'
  ista: 'Geen S, Agrawal P, Crowther PA, Keller BW, de Koter A, Keszthelyi Z, van
    de Voort F, Ali AA, Backs F, Bonne L, Brugaletta V, Derkink A, Ekström S, Fichtner
    YA, Grassitelli L, Götberg YLL, Higgins ER, Laplace E, You Liow K, Lorenzo M,
    McLeod AF, Meynet G, Newsome M, André Oliva G, Ramachandran V, Rey MP, Rieder
    S, Romano-Díaz E, Sabhahit G, Sander AAC, Sarwar R, Stinshoff H, Stoop M, Szécsi
    D, Trebitsch M, Vink JS, Winch E. 2023. Bringing stellar evolution and feedback
    together: Summary of proposals from the Lorentz Center workshop. Publications
    of the Astronomical Society of the Pacific. 135(1044), 021001.'
  mla: 'Geen, Sam, et al. “Bringing Stellar Evolution and Feedback Together: Summary
    of Proposals from the Lorentz Center Workshop.” <i>Publications of the Astronomical
    Society of the Pacific</i>, vol. 135, no. 1044, 021001, IOP Publishing, 2023,
    doi:<a href="https://doi.org/10.1088/1538-3873/acb6b5">10.1088/1538-3873/acb6b5</a>.'
  short: S. Geen, P. Agrawal, P.A. Crowther, B.W. Keller, A. de Koter, Z. Keszthelyi,
    F. van de Voort, A.A. Ali, F. Backs, L. Bonne, V. Brugaletta, A. Derkink, S. Ekström,
    Y.A. Fichtner, L. Grassitelli, Y.L.L. Götberg, E.R. Higgins, E. Laplace, K. You
    Liow, M. Lorenzo, A.F. McLeod, G. Meynet, M. Newsome, G. André Oliva, V. Ramachandran,
    M.P. Rey, S. Rieder, E. Romano-Díaz, G. Sabhahit, A.A.C. Sander, R. Sarwar, H.
    Stinshoff, M. Stoop, D. Szécsi, M. Trebitsch, J.S. Vink, E. Winch, Publications
    of the Astronomical Society of the Pacific 135 (2023).
date_created: 2023-08-03T10:09:57Z
date_published: 2023-03-09T00:00:00Z
date_updated: 2023-08-21T12:09:14Z
day: '09'
doi: 10.1088/1538-3873/acb6b5
extern: '1'
external_id:
  arxiv:
  - '2301.13611'
intvolume: '       135'
issue: '1044'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1088/1538-3873/acb6b5
month: '03'
oa: 1
oa_version: Published Version
publication: Publications of the Astronomical Society of the Pacific
publication_identifier:
  eissn:
  - 1538-3873
  issn:
  - 0004-6280
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Bringing stellar evolution and feedback together: Summary of proposals from
  the Lorentz Center workshop'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 135
year: '2023'
...
---
_id: '13450'
abstract:
- lang: eng
  text: In previous work, we identified a population of 38 cool and luminous variable
    stars in the Magellanic Clouds and examined 11 in detail in order to classify
    them as either Thorne–Żytkow objects (TŻOs; red supergiants with a neutron star
    cores) or super-asymptotic giant branch (sAGB) stars (the most massive stars that
    will not undergo core collapse). This population includes HV 2112, a peculiar
    star previously considered in other works to be either a TŻO or high-mass asymptotic
    giant branch (AGB) star. Here we continue this investigation, using the kinematic
    and radio environments and local star formation history of these stars to place
    constraints on the age of the progenitor systems and the presence of past supernovae.
    These stars are not associated with regions of recent star formation, and we find
    no evidence of past supernovae at their locations. Finally, we also assess the
    presence of heavy elements and lithium in their spectra compared to red supergiants.
    We find strong absorption in Li and s-process elements compared to RSGs in most
    of the sample, consistent with sAGB nucleosynthesis, while HV 2112 shows additional
    strong lines associated with TŻO nucleosynthesis. Coupled with our previous mass
    estimates, the results are consistent with the stars being massive (∼4–6.5 M⊙)
    or sAGB (∼6.5–12 M⊙) stars in the thermally pulsing phase, providing crucial observations
    of the transition between low- and high-mass stellar populations. HV 2112 is more
    ambiguous; it could either be a maximally massive sAGB star, or a TŻO if the minimum
    mass for stability extends down to ≲13 M⊙.
article_number: '18'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Anna J. G.
  full_name: O‘Grady, Anna J. G.
  last_name: O‘Grady
- first_name: Maria R.
  full_name: Drout, Maria R.
  last_name: Drout
- first_name: B. M.
  full_name: Gaensler, B. M.
  last_name: Gaensler
- first_name: C. S.
  full_name: Kochanek, C. S.
  last_name: Kochanek
- first_name: Kathryn F.
  full_name: Neugent, Kathryn F.
  last_name: Neugent
- first_name: Carolyn L.
  full_name: Doherty, Carolyn L.
  last_name: Doherty
- first_name: Joshua S.
  full_name: Speagle, Joshua S.
  last_name: Speagle
- first_name: B. J.
  full_name: Shappee, B. J.
  last_name: Shappee
- first_name: Michael
  full_name: Rauch, Michael
  last_name: Rauch
- first_name: Ylva Louise Linsdotter
  full_name: Götberg, Ylva Louise Linsdotter
  id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
  last_name: Götberg
  orcid: 0000-0002-6960-6911
- first_name: Bethany
  full_name: Ludwig, Bethany
  last_name: Ludwig
- first_name: Todd A.
  full_name: Thompson, Todd A.
  last_name: Thompson
citation:
  ama: O‘Grady AJG, Drout MR, Gaensler BM, et al. Cool, luminous, and highly variable
    stars in the Magellanic Clouds. II. Spectroscopic and environmental analysis of
    Thorne–Żytkow object and super-AGB star candidates. <i>The Astrophysical Journal</i>.
    2023;943(1). doi:<a href="https://doi.org/10.3847/1538-4357/aca655">10.3847/1538-4357/aca655</a>
  apa: O‘Grady, A. J. G., Drout, M. R., Gaensler, B. M., Kochanek, C. S., Neugent,
    K. F., Doherty, C. L., … Thompson, T. A. (2023). Cool, luminous, and highly variable
    stars in the Magellanic Clouds. II. Spectroscopic and environmental analysis of
    Thorne–Żytkow object and super-AGB star candidates. <i>The Astrophysical Journal</i>.
    American Astronomical Society. <a href="https://doi.org/10.3847/1538-4357/aca655">https://doi.org/10.3847/1538-4357/aca655</a>
  chicago: O‘Grady, Anna J. G., Maria R. Drout, B. M. Gaensler, C. S. Kochanek, Kathryn
    F. Neugent, Carolyn L. Doherty, Joshua S. Speagle, et al. “Cool, Luminous, and
    Highly Variable Stars in the Magellanic Clouds. II. Spectroscopic and Environmental
    Analysis of Thorne–Żytkow Object and Super-AGB Star Candidates.” <i>The Astrophysical
    Journal</i>. American Astronomical Society, 2023. <a href="https://doi.org/10.3847/1538-4357/aca655">https://doi.org/10.3847/1538-4357/aca655</a>.
  ieee: A. J. G. O‘Grady <i>et al.</i>, “Cool, luminous, and highly variable stars
    in the Magellanic Clouds. II. Spectroscopic and environmental analysis of Thorne–Żytkow
    object and super-AGB star candidates,” <i>The Astrophysical Journal</i>, vol.
    943, no. 1. American Astronomical Society, 2023.
  ista: O‘Grady AJG, Drout MR, Gaensler BM, Kochanek CS, Neugent KF, Doherty CL, Speagle
    JS, Shappee BJ, Rauch M, Götberg YLL, Ludwig B, Thompson TA. 2023. Cool, luminous,
    and highly variable stars in the Magellanic Clouds. II. Spectroscopic and environmental
    analysis of Thorne–Żytkow object and super-AGB star candidates. The Astrophysical
    Journal. 943(1), 18.
  mla: O‘Grady, Anna J. G., et al. “Cool, Luminous, and Highly Variable Stars in the
    Magellanic Clouds. II. Spectroscopic and Environmental Analysis of Thorne–Żytkow
    Object and Super-AGB Star Candidates.” <i>The Astrophysical Journal</i>, vol.
