---
OA_type: closed access
_id: '21625'
abstract:
- lang: eng
  text: We demonstrate how Implosion Fabrication, a new three-dimensional nanofabrication
    technique, enables the realization of three-dimensional photonic devices at optical
    wavelengths. We realize two- and three-dimensional optical crystals of hydrogel-embedded
    silver meta-atoms.
article_number: FF2D.1
article_processing_charge: No
author:
- first_name: Yannick
  full_name: Salamin, Yannick
  last_name: Salamin
- first_name: Brian
  full_name: Mills, Brian
  last_name: Mills
- first_name: Gaojie
  full_name: Yang, Gaojie
  last_name: Yang
- first_name: Quansan
  full_name: Yang, Quansan
  last_name: Yang
- first_name: Corban
  full_name: Swain, Corban
  last_name: Swain
- first_name: Daniel
  full_name: Oran, Daniel
  last_name: Oran
- first_name: Jamison
  full_name: Sloan, Jamison
  last_name: Sloan
- first_name: Charles
  full_name: Roques-Carmes, Charles
  id: e2e68fc9-6505-11ef-a541-eb4e72cc3e82
  last_name: Roques-Carmes
- first_name: Justin
  full_name: Beroz, Justin
  last_name: Beroz
- first_name: Steven E.
  full_name: Kooi, Steven E.
  last_name: Kooi
- first_name: Edward S.
  full_name: Boyden, Edward S.
  last_name: Boyden
- first_name: Marin
  full_name: Soljačić, Marin
  last_name: Soljačić
citation:
  ama: 'Salamin Y, Mills B, Yang G, et al. Three-dimensional optical crystals nanoprinted
    in a hydrogel. In: <i>Conference on Lasers and Electro-Optics</i>. Optica Publishing
    Group; 2022. doi:<a href="https://doi.org/10.1364/cleo_qels.2022.ff2d.1">10.1364/cleo_qels.2022.ff2d.1</a>'
  apa: 'Salamin, Y., Mills, B., Yang, G., Yang, Q., Swain, C., Oran, D., … Soljačić,
    M. (2022). Three-dimensional optical crystals nanoprinted in a hydrogel. In <i>Conference
    on Lasers and Electro-Optics</i>. San Jose, CA, United States: Optica Publishing
    Group. <a href="https://doi.org/10.1364/cleo_qels.2022.ff2d.1">https://doi.org/10.1364/cleo_qels.2022.ff2d.1</a>'
  chicago: Salamin, Yannick, Brian Mills, Gaojie Yang, Quansan Yang, Corban Swain,
    Daniel Oran, Jamison Sloan, et al. “Three-Dimensional Optical Crystals Nanoprinted
    in a Hydrogel.” In <i>Conference on Lasers and Electro-Optics</i>. Optica Publishing
    Group, 2022. <a href="https://doi.org/10.1364/cleo_qels.2022.ff2d.1">https://doi.org/10.1364/cleo_qels.2022.ff2d.1</a>.
  ieee: Y. Salamin <i>et al.</i>, “Three-dimensional optical crystals nanoprinted
    in a hydrogel,” in <i>Conference on Lasers and Electro-Optics</i>, San Jose, CA,
    United States, 2022.
  ista: 'Salamin Y, Mills B, Yang G, Yang Q, Swain C, Oran D, Sloan J, Roques-Carmes
    C, Beroz J, Kooi SE, Boyden ES, Soljačić M. 2022. Three-dimensional optical crystals
    nanoprinted in a hydrogel. Conference on Lasers and Electro-Optics. CLEO: Fundamental
    Science, FF2D.1.'
  mla: Salamin, Yannick, et al. “Three-Dimensional Optical Crystals Nanoprinted in
    a Hydrogel.” <i>Conference on Lasers and Electro-Optics</i>, FF2D.1, Optica Publishing
    Group, 2022, doi:<a href="https://doi.org/10.1364/cleo_qels.2022.ff2d.1">10.1364/cleo_qels.2022.ff2d.1</a>.
  short: Y. Salamin, B. Mills, G. Yang, Q. Yang, C. Swain, D. Oran, J. Sloan, C. Roques-Carmes,
    J. Beroz, S.E. Kooi, E.S. Boyden, M. Soljačić, in:, Conference on Lasers and Electro-Optics,
    Optica Publishing Group, 2022.
conference:
  end_date: 2022-05-20
  location: San Jose, CA, United States
  name: 'CLEO: Fundamental Science'
  start_date: 2022-05-15
date_created: 2026-03-30T12:22:48Z
date_published: 2022-06-01T00:00:00Z
date_updated: 2026-05-04T13:10:36Z
day: '01'
doi: 10.1364/cleo_qels.2022.ff2d.1
extern: '1'
language:
- iso: eng
month: '06'
oa_version: None
publication: Conference on Lasers and Electro-Optics
publication_identifier:
  eisbn:
  - '9781957171050'
publication_status: published
publisher: Optica Publishing Group
quality_controlled: '1'
status: public
title: Three-dimensional optical crystals nanoprinted in a hydrogel
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2022'
...