    943, no. 1, 18, American Astronomical Society, 2023, doi:<a href="https://doi.org/10.3847/1538-4357/aca655">10.3847/1538-4357/aca655</a>.
  short: A.J.G. O‘Grady, M.R. Drout, B.M. Gaensler, C.S. Kochanek, K.F. Neugent, C.L.
    Doherty, J.S. Speagle, B.J. Shappee, M. Rauch, Y.L.L. Götberg, B. Ludwig, T.A.
    Thompson, The Astrophysical Journal 943 (2023).
date_created: 2023-08-03T10:10:12Z
date_published: 2023-01-20T00:00:00Z
date_updated: 2023-08-21T12:07:05Z
day: '20'
doi: 10.3847/1538-4357/aca655
extern: '1'
external_id:
  arxiv:
  - '2211.12438'
intvolume: '       943'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.3847/1538-4357/aca655
month: '01'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
  eissn:
  - 1538-4357
  issn:
  - 0004-637X
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Cool, luminous, and highly variable stars in the Magellanic Clouds. II. Spectroscopic
  and environmental analysis of Thorne–Żytkow object and super-AGB star candidates
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 943
year: '2023'
...
---
_id: '13989'
abstract:
- lang: eng
  text: Characterizing and controlling entanglement in quantum materials is crucial
    for the development of next-generation quantum technologies. However, defining
    a quantifiable figure of merit for entanglement in macroscopic solids is theoretically
    and experimentally challenging. At equilibrium the presence of entanglement can
    be diagnosed by extracting entanglement witnesses from spectroscopic observables
    and a nonequilibrium extension of this method could lead to the discovery of novel
    dynamical phenomena. Here, we propose a systematic approach to quantify the time-dependent
    quantum Fisher information and entanglement depth of transient states of quantum
    materials with time-resolved resonant inelastic x-ray scattering. Using a quarter-filled
    extended Hubbard model as an example, we benchmark the efficiency of this approach
    and predict a light-enhanced many-body entanglement due to the proximity to a
    phase boundary. Our work sets the stage for experimentally witnessing and controlling
    entanglement in light-driven quantum materials via ultrafast spectroscopic measurements.
article_number: '3512'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Jordyn
  full_name: Hales, Jordyn
  last_name: Hales
- first_name: Utkarsh
  full_name: Bajpai, Utkarsh
  last_name: Bajpai
- first_name: Tongtong
  full_name: Liu, Tongtong
  last_name: Liu
- first_name: Denitsa Rangelova
  full_name: Baykusheva, Denitsa Rangelova
  id: 71b4d059-2a03-11ee-914d-dfa3beed6530
  last_name: Baykusheva
- first_name: Mingda
  full_name: Li, Mingda
  last_name: Li
- first_name: Matteo
  full_name: Mitrano, Matteo
  last_name: Mitrano
- first_name: Yao
  full_name: Wang, Yao
  last_name: Wang
citation:
  ama: Hales J, Bajpai U, Liu T, et al. Witnessing light-driven entanglement using
    time-resolved resonant inelastic X-ray scattering. <i>Nature Communications</i>.
    2023;14. doi:<a href="https://doi.org/10.1038/s41467-023-38540-3">10.1038/s41467-023-38540-3</a>
  apa: Hales, J., Bajpai, U., Liu, T., Baykusheva, D. R., Li, M., Mitrano, M., &#38;
    Wang, Y. (2023). Witnessing light-driven entanglement using time-resolved resonant
    inelastic X-ray scattering. <i>Nature Communications</i>. Springer Nature. <a
    href="https://doi.org/10.1038/s41467-023-38540-3">https://doi.org/10.1038/s41467-023-38540-3</a>
  chicago: Hales, Jordyn, Utkarsh Bajpai, Tongtong Liu, Denitsa Rangelova Baykusheva,
    Mingda Li, Matteo Mitrano, and Yao Wang. “Witnessing Light-Driven Entanglement
    Using Time-Resolved Resonant Inelastic X-Ray Scattering.” <i>Nature Communications</i>.
    Springer Nature, 2023. <a href="https://doi.org/10.1038/s41467-023-38540-3">https://doi.org/10.1038/s41467-023-38540-3</a>.
  ieee: J. Hales <i>et al.</i>, “Witnessing light-driven entanglement using time-resolved
    resonant inelastic X-ray scattering,” <i>Nature Communications</i>, vol. 14. Springer
    Nature, 2023.
  ista: Hales J, Bajpai U, Liu T, Baykusheva DR, Li M, Mitrano M, Wang Y. 2023. Witnessing
    light-driven entanglement using time-resolved resonant inelastic X-ray scattering.
    Nature Communications. 14, 3512.
  mla: Hales, Jordyn, et al. “Witnessing Light-Driven Entanglement Using Time-Resolved
    Resonant Inelastic X-Ray Scattering.” <i>Nature Communications</i>, vol. 14, 3512,
    Springer Nature, 2023, doi:<a href="https://doi.org/10.1038/s41467-023-38540-3">10.1038/s41467-023-38540-3</a>.
  short: J. Hales, U. Bajpai, T. Liu, D.R. Baykusheva, M. Li, M. Mitrano, Y. Wang,
    Nature Communications 14 (2023).
date_created: 2023-08-09T13:06:59Z
date_published: 2023-06-14T00:00:00Z
date_updated: 2023-08-22T06:50:04Z
day: '14'
doi: 10.1038/s41467-023-38540-3
extern: '1'
external_id:
  arxiv:
  - '2209.02283'
  pmid:
  - '37316515'
intvolume: '        14'
keyword:
- General Physics and Astronomy
- General Biochemistry
- Genetics and Molecular Biology
- General Chemistry
- Multidisciplinary
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1038/s41467-023-38540-3
month: '06'
oa: 1
oa_version: Published Version
pmid: 1
publication: Nature Communications
publication_identifier:
  eissn:
  - 2041-1723
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Witnessing light-driven entanglement using time-resolved resonant inelastic
  X-ray scattering
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 14
year: '2023'
...
---
_id: '13990'
abstract:
- lang: eng
  text: Many-body entanglement in condensed matter systems can be diagnosed from equilibrium
    response functions through the use of entanglement witnesses and operator-specific
    quantum bounds. Here, we investigate the applicability of this approach for detecting
    entangled states in quantum systems driven out of equilibrium. We use a multipartite
    entanglement witness, the quantum Fisher information, to study the dynamics of
    a paradigmatic fermion chain undergoing a time-dependent change of the Coulomb
    interaction. Our results show that the quantum Fisher information is able to witness
    distinct signatures of multipartite entanglement both near and far from equilibrium
    that are robust against decoherence. We discuss implications of these findings
    for probing entanglement in light-driven quantum materials with time-resolved
    optical and x-ray scattering methods.
article_number: '106902'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Denitsa Rangelova
  full_name: Baykusheva, Denitsa Rangelova
  id: 71b4d059-2a03-11ee-914d-dfa3beed6530
  last_name: Baykusheva
- first_name: Mona H.
  full_name: Kalthoff, Mona H.
  last_name: Kalthoff
- first_name: Damian
  full_name: Hofmann, Damian
  last_name: Hofmann
- first_name: Martin
  full_name: Claassen, Martin
  last_name: Claassen
- first_name: Dante M.
  full_name: Kennes, Dante M.
  last_name: Kennes
- first_name: Michael A.
  full_name: Sentef, Michael A.
  last_name: Sentef
- first_name: Matteo
  full_name: Mitrano, Matteo
  last_name: Mitrano
citation:
  ama: Baykusheva DR, Kalthoff MH, Hofmann D, et al. Witnessing nonequilibrium entanglement
    dynamics in a strongly correlated fermionic chain. <i>Physical Review Letters</i>.
    2023;130(10). doi:<a href="https://doi.org/10.1103/physrevlett.130.106902">10.1103/physrevlett.130.106902</a>
  apa: Baykusheva, D. R., Kalthoff, M. H., Hofmann, D., Claassen, M., Kennes, D. M.,
    Sentef, M. A., &#38; Mitrano, M. (2023). Witnessing nonequilibrium entanglement
    dynamics in a strongly correlated fermionic chain. <i>Physical Review Letters</i>.