---
OA_type: closed access
_id: '21628'
abstract:
- lang: eng
  text: We develop a general framework to enhance and control X-ray scintillation
    by embedding nanophotonic structures into scintillators. We demonstrate 10-fold
    scintillation enhancement in a conventional scintillator, showing the potential
    of our technique for X-ray imaging.
article_number: SM3K.1
article_processing_charge: No
author:
- first_name: Charles
  full_name: Roques-Carmes, Charles
  id: e2e68fc9-6505-11ef-a541-eb4e72cc3e82
  last_name: Roques-Carmes
- first_name: Nicholas
  full_name: Rivera, Nicholas
  last_name: Rivera
- first_name: Steven E.
  full_name: Kooi, Steven E.
  last_name: Kooi
- first_name: Yang
  full_name: Yu, Yang
  last_name: Yu
- first_name: John D.
  full_name: Joannopoulos, John D.
  last_name: Joannopoulos
- first_name: Ido
  full_name: Kaminer, Ido
  last_name: Kaminer
- first_name: Marin
  full_name: Soljačić, Marin
  last_name: Soljačić
citation:
  ama: 'Roques-Carmes C, Rivera N, Kooi SE, et al. X-ray imaging with nanophotonic
    scintillators. In: <i>Conference on Lasers and Electro-Optics</i>. Optica Publishing
    Group; 2022. doi:<a href="https://doi.org/10.1364/cleo_si.2022.sm3k.1">10.1364/cleo_si.2022.sm3k.1</a>'
  apa: 'Roques-Carmes, C., Rivera, N., Kooi, S. E., Yu, Y., Joannopoulos, J. D., Kaminer,
    I., &#38; Soljačić, M. (2022). X-ray imaging with nanophotonic scintillators.
    In <i>Conference on Lasers and Electro-Optics</i>. San Jose, CA, United States:
    Optica Publishing Group. <a href="https://doi.org/10.1364/cleo_si.2022.sm3k.1">https://doi.org/10.1364/cleo_si.2022.sm3k.1</a>'
  chicago: Roques-Carmes, Charles, Nicholas Rivera, Steven E. Kooi, Yang Yu, John
    D. Joannopoulos, Ido Kaminer, and Marin Soljačić. “X-Ray Imaging with Nanophotonic
    Scintillators.” In <i>Conference on Lasers and Electro-Optics</i>. Optica Publishing
    Group, 2022. <a href="https://doi.org/10.1364/cleo_si.2022.sm3k.1">https://doi.org/10.1364/cleo_si.2022.sm3k.1</a>.
  ieee: C. Roques-Carmes <i>et al.</i>, “X-ray imaging with nanophotonic scintillators,”
    in <i>Conference on Lasers and Electro-Optics</i>, San Jose, CA, United States,
    2022.
  ista: 'Roques-Carmes C, Rivera N, Kooi SE, Yu Y, Joannopoulos JD, Kaminer I, Soljačić
    M. 2022. X-ray imaging with nanophotonic scintillators. Conference on Lasers and
    Electro-Optics. CLEO: Science and Innovations, SM3K.1.'
  mla: Roques-Carmes, Charles, et al. “X-Ray Imaging with Nanophotonic Scintillators.”
    <i>Conference on Lasers and Electro-Optics</i>, SM3K.1, Optica Publishing Group,
    2022, doi:<a href="https://doi.org/10.1364/cleo_si.2022.sm3k.1">10.1364/cleo_si.2022.sm3k.1</a>.
  short: C. Roques-Carmes, N. Rivera, S.E. Kooi, Y. Yu, J.D. Joannopoulos, I. Kaminer,
    M. Soljačić, in:, Conference on Lasers and Electro-Optics, Optica Publishing Group,
    2022.
conference:
  end_date: 2022-05-20
  location: San Jose, CA, United States
  name: 'CLEO: Science and Innovations'
  start_date: 2022-05-15
date_created: 2026-03-30T12:22:48Z
date_published: 2022-06-01T00:00:00Z
date_updated: 2026-05-04T13:11:24Z
day: '01'
doi: 10.1364/cleo_si.2022.sm3k.1
extern: '1'
language:
- iso: eng
month: '06'
oa_version: None
publication: Conference on Lasers and Electro-Optics
publication_identifier:
  eisbn:
  - '9781957171050'
publication_status: published
publisher: Optica Publishing Group
quality_controlled: '1'
status: public
title: X-ray imaging with nanophotonic scintillators
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2022'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '21638'
abstract:
- lang: eng
  text: 'We introduce end-to-end inverse design for multi-channel imaging, in which
    a nanophotonic frontend is optimized in conjunction with an image-processing backend
    to extract depth, spectral and polarization channels from a single monochrome
    image. Unlike diffractive optics, we show that subwavelength-scale “metasurface”
    designs can easily distinguish similar wavelength and polarization inputs. The
    proposed technique integrates a single-layer metasurface frontend with an efficient
    Tikhonov reconstruction backend, without any additional optics except a grayscale
    sensor. Our method yields multi-channel imaging by spontaneous demultiplexing:
    the metaoptics front-end separates different channels into distinct spatial domains
    whose locations on the sensor are optimally discovered by the inverse-design algorithm.