    American Physical Society. <a href="https://doi.org/10.1103/physrevlett.130.106902">https://doi.org/10.1103/physrevlett.130.106902</a>
  chicago: Baykusheva, Denitsa Rangelova, Mona H. Kalthoff, Damian Hofmann, Martin
    Claassen, Dante M. Kennes, Michael A. Sentef, and Matteo Mitrano. “Witnessing
    Nonequilibrium Entanglement Dynamics in a Strongly Correlated Fermionic Chain.”
    <i>Physical Review Letters</i>. American Physical Society, 2023. <a href="https://doi.org/10.1103/physrevlett.130.106902">https://doi.org/10.1103/physrevlett.130.106902</a>.
  ieee: D. R. Baykusheva <i>et al.</i>, “Witnessing nonequilibrium entanglement dynamics
    in a strongly correlated fermionic chain,” <i>Physical Review Letters</i>, vol.
    130, no. 10. American Physical Society, 2023.
  ista: Baykusheva DR, Kalthoff MH, Hofmann D, Claassen M, Kennes DM, Sentef MA, Mitrano
    M. 2023. Witnessing nonequilibrium entanglement dynamics in a strongly correlated
    fermionic chain. Physical Review Letters. 130(10), 106902.
  mla: Baykusheva, Denitsa Rangelova, et al. “Witnessing Nonequilibrium Entanglement
    Dynamics in a Strongly Correlated Fermionic Chain.” <i>Physical Review Letters</i>,
    vol. 130, no. 10, 106902, American Physical Society, 2023, doi:<a href="https://doi.org/10.1103/physrevlett.130.106902">10.1103/physrevlett.130.106902</a>.
  short: D.R. Baykusheva, M.H. Kalthoff, D. Hofmann, M. Claassen, D.M. Kennes, M.A.
    Sentef, M. Mitrano, Physical Review Letters 130 (2023).
date_created: 2023-08-09T13:07:24Z
date_published: 2023-03-10T00:00:00Z
date_updated: 2023-08-22T07:18:01Z
day: '10'
doi: 10.1103/physrevlett.130.106902
extern: '1'
external_id:
  arxiv:
  - '2209.02081'
  pmid:
  - '36962013'
intvolume: '       130'
issue: '10'
keyword:
- General Physics and Astronomy
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2209.02081
month: '03'
oa: 1
oa_version: Preprint
pmid: 1
publication: Physical Review Letters
publication_identifier:
  eissn:
  - 1079-7114
  issn:
  - 0031-9007
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Witnessing nonequilibrium entanglement dynamics in a strongly correlated fermionic
  chain
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 130
year: '2023'
...
---
_id: '14032'
abstract:
- lang: eng
  text: Arrays of Josephson junctions are governed by a competition between superconductivity
    and repulsive Coulomb interactions, and are expected to exhibit diverging low-temperature
    resistance when interactions exceed a critical level. Here we report a study of
    the transport and microwave response of Josephson arrays with interactions exceeding
    this level. Contrary to expectations, we observe that the array resistance drops
    dramatically as the temperature is decreased—reminiscent of superconducting behaviour—and
    then saturates at low temperature. Applying a magnetic field, we eventually observe
    a transition to a highly resistive regime. These observations can be understood
    within a theoretical picture that accounts for the effect of thermal fluctuations
    on the insulating phase. On the basis of the agreement between experiment and
    theory, we suggest that apparent superconductivity in our Josephson arrays arises
    from melting the zero-temperature insulator.
acknowledged_ssus:
- _id: M-Shop
- _id: NanoFab
acknowledgement: We thank D. Haviland, J. Pekola, C. Ciuti, A. Bubis and A. Shnirman
  for helpful feedback on the paper. This research was supported by the Scientific
  Service Units of IST Austria through resources provided by the MIBA Machine Shop
  and the Nanofabrication Facility. Work supported by the Austrian FWF grant P33692-N
  (S.M., J.S. and A.P.H.), the European Union’s Horizon 2020 Research and Innovation
  programme under the Marie Skłodowska-Curie Grant Agreement No. 754411 (J.S.) and
  a NOMIS foundation research grant (J.M.F. and A.P.H.).
article_processing_charge: Yes (in subscription journal)
article_type: original
author:
- first_name: Soham
  full_name: Mukhopadhyay, Soham
  id: FDE60288-A89D-11E9-947F-1AF6E5697425
  last_name: Mukhopadhyay
- first_name: Jorden L
  full_name: Senior, Jorden L
  id: 5479D234-2D30-11EA-89CC-40953DDC885E
  last_name: Senior
  orcid: 0000-0002-0672-9295
- first_name: Jaime
  full_name: Saez Mollejo, Jaime
  id: e0390f72-f6e0-11ea-865d-862393336714
  last_name: Saez Mollejo
- first_name: Denise
  full_name: Puglia, Denise
  id: 4D495994-AE37-11E9-AC72-31CAE5697425
  last_name: Puglia
  orcid: 0000-0003-1144-2763
- first_name: Martin
  full_name: Zemlicka, Martin
  id: 2DCF8DE6-F248-11E8-B48F-1D18A9856A87
  last_name: Zemlicka
- first_name: Johannes M
  full_name: Fink, Johannes M
  id: 4B591CBA-F248-11E8-B48F-1D18A9856A87
  last_name: Fink
  orcid: 0000-0001-8112-028X
- first_name: Andrew P
  full_name: Higginbotham, Andrew P
  id: 4AD6785A-F248-11E8-B48F-1D18A9856A87
  last_name: Higginbotham
  orcid: 0000-0003-2607-2363
citation:
  ama: Mukhopadhyay S, Senior JL, Saez Mollejo J, et al. Superconductivity from a
    melted insulator in Josephson junction arrays. <i>Nature Physics</i>. 2023;19:1630-1635.
    doi:<a href="https://doi.org/10.1038/s41567-023-02161-w">10.1038/s41567-023-02161-w</a>
  apa: Mukhopadhyay, S., Senior, J. L., Saez Mollejo, J., Puglia, D., Zemlicka, M.,
    Fink, J. M., &#38; Higginbotham, A. P. (2023). Superconductivity from a melted
    insulator in Josephson junction arrays. <i>Nature Physics</i>. Springer Nature.
    <a href="https://doi.org/10.1038/s41567-023-02161-w">https://doi.org/10.1038/s41567-023-02161-w</a>
  chicago: Mukhopadhyay, Soham, Jorden L Senior, Jaime Saez Mollejo, Denise Puglia,
    Martin Zemlicka, Johannes M Fink, and Andrew P Higginbotham. “Superconductivity
    from a Melted Insulator in Josephson Junction Arrays.” <i>Nature Physics</i>.
    Springer Nature, 2023. <a href="https://doi.org/10.1038/s41567-023-02161-w">https://doi.org/10.1038/s41567-023-02161-w</a>.
  ieee: S. Mukhopadhyay <i>et al.</i>, “Superconductivity from a melted insulator
    in Josephson junction arrays,” <i>Nature Physics</i>, vol. 19. Springer Nature,
    pp. 1630–1635, 2023.
  ista: Mukhopadhyay S, Senior JL, Saez Mollejo J, Puglia D, Zemlicka M, Fink JM,
    Higginbotham AP. 2023. Superconductivity from a melted insulator in Josephson
    junction arrays. Nature Physics. 19, 1630–1635.
  mla: Mukhopadhyay, Soham, et al. “Superconductivity from a Melted Insulator in Josephson
    Junction Arrays.” <i>Nature Physics</i>, vol. 19, Springer Nature, 2023, pp. 1630–35,
    doi:<a href="https://doi.org/10.1038/s41567-023-02161-w">10.1038/s41567-023-02161-w</a>.
  short: S. Mukhopadhyay, J.L. Senior, J. Saez Mollejo, D. Puglia, M. Zemlicka, J.M.
    Fink, A.P. Higginbotham, Nature Physics 19 (2023) 1630–1635.
date_created: 2023-08-11T07:41:17Z
date_published: 2023-11-01T00:00:00Z
date_updated: 2024-01-29T11:27:49Z
day: '01'
ddc:
- '530'
department:
- _id: GradSch
- _id: AnHi
- _id: JoFi
doi: 10.1038/s41567-023-02161-w
ec_funded: 1
external_id:
  isi:
  - '001054563800006'
file:
- access_level: open_access
  checksum: 1fc86d71bfbf836e221c1e925343adc5
  content_type: application/pdf
  creator: dernst
  date_created: 2024-01-29T11:25:38Z
  date_updated: 2024-01-29T11:25:38Z
  file_id: '14899'
  file_name: 2023_NaturePhysics_Mukhopadhyay.pdf
  file_size: 1977706
  relation: main_file
  success: 1
file_date_updated: 2024-01-29T11:25:38Z
has_accepted_license: '1'
intvolume: '        19'
isi: 1
keyword:
- General Physics and Astronomy
language:
- iso: eng
month: '11'
oa: 1
oa_version: Published Version
page: 1630-1635
project:
- _id: 0aa3608a-070f-11eb-9043-e9cd8a2bd931
  grant_number: P33692
  name: Cavity electromechanics across a quantum phase transition
- _id: 260C2330-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '754411'
  name: ISTplus - Postdoctoral Fellowships
- _id: eb9b30ac-77a9-11ec-83b8-871f581d53d2
  name: Protected states of quantum matter
- _id: bd5b4ec5-d553-11ed-ba76-a6eedb083344
  name: Protected states of quantum matter
publication: Nature Physics
publication_identifier:
  eissn:
  - 1745-2481
  issn:
  - 1745-2473
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Superconductivity from a melted insulator in Josephson junction arrays
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 19
year: '2023'
...
---
_id: '14103'
abstract:
- lang: eng
  text: Observations of individual massive stars, super-luminous supernovae, gamma-ray
    bursts, and gravitational wave events involving spectacular black hole mergers
    indicate that the low-metallicity Universe is fundamentally different from our
    own Galaxy. Many transient phenomena will remain enigmatic until we achieve a
    firm understanding of the physics and evolution of massive stars at low metallicity
    (Z). The Hubble Space Telescope has devoted 500 orbits to observing ∼250 massive
    stars at low Z in the ultraviolet (UV) with the COS and STIS spectrographs under
    the ULLYSES programme. The complementary X-Shooting ULLYSES (XShootU) project
    provides an enhanced legacy value with high-quality optical and near-infrared
    spectra obtained with the wide-wavelength coverage X-shooter spectrograph at ESO’s
    Very Large Telescope. We present an overview of the XShootU project, showing that
    combining ULLYSES UV and XShootU optical spectra is critical for the uniform determination
    of stellar parameters such as effective temperature, surface gravity, luminosity,
    and abundances, as well as wind properties such as mass-loss rates as a function
    of Z. As uncertainties in stellar and wind parameters percolate into many adjacent
    areas of astrophysics, the data and modelling of the XShootU project is expected
    to be a game changer for our physical understanding of massive stars at low Z.
    To be able to confidently interpret James Webb Space Telescope spectra of the
    first stellar generations, the individual spectra of low-Z stars need to be understood,
    which is exactly where XShootU can deliver.
article_number: A154
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Jorick S.
  full_name: Vink, Jorick S.
  last_name: Vink
- first_name: A.
  full_name: Mehner, A.
  last_name: Mehner
- first_name: P. A.
  full_name: Crowther, P. A.
  last_name: Crowther
- first_name: A.
  full_name: Fullerton, A.
  last_name: Fullerton
- first_name: M.
  full_name: Garcia, M.
  last_name: Garcia
- first_name: F.
  full_name: Martins, F.
  last_name: Martins
- first_name: N.
  full_name: Morrell, N.
  last_name: Morrell
- first_name: L. M.
  full_name: Oskinova, L. M.
  last_name: Oskinova
- first_name: N.
  full_name: St-Louis, N.
  last_name: St-Louis
- first_name: A.
  full_name: ud-Doula, A.
  last_name: ud-Doula
- first_name: A. A. C.
  full_name: Sander, A. A. C.
  last_name: Sander
- first_name: H.
  full_name: Sana, H.
  last_name: Sana
- first_name: J.-C.
  full_name: Bouret, J.-C.
  last_name: Bouret
- first_name: B.
  full_name: Kubátová, B.
  last_name: Kubátová
- first_name: P.
  full_name: Marchant, P.
  last_name: Marchant
- first_name: L. P.
  full_name: Martins, L. P.
  last_name: Martins
- first_name: A.
  full_name: Wofford, A.
  last_name: Wofford
- first_name: J. Th.
  full_name: van Loon, J. Th.
  last_name: van Loon
- first_name: O.
  full_name: Grace Telford, O.
  last_name: Grace Telford
- first_name: Ylva Louise Linsdotter
  full_name: Götberg, Ylva Louise Linsdotter
  id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
  last_name: Götberg
  orcid: 0000-0002-6960-6911
- first_name: D. M.
  full_name: Bowman, D. M.
  last_name: Bowman
- first_name: C.
  full_name: Erba, C.
  last_name: Erba
- first_name: V. M.
  full_name: Kalari, V. M.
  last_name: Kalari
- first_name: M.
  full_name: Abdul-Masih, M.
  last_name: Abdul-Masih
- first_name: T.
  full_name: Alkousa, T.
  last_name: Alkousa
- first_name: F.
  full_name: Backs, F.
  last_name: Backs
- first_name: C. L.
  full_name: Barbosa, C. L.
  last_name: Barbosa
- first_name: S. R.
  full_name: Berlanas, S. R.
  last_name: Berlanas
- first_name: M.
  full_name: Bernini-Peron, M.
  last_name: Bernini-Peron
- first_name: J. M.
  full_name: Bestenlehner, J. M.
  last_name: Bestenlehner
- first_name: R.
  full_name: Blomme, R.
  last_name: Blomme
- first_name: J.
  full_name: Bodensteiner, J.
  last_name: Bodensteiner
- first_name: S. A.
  full_name: Brands, S. A.
  last_name: Brands
- first_name: C. J.
  full_name: Evans, C. J.
  last_name: Evans
- first_name: A.
  full_name: David-Uraz, A.
  last_name: David-Uraz
- first_name: F. A.
  full_name: Driessen, F. A.
  last_name: Driessen
- first_name: K.
  full_name: Dsilva, K.
  last_name: Dsilva
- first_name: S.
  full_name: Geen, S.
  last_name: Geen
- first_name: V. M. A.
  full_name: Gómez-González, V. M. A.
  last_name: Gómez-González
- first_name: L.
  full_name: Grassitelli, L.
  last_name: Grassitelli
- first_name: W.-R.
  full_name: Hamann, W.-R.
  last_name: Hamann
- first_name: C.
  full_name: Hawcroft, C.
  last_name: Hawcroft
- first_name: A.
  full_name: Herrero, A.
  last_name: Herrero
- first_name: E. R.
  full_name: Higgins, E. R.
  last_name: Higgins
- first_name: D.
  full_name: John Hillier, D.
  last_name: John Hillier
- first_name: R.
  full_name: Ignace, R.
  last_name: Ignace
- first_name: A. G.
  full_name: Istrate, A. G.
  last_name: Istrate
- first_name: L.
  full_name: Kaper, L.
  last_name: Kaper
- first_name: N. D.
  full_name: Kee, N. D.
  last_name: Kee
- first_name: C.
  full_name: Kehrig, C.
  last_name: Kehrig
- first_name: Z.
  full_name: Keszthelyi, Z.
  last_name: Keszthelyi
- first_name: J.
  full_name: Klencki, J.
  last_name: Klencki
- first_name: A.
  full_name: de Koter, A.
  last_name: de Koter
- first_name: R.
  full_name: Kuiper, R.
  last_name: Kuiper
- first_name: E.
  full_name: Laplace, E.
  last_name: Laplace
- first_name: C. J. K.
  full_name: Larkin, C. J. K.
  last_name: Larkin
- first_name: R. R.
  full_name: Lefever, R. R.
  last_name: Lefever
- first_name: C.
  full_name: Leitherer, C.
  last_name: Leitherer
- first_name: D. J.
  full_name: Lennon, D. J.
  last_name: Lennon
- first_name: L.
  full_name: Mahy, L.
  last_name: Mahy
- first_name: J.
  full_name: Maíz Apellániz, J.
  last_name: Maíz Apellániz
- first_name: G.
  full_name: Maravelias, G.
  last_name: Maravelias
- first_name: W.
  full_name: Marcolino, W.
  last_name: Marcolino
- first_name: A. F.
  full_name: McLeod, A. F.
  last_name: McLeod
- first_name: S. E.
  full_name: de Mink, S. E.
  last_name: de Mink
- first_name: F.
  full_name: Najarro, F.
  last_name: Najarro
- first_name: M. S.
  full_name: Oey, M. S.
  last_name: Oey
- first_name: T. N.
  full_name: Parsons, T. N.
  last_name: Parsons
- first_name: D.
  full_name: Pauli, D.
  last_name: Pauli
- first_name: M. G.
  full_name: Pedersen, M. G.
  last_name: Pedersen
- first_name: R. K.
  full_name: Prinja, R. K.
  last_name: Prinja
- first_name: V.
  full_name: Ramachandran, V.
  last_name: Ramachandran
- first_name: M. C.
  full_name: Ramírez-Tannus, M. C.
  last_name: Ramírez-Tannus
- first_name: G. N.
  full_name: Sabhahit, G. N.
  last_name: Sabhahit
- first_name: A.
  full_name: Schootemeijer, A.
  last_name: Schootemeijer
- first_name: S.
  full_name: Reyero Serantes, S.
  last_name: Reyero Serantes
- first_name: T.
  full_name: Shenar, T.
  last_name: Shenar
- first_name: G. S.
  full_name: Stringfellow, G. S.
  last_name: Stringfellow
- first_name: N.
  full_name: Sudnik, N.
  last_name: Sudnik
- first_name: F.
  full_name: Tramper, F.
  last_name: Tramper
- first_name: L.
  full_name: Wang, L.
  last_name: Wang
citation:
  ama: 'Vink JS, Mehner A, Crowther PA, et al. X-shooting ULLYSES: Massive stars at
    low metallicity. I. Project description. <i>Astronomy &#38; Astrophysics</i>.
    2023;675. doi:<a href="https://doi.org/10.1051/0004-6361/202245650">10.1051/0004-6361/202245650</a>'
  apa: 'Vink, J. S., Mehner, A., Crowther, P. A., Fullerton, A., Garcia, M., Martins,
    F., … Wang, L. (2023). X-shooting ULLYSES: Massive stars at low metallicity. I.
    Project description. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/202245650">https://doi.org/10.1051/0004-6361/202245650</a>'
  chicago: 'Vink, Jorick S., A. Mehner, P. A. Crowther, A. Fullerton, M. Garcia, F.
    Martins, N. Morrell, et al. “X-Shooting ULLYSES: Massive Stars at Low Metallicity.
    I. Project Description.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2023.
    <a href="https://doi.org/10.1051/0004-6361/202245650">https://doi.org/10.1051/0004-6361/202245650</a>.'
  ieee: 'J. S. Vink <i>et al.</i>, “X-shooting ULLYSES: Massive stars at low metallicity.
    I. Project description,” <i>Astronomy &#38; Astrophysics</i>, vol. 675. EDP Sciences,
    2023.'
  ista: 'Vink JS, Mehner A, Crowther PA, Fullerton A, Garcia M, Martins F, Morrell
    N, Oskinova LM, St-Louis N, ud-Doula A, Sander AAC, Sana H, Bouret J-C, Kubátová
    B, Marchant P, Martins LP, Wofford A, van Loon JT, Grace Telford O, Götberg YLL,
    Bowman DM, Erba C, Kalari VM, Abdul-Masih M, Alkousa T, Backs F, Barbosa CL, Berlanas
    SR, Bernini-Peron M, Bestenlehner JM, Blomme R, Bodensteiner J, Brands SA, Evans
    CJ, David-Uraz A, Driessen FA, Dsilva K, Geen S, Gómez-González VMA, Grassitelli
    L, Hamann W-R, Hawcroft C, Herrero A, Higgins ER, John Hillier D, Ignace R, Istrate
    AG, Kaper L, Kee ND, Kehrig C, Keszthelyi Z, Klencki J, de Koter A, Kuiper R,
    Laplace E, Larkin CJK, Lefever RR, Leitherer C, Lennon DJ, Mahy L, Maíz Apellániz
    J, Maravelias G, Marcolino W, McLeod AF, de Mink SE, Najarro F, Oey MS, Parsons
    TN, Pauli D, Pedersen MG, Prinja RK, Ramachandran V, Ramírez-Tannus MC, Sabhahit
    GN, Schootemeijer A, Reyero Serantes S, Shenar T, Stringfellow GS, Sudnik N, Tramper
    F, Wang L. 2023. X-shooting ULLYSES: Massive stars at low metallicity. I. Project
    description. Astronomy &#38; Astrophysics. 675, A154.'
  mla: 'Vink, Jorick S., et al. “X-Shooting ULLYSES: Massive Stars at Low Metallicity.
    I. Project Description.” <i>Astronomy &#38; Astrophysics</i>, vol. 675, A154,
    EDP Sciences, 2023, doi:<a href="https://doi.org/10.1051/0004-6361/202245650">10.1051/0004-6361/202245650</a>.'
  short: J.S. Vink, A. Mehner, P.A. Crowther, A. Fullerton, M. Garcia, F. Martins,
    N. Morrell, L.M. Oskinova, N. St-Louis, A. ud-Doula, A.A.C. Sander, H. Sana, J.-C.
    Bouret, B. Kubátová, P. Marchant, L.P. Martins, A. Wofford, J.T. van Loon, O.
    Grace Telford, Y.L.L. Götberg, D.M. Bowman, C. Erba, V.M. Kalari, M. Abdul-Masih,
    T. Alkousa, F. Backs, C.L. Barbosa, S.R. Berlanas, M. Bernini-Peron, J.M. Bestenlehner,
    R. Blomme, J. Bodensteiner, S.A. Brands, C.J. Evans, A. David-Uraz, F.A. Driessen,
    K. Dsilva, S. Geen, V.M.A. Gómez-González, L. Grassitelli, W.-R. Hamann, C. Hawcroft,
    A. Herrero, E.R. Higgins, D. John Hillier, R. Ignace, A.G. Istrate, L. Kaper,
    N.D. Kee, C. Kehrig, Z. Keszthelyi, J. Klencki, A. de Koter, R. Kuiper, E. Laplace,
    C.J.K. Larkin, R.R. Lefever, C. Leitherer, D.J. Lennon, L. Mahy, J. Maíz Apellániz,
    G. Maravelias, W. Marcolino, A.F. McLeod, S.E. de Mink, F. Najarro, M.S. Oey,
    T.N. Parsons, D. Pauli, M.G. Pedersen, R.K. Prinja, V. Ramachandran, M.C. Ramírez-Tannus,
    G.N. Sabhahit, A. Schootemeijer, S. Reyero Serantes, T. Shenar, G.S. Stringfellow,
    N. Sudnik, F. Tramper, L. Wang, Astronomy &#38; Astrophysics 675 (2023).
date_created: 2023-08-21T10:12:35Z
date_published: 2023-07-01T00:00:00Z
date_updated: 2023-08-22T11:01:07Z
day: '01'
doi: 10.1051/0004-6361/202245650
extern: '1'
external_id:
  arxiv:
  - '2305.06376'
intvolume: '       675'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1051/0004-6361/202245650
month: '07'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
  eissn:
  - 1432-0746
  issn:
  - 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'X-shooting ULLYSES: Massive stars at low metallicity. I. Project description'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 675
year: '2023'
...
---
_id: '14104'
abstract:
- lang: eng
  text: 'Thorne–Żytkow objects (TŻO) are potential end products of the merger of a
    neutron star with a non-degenerate star. In this work, we have computed the first
    grid of evolutionary models of TŻOs with the MESA stellar evolution code. With
    these models, we predict several observational properties of TŻOs, including their
    surface temperatures and luminosities, pulsation periods, and nucleosynthetic
    products. We expand the range of possible TŻO solutions to cover 3.45≲log(Teff/K)≲3.65
    and 4.85≲log(L/L⊙)≲5.5⁠. Due to the much higher densities our TŻOs reach compared
    to previous models, if TŻOs form we expect them to be stable over a larger mass
    range than previously predicted, without exhibiting a gap in their mass distribution.
    Using the GYRE stellar pulsation code we show that TŻOs should have fundamental
    pulsation periods of 1000–2000 d, and period ratios of ≈0.2–0.3. Models computed
    with a large 399 isotope fully coupled nuclear network show a nucleosynthetic
    signal that is different to previously predicted. We propose a new nucleosynthetic
    signal to determine a star’s status as a TŻO: the isotopologues 44TiO2 and 44TiO⁠,
    which will have a shift in their spectral features as compared to stable titanium-containing
    molecules. We find that in the local Universe (∼SMC metallicities and above) TŻOs
    show little heavy metal enrichment, potentially explaining the difficulty in finding
    TŻOs to-date.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: R
  full_name: Farmer, R
  last_name: Farmer
- first_name: M
  full_name: Renzo, M
  last_name: Renzo
- first_name: Ylva Louise Linsdotter
  full_name: Götberg, Ylva Louise Linsdotter
  id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
  last_name: Götberg
  orcid: 0000-0002-6960-6911
- first_name: E
  full_name: Bellinger, E
  last_name: Bellinger
- first_name: S
  full_name: Justham, S
  last_name: Justham
- first_name: S E
  full_name: de Mink, S E
  last_name: de Mink
citation:
  ama: Farmer R, Renzo M, Götberg YLL, Bellinger E, Justham S, de Mink SE. Observational
    predictions for Thorne–Żytkow objects. <i>Monthly Notices of the Royal Astronomical
    Society</i>. 2023;524(2):1692-1709. doi:<a href="https://doi.org/10.1093/mnras/stad1977">10.1093/mnras/stad1977</a>
  apa: Farmer, R., Renzo, M., Götberg, Y. L. L., Bellinger, E., Justham, S., &#38;
    de Mink, S. E. (2023). Observational predictions for Thorne–Żytkow objects. <i>Monthly
    Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href="https://doi.org/10.1093/mnras/stad1977">https://doi.org/10.1093/mnras/stad1977</a>
  chicago: Farmer, R, M Renzo, Ylva Louise Linsdotter Götberg, E Bellinger, S Justham,
    and S E de Mink. “Observational Predictions for Thorne–Żytkow Objects.” <i>Monthly
    Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023.
    <a href="https://doi.org/10.1093/mnras/stad1977">https://doi.org/10.1093/mnras/stad1977</a>.
  ieee: R. Farmer, M. Renzo, Y. L. L. Götberg, E. Bellinger, S. Justham, and S. E.
    de Mink, “Observational predictions for Thorne–Żytkow objects,” <i>Monthly Notices
    of the Royal Astronomical Society</i>, vol. 524, no. 2. Oxford University Press,
    pp. 1692–1709, 2023.
  ista: Farmer R, Renzo M, Götberg YLL, Bellinger E, Justham S, de Mink SE. 2023.
    Observational predictions for Thorne–Żytkow objects. Monthly Notices of the Royal
    Astronomical Society. 524(2), 1692–1709.
  mla: Farmer, R., et al. “Observational Predictions for Thorne–Żytkow Objects.” <i>Monthly
    Notices of the Royal Astronomical Society</i>, vol. 524, no. 2, Oxford University
    Press, 2023, pp. 1692–709, doi:<a href="https://doi.org/10.1093/mnras/stad1977">10.1093/mnras/stad1977</a>.
  short: R. Farmer, M. Renzo, Y.L.L. Götberg, E. Bellinger, S. Justham, S.E. de Mink,
    Monthly Notices of the Royal Astronomical Society 524 (2023) 1692–1709.
date_created: 2023-08-21T10:13:56Z
date_published: 2023-09-01T00:00:00Z
date_updated: 2023-08-21T12:12:48Z
day: '01'
doi: 10.1093/mnras/stad1977
extern: '1'
external_id:
  arxiv:
  - '2305.07337'
intvolume: '       524'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2305.07337
month: '09'
oa: 1
oa_version: Preprint
page: 1692-1709
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
  eissn:
  - 1365-2966
  issn:
  - 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Observational predictions for Thorne–Żytkow objects
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 524
year: '2023'
...
---
_id: '14246'
abstract:
- lang: eng
  text: The model of a ring threaded by the Aharonov-Bohm flux underlies our understanding
    of a coupling between gauge potentials and matter. The typical formulation of
    the model is based upon a single particle picture, and should be extended when
    interactions with other particles become relevant. Here, we illustrate such an
    extension for a particle in an Aharonov-Bohm ring subject to interactions with
    a weakly interacting Bose gas. We show that the ground state of the system can
    be described using the Bose-polaron concept—a particle dressed by interactions
    with a bosonic environment. We connect the energy spectrum to the effective mass
    of the polaron, and demonstrate how to change currents in the system by tuning
    boson-particle interactions. Our results suggest the Aharonov-Bohm ring as a platform
    for studying coherence and few- to many-body crossover of quasi-particles that
    arise from an impurity immersed in a medium.
acknowledgement: "Open Access funding enabled and organized by Projekt DEAL.\r\nWe
  would like to thank Jonas Jager for sharing his data with us in the early stages
  of this project. We thank Joachim Brand and Ray Yang for sharing with us data from
  Yang et al.46. This work has received funding from the DFG Project no. 413495248
  [VO 2437/1-1] (F.B., H.-W.H., A.G.V.). We acknowledge support from the Deutsche
  Forschungsgemeinschaft (DFG - German Research Foundation) and the Open Access Publishing
  Fund of the Technical University of Darmstadt."
article_number: '224'
article_processing_charge: Yes (via OA deal)
article_type: original
arxiv: 1
author:
- first_name: Fabian
  full_name: Brauneis, Fabian
  last_name: Brauneis
- first_name: Areg
  full_name: Ghazaryan, Areg
  id: 4AF46FD6-F248-11E8-B48F-1D18A9856A87
  last_name: Ghazaryan
  orcid: 0000-0001-9666-3543
- first_name: Hans-Werner
  full_name: Hammer, Hans-Werner
  last_name: Hammer
- first_name: Artem
  full_name: Volosniev, Artem
  id: 37D278BC-F248-11E8-B48F-1D18A9856A87
  last_name: Volosniev
  orcid: 0000-0003-0393-5525
citation:
  ama: Brauneis F, Ghazaryan A, Hammer H-W, Volosniev A. Emergence of a Bose polaron
    in a small ring threaded by the Aharonov-Bohm flux. <i>Communications Physics</i>.
    2023;6. doi:<a href="https://doi.org/10.1038/s42005-023-01281-2">10.1038/s42005-023-01281-2</a>
  apa: Brauneis, F., Ghazaryan, A., Hammer, H.-W., &#38; Volosniev, A. (2023). Emergence
    of a Bose polaron in a small ring threaded by the Aharonov-Bohm flux. <i>Communications
    Physics</i>. Springer Nature. <a href="https://doi.org/10.1038/s42005-023-01281-2">https://doi.org/10.1038/s42005-023-01281-2</a>
  chicago: Brauneis, Fabian, Areg Ghazaryan, Hans-Werner Hammer, and Artem Volosniev.
    “Emergence of a Bose Polaron in a Small Ring Threaded by the Aharonov-Bohm Flux.”
    <i>Communications Physics</i>. Springer Nature, 2023. <a href="https://doi.org/10.1038/s42005-023-01281-2">https://doi.org/10.1038/s42005-023-01281-2</a>.
  ieee: F. Brauneis, A. Ghazaryan, H.-W. Hammer, and A. Volosniev, “Emergence of a
    Bose polaron in a small ring threaded by the Aharonov-Bohm flux,” <i>Communications
    Physics</i>, vol. 6. Springer Nature, 2023.
  ista: Brauneis F, Ghazaryan A, Hammer H-W, Volosniev A. 2023. Emergence of a Bose
    polaron in a small ring threaded by the Aharonov-Bohm flux. Communications Physics.
    6, 224.
  mla: Brauneis, Fabian, et al. “Emergence of a Bose Polaron in a Small Ring Threaded
    by the Aharonov-Bohm Flux.” <i>Communications Physics</i>, vol. 6, 224, Springer
    Nature, 2023, doi:<a href="https://doi.org/10.1038/s42005-023-01281-2">10.1038/s42005-023-01281-2</a>.
  short: F. Brauneis, A. Ghazaryan, H.-W. Hammer, A. Volosniev, Communications Physics
    6 (2023).
date_created: 2023-08-28T12:36:49Z
date_published: 2023-08-22T00:00:00Z
date_updated: 2023-12-13T12:21:09Z
day: '22'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1038/s42005-023-01281-2
external_id:
  arxiv:
  - '2301.10488'
  isi:
  - '001052577500002'
file:
- access_level: open_access
  checksum: 6edfc59b0ee7dc406d0968b05236e83d
  content_type: application/pdf
  creator: dernst
  date_created: 2023-09-05T08:45:49Z
  date_updated: 2023-09-05T08:45:49Z
  file_id: '14268'
  file_name: 2023_CommPhysics_Brauneis.pdf
  file_size: 855960
  relation: main_file
  success: 1
file_date_updated: 2023-09-05T08:45:49Z
has_accepted_license: '1'
intvolume: '         6'
isi: 1
keyword:
- General Physics and Astronomy
language:
- iso: eng
month: '08'
oa: 1
oa_version: Published Version
publication: Communications Physics
publication_identifier:
  issn:
  - 2399-3650
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Emergence of a Bose polaron in a small ring threaded by the Aharonov-Bohm flux
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 6
year: '2023'
...
---
_id: '14321'
abstract:
- lang: eng
  text: We demonstrate the possibility of a coupling between the magnetization direction
    of a ferromagnet and the tilting angle of adsorbed achiral molecules. To illustrate
    the mechanism of the coupling, we analyze a minimal Stoner model that includes
    Rashba spin–orbit coupling due to the electric field on the surface of the ferromagnet.
    The proposed mechanism allows us to study magnetic anisotropy of the system with
    an extended Stoner–Wohlfarth model and argue that adsorbed achiral molecules can
    change magnetocrystalline anisotropy of the substrate. Our research aims to motivate
    further experimental studies of the current-free chirality induced spin selectivity
    effect involving both enantiomers.
acknowledgement: "We thank Zhanybek Alpichshev, Mohammad Reza Safari, Binghai Yan,
  and Yossi Paltiel for enlightening discussions.\r\nM.L. acknowledges support from
  the European Research Council (ERC) Starting Grant No. 801770 (ANGULON). A. C. received
  funding from the European Union’s Horizon Europe research and innovation program
  under the Marie Skłodowska-Curie Grant Agreement No. 101062862 - NeqMolRot."
article_number: '104103'
article_processing_charge: Yes (in subscription journal)
article_type: original
arxiv: 1
author:
- first_name: Ragheed
  full_name: Al Hyder, Ragheed
  id: d1c405be-ae15-11ed-8510-ccf53278162e
  last_name: Al Hyder
- first_name: Alberto
  full_name: Cappellaro, Alberto
  id: 9d13b3cb-30a2-11eb-80dc-f772505e8660
  last_name: Cappellaro
  orcid: 0000-0001-6110-2359
- first_name: Mikhail
  full_name: Lemeshko, Mikhail
  id: 37CB05FA-F248-11E8-B48F-1D18A9856A87
  last_name: Lemeshko
  orcid: 0000-0002-6990-7802
- first_name: Artem
  full_name: Volosniev, Artem
  id: 37D278BC-F248-11E8-B48F-1D18A9856A87
  last_name: Volosniev
  orcid: 0000-0003-0393-5525
citation:
  ama: Al Hyder R, Cappellaro A, Lemeshko M, Volosniev A. Achiral dipoles on a ferromagnet
    can affect its magnetization direction. <i>The Journal of Chemical Physics</i>.
    2023;159(10). doi:<a href="https://doi.org/10.1063/5.0165806">10.1063/5.0165806</a>
  apa: Al Hyder, R., Cappellaro, A., Lemeshko, M., &#38; Volosniev, A. (2023). Achiral
    dipoles on a ferromagnet can affect its magnetization direction. <i>The Journal
    of Chemical Physics</i>. AIP Publishing. <a href="https://doi.org/10.1063/5.0165806">https://doi.org/10.1063/5.0165806</a>
  chicago: Al Hyder, Ragheed, Alberto Cappellaro, Mikhail Lemeshko, and Artem Volosniev.
    “Achiral Dipoles on a Ferromagnet Can Affect Its Magnetization Direction.” <i>The
    Journal of Chemical Physics</i>. AIP Publishing, 2023. <a href="https://doi.org/10.1063/5.0165806">https://doi.org/10.1063/5.0165806</a>.
  ieee: R. Al Hyder, A. Cappellaro, M. Lemeshko, and A. Volosniev, “Achiral dipoles
    on a ferromagnet can affect its magnetization direction,” <i>The Journal of Chemical
    Physics</i>, vol. 159, no. 10. AIP Publishing, 2023.
  ista: Al Hyder R, Cappellaro A, Lemeshko M, Volosniev A. 2023. Achiral dipoles on
    a ferromagnet can affect its magnetization direction. The Journal of Chemical
    Physics. 159(10), 104103.
  mla: Al Hyder, Ragheed, et al. “Achiral Dipoles on a Ferromagnet Can Affect Its
    Magnetization Direction.” <i>The Journal of Chemical Physics</i>, vol. 159, no.
    10, 104103, AIP Publishing, 2023, doi:<a href="https://doi.org/10.1063/5.0165806">10.1063/5.0165806</a>.
  short: R. Al Hyder, A. Cappellaro, M. Lemeshko, A. Volosniev, The Journal of Chemical
    Physics 159 (2023).
date_created: 2023-09-13T09:25:09Z
date_published: 2023-09-11T00:00:00Z
date_updated: 2023-09-20T09:48:12Z
day: '11'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.1063/5.0165806
ec_funded: 1
external_id:
  arxiv:
  - '2306.17592'
  pmid:
  - '37694742'
file:
- access_level: open_access
  checksum: 507ab65ab29e2c987c94cabad7c5370b
  content_type: application/pdf
  creator: acappell
  date_created: 2023-09-13T09:34:20Z
  date_updated: 2023-09-13T09:34:20Z
  file_id: '14322'
  file_name: 104103_1_5.0165806.pdf
  file_size: 5749653
  relation: main_file
  success: 1
file_date_updated: 2023-09-13T09:34:20Z
has_accepted_license: '1'
intvolume: '       159'
issue: '10'
keyword:
- Physical and Theoretical Chemistry
- General Physics and Astronomy
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: bd7b5202-d553-11ed-ba76-9b1c1b258338
  grant_number: '101062862'
  name: Non-equilibrium Field Theory of Molecular Rotations
- _id: 2688CF98-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '801770'
  name: 'Angulon: physics and applications of a new quasiparticle'
publication: The Journal of Chemical Physics
publication_identifier:
  eissn:
  - 1089-7690
  issn:
  - 0021-9606
publication_status: published
publisher: AIP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Achiral dipoles on a ferromagnet can affect its magnetization direction
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 159
year: '2023'
...
---
_id: '14334'
abstract:
- lang: eng
  text: Quantum kinetically constrained models have recently attracted significant
    attention due to their anomalous dynamics and thermalization. In this work, we
    introduce a hitherto unexplored family of kinetically constrained models featuring
    conserved particle number and strong inversion-symmetry breaking due to facilitated
    hopping. We demonstrate that these models provide a generic example of so-called
    quantum Hilbert space fragmentation, that is manifested in disconnected sectors
    in the Hilbert space that are not apparent in the computational basis. Quantum
    Hilbert space fragmentation leads to an exponential in system size number of eigenstates
    with exactly zero entanglement entropy across several bipartite cuts. These eigenstates
    can be probed dynamically using quenches from simple initial product states. In
    addition, we study the particle spreading under unitary dynamics launched from
    the domain wall state, and find faster than diffusive dynamics at high particle
    densities, that crosses over into logarithmically slow relaxation at smaller densities.
    Using a classically simulable cellular automaton, we reproduce the logarithmic
    dynamics observed in the quantum case. Our work suggests that particle conserving
    constrained models with inversion symmetry breaking realize so far unexplored
    dynamical behavior and invite their further theoretical and experimental studies.
acknowledgement: "We would like to thank Raimel A. Medina, Hansveer Singh, and Dmitry
  Abanin for useful\r\ndiscussions.The authors acknowledge support by the European
  Research Council\r\n(ERC) under the European Union’s Horizon 2020 research and innovation
  program (Grant\r\nAgreement No. 850899). We acknowledge support by the Erwin Schrödinger
  International\r\nInstitute for Mathematics and Physics (ESI)."
article_number: '093'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Pietro
  full_name: Brighi, Pietro
  id: 4115AF5C-F248-11E8-B48F-1D18A9856A87
  last_name: Brighi
  orcid: 0000-0002-7969-2729
- first_name: Marko
  full_name: Ljubotina, Marko
  id: F75EE9BE-5C90-11EA-905D-16643DDC885E
  last_name: Ljubotina
  orcid: 0000-0003-0038-7068
- first_name: Maksym
  full_name: Serbyn, Maksym
  id: 47809E7E-F248-11E8-B48F-1D18A9856A87
  last_name: Serbyn
  orcid: 0000-0002-2399-5827
citation:
  ama: Brighi P, Ljubotina M, Serbyn M. Hilbert space fragmentation and slow dynamics
    in particle-conserving quantum East models. <i>SciPost Physics</i>. 2023;15(3).
    doi:<a href="https://doi.org/10.21468/scipostphys.15.3.093">10.21468/scipostphys.15.3.093</a>
  apa: Brighi, P., Ljubotina, M., &#38; Serbyn, M. (2023). Hilbert space fragmentation
    and slow dynamics in particle-conserving quantum East models. <i>SciPost Physics</i>.
    SciPost Foundation. <a href="https://doi.org/10.21468/scipostphys.15.3.093">https://doi.org/10.21468/scipostphys.15.3.093</a>
  chicago: Brighi, Pietro, Marko Ljubotina, and Maksym Serbyn. “Hilbert Space Fragmentation
    and Slow Dynamics in Particle-Conserving Quantum East Models.” <i>SciPost Physics</i>.
    SciPost Foundation, 2023. <a href="https://doi.org/10.21468/scipostphys.15.3.093">https://doi.org/10.21468/scipostphys.15.3.093</a>.
  ieee: P. Brighi, M. Ljubotina, and M. Serbyn, “Hilbert space fragmentation and slow
    dynamics in particle-conserving quantum East models,” <i>SciPost Physics</i>,
    vol. 15, no. 3. SciPost Foundation, 2023.
  ista: Brighi P, Ljubotina M, Serbyn M. 2023. Hilbert space fragmentation and slow
    dynamics in particle-conserving quantum East models. SciPost Physics. 15(3), 093.
  mla: Brighi, Pietro, et al. “Hilbert Space Fragmentation and Slow Dynamics in Particle-Conserving
    Quantum East Models.” <i>SciPost Physics</i>, vol. 15, no. 3, 093, SciPost Foundation,
    2023, doi:<a href="https://doi.org/10.21468/scipostphys.15.3.093">10.21468/scipostphys.15.3.093</a>.
  short: P. Brighi, M. Ljubotina, M. Serbyn, SciPost Physics 15 (2023).
date_created: 2023-09-14T13:08:23Z
date_published: 2023-09-13T00:00:00Z
date_updated: 2023-09-20T10:46:29Z
day: '13'
ddc:
- '530'
department:
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doi: 10.21468/scipostphys.15.3.093
ec_funded: 1
external_id:
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  - '2210.15607'
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month: '09'
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  name: 'Non-Ergodic Quantum Matter: Universality, Dynamics and Control'
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title: Hilbert space fragmentation and slow dynamics in particle-conserving quantum
  East models
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type: journal_article
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---
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abstract:
- lang: eng
  text: We study the out-of-equilibrium quantum dynamics of dipolar polarons, i.e.,
    impurities immersed in a dipolar Bose-Einstein condensate, after a quench of the
    impurity-boson interaction. We show that the dipolar nature of the condensate
    and of the impurity results in anisotropic relaxation dynamics, in particular,
    anisotropic dressing of the polaron. More relevantly for cold-atom setups, quench
    dynamics is strongly affected by the interplay between dipolar anisotropy and
    trap geometry. Our findings pave the way for simulating impurities in anisotropic
    media utilizing experiments with dipolar mixtures.
acknowledgement: "We thank Lauriane Chomaz for useful discussions and comments on
  the manuscript. We also\r\nthank Ragheed Al Hyder for comments on the manuscript.\r\nG.B.
  acknowledges support from the Austrian Science Fund (FWF),\r\nunder Project No.
  M2641-N27. This work is supported by the Deutsche Forschungsgemeinschaft (DFG, German
  Research Foundation) under Germany’s Excellence Strategy EXC2181/1-\r\n390900948
  (the Heidelberg STRUCTURES Excellence Cluster). A. G. V. acknowledges support from
  the European Union’s Horizon 2020 research and innovation programme under the\r\nMarie
  Skłodowska-Curie Grant Agreement No. 754411. L.A.P.A acknowledges by the PNRR\r\nMUR
  project PE0000023 - NQSTI and the Deutsche Forschungsgemeinschaft (DFG, German\r\nResearch
  Foundation) under Germany’s Excellence Strategy - EXC - 2123 Quantum Frontiers390837967
  and FOR2247."
article_number: '232'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Artem
  full_name: Volosniev, Artem
  id: 37D278BC-F248-11E8-B48F-1D18A9856A87
  last_name: Volosniev
  orcid: 0000-0003-0393-5525
- first_name: Giacomo
  full_name: Bighin, Giacomo
  id: 4CA96FD4-F248-11E8-B48F-1D18A9856A87
  last_name: Bighin
  orcid: 0000-0001-8823-9777
- first_name: Luis
  full_name: Santos, Luis
  last_name: Santos
- first_name: Luisllu A.
  full_name: Peña Ardila, Luisllu A.
  last_name: Peña Ardila
citation:
  ama: Volosniev A, Bighin G, Santos L, Peña Ardila LA. Non-equilibrium dynamics of
    dipolar polarons. <i>SciPost Physics</i>. 2023;15(6). doi:<a href="https://doi.org/10.21468/scipostphys.15.6.232">10.21468/scipostphys.15.6.232</a>
  apa: Volosniev, A., Bighin, G., Santos, L., &#38; Peña Ardila, L. A. (2023). Non-equilibrium
    dynamics of dipolar polarons. <i>SciPost Physics</i>. SciPost Foundation. <a href="https://doi.org/10.21468/scipostphys.15.6.232">https://doi.org/10.21468/scipostphys.15.6.232</a>
  chicago: Volosniev, Artem, Giacomo Bighin, Luis Santos, and Luisllu A. Peña Ardila.
    “Non-Equilibrium Dynamics of Dipolar Polarons.” <i>SciPost Physics</i>. SciPost
    Foundation, 2023. <a href="https://doi.org/10.21468/scipostphys.15.6.232">https://doi.org/10.21468/scipostphys.15.6.232</a>.
  ieee: A. Volosniev, G. Bighin, L. Santos, and L. A. Peña Ardila, “Non-equilibrium
    dynamics of dipolar polarons,” <i>SciPost Physics</i>, vol. 15, no. 6. SciPost
    Foundation, 2023.
  ista: Volosniev A, Bighin G, Santos L, Peña Ardila LA. 2023. Non-equilibrium dynamics
    of dipolar polarons. SciPost Physics. 15(6), 232.
  mla: Volosniev, Artem, et al. “Non-Equilibrium Dynamics of Dipolar Polarons.” <i>SciPost
    Physics</i>, vol. 15, no. 6, 232, SciPost Foundation, 2023, doi:<a href="https://doi.org/10.21468/scipostphys.15.6.232">10.21468/scipostphys.15.6.232</a>.
  short: A. Volosniev, G. Bighin, L. Santos, L.A. Peña Ardila, SciPost Physics 15
    (2023).
date_created: 2023-12-10T13:03:07Z
date_published: 2023-12-07T00:00:00Z
date_updated: 2024-08-07T07:16:53Z
day: '07'
ddc:
- '530'
department:
- _id: MiLe
doi: 10.21468/scipostphys.15.6.232
ec_funded: 1
external_id:
  arxiv:
  - '2305.17969'
file:
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  date_created: 2023-12-11T07:42:04Z
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intvolume: '        15'
issue: '6'
keyword:
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language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
project:
- _id: 26986C82-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: M02641
  name: A path-integral approach to composite impurities
- _id: 260C2330-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '754411'
  name: ISTplus - Postdoctoral Fellowships
publication: SciPost Physics
publication_identifier:
  issn:
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publication_status: published
publisher: SciPost Foundation
quality_controlled: '1'
status: public
title: Non-equilibrium dynamics of dipolar polarons
tmp:
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  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 15
year: '2023'
...