    We present large-area metasurface designs, compatible with standard lithography,
    for multi-spectral imaging, depth-spectral imaging, and “all-in-one” spectro-polarimetric-depth
    imaging with robust reconstruction performance (≲ 10% error with 1% detector noise).
    In contrast to neural networks, our framework is physically interpretable and
    does not require large training sets. It can be used to reconstruct arbitrary
    three-dimensional scenes with full multi-wavelength spectra and polarization textures.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Zin
  full_name: Lin, Zin
  last_name: Lin
- first_name: Raphaël
  full_name: Pestourie, Raphaël
  last_name: Pestourie
- first_name: Charles
  full_name: Roques-Carmes, Charles
  id: e2e68fc9-6505-11ef-a541-eb4e72cc3e82
  last_name: Roques-Carmes
- first_name: Zhaoyi
  full_name: Li, Zhaoyi
  last_name: Li
- first_name: Federico
  full_name: Capasso, Federico
  last_name: Capasso
- first_name: Marin
  full_name: Soljačić, Marin
  last_name: Soljačić
- first_name: Steven G.
  full_name: Johnson, Steven G.
  last_name: Johnson
citation:
  ama: Lin Z, Pestourie R, Roques-Carmes C, et al. End-to-end metasurface inverse
    design for single-shot multi-channel imaging. <i>Optics Express</i>. 2022;30(16):28358-28370.
    doi:<a href="https://doi.org/10.1364/oe.449985">10.1364/oe.449985</a>
  apa: Lin, Z., Pestourie, R., Roques-Carmes, C., Li, Z., Capasso, F., Soljačić, M.,
    &#38; Johnson, S. G. (2022). End-to-end metasurface inverse design for single-shot
    multi-channel imaging. <i>Optics Express</i>. Optica Publishing Group. <a href="https://doi.org/10.1364/oe.449985">https://doi.org/10.1364/oe.449985</a>
  chicago: Lin, Zin, Raphaël Pestourie, Charles Roques-Carmes, Zhaoyi Li, Federico
    Capasso, Marin Soljačić, and Steven G. Johnson. “End-to-End Metasurface Inverse
    Design for Single-Shot Multi-Channel Imaging.” <i>Optics Express</i>. Optica Publishing
    Group, 2022. <a href="https://doi.org/10.1364/oe.449985">https://doi.org/10.1364/oe.449985</a>.
  ieee: Z. Lin <i>et al.</i>, “End-to-end metasurface inverse design for single-shot
    multi-channel imaging,” <i>Optics Express</i>, vol. 30, no. 16. Optica Publishing
    Group, pp. 28358–28370, 2022.
  ista: Lin Z, Pestourie R, Roques-Carmes C, Li Z, Capasso F, Soljačić M, Johnson
    SG. 2022. End-to-end metasurface inverse design for single-shot multi-channel
    imaging. Optics Express. 30(16), 28358–28370.
  mla: Lin, Zin, et al. “End-to-End Metasurface Inverse Design for Single-Shot Multi-Channel
    Imaging.” <i>Optics Express</i>, vol. 30, no. 16, Optica Publishing Group, 2022,
    pp. 28358–70, doi:<a href="https://doi.org/10.1364/oe.449985">10.1364/oe.449985</a>.
  short: Z. Lin, R. Pestourie, C. Roques-Carmes, Z. Li, F. Capasso, M. Soljačić, S.G.
    Johnson, Optics Express 30 (2022) 28358–28370.
date_created: 2026-03-30T12:22:48Z
date_published: 2022-07-19T00:00:00Z
date_updated: 2026-04-27T09:09:05Z
day: '19'
ddc:
- '530'
doi: 10.1364/oe.449985
extern: '1'
external_id:
  arxiv:
  - '2111.01071'
  pmid:
  - ' 36299033'
intvolume: '        30'
issue: '16'
language:
- iso: eng
license: https://creativecommons.org/licenses/by/4.0/
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1364/OE.449985
month: '07'
oa: 1
oa_version: Published Version
page: 28358-28370
pmid: 1
publication: Optics Express
publication_identifier:
  eissn:
  - 1094-4087
publication_status: published
publisher: Optica Publishing Group
quality_controlled: '1'
scopus_import: '1'
status: public
title: End-to-end metasurface inverse design for single-shot multi-channel imaging
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: ba8df636-2132-11f1-aed0-ed93e2281fdd
volume: 30
year: '2022'
...
---
OA_place: repository
OA_type: green
_id: '21673'
abstract:
- lang: eng
  text: 'When impinging on optical structures or passing in their vicinity, free electrons
    can spontaneously emit electromagnetic radiation, a phenomenon generally known
    as cathodoluminescence. Free-electron radiation comes in many guises: Cherenkov,
    transition, and Smith-Purcell radiation, but also electron scintillation, commonly
    referred to as incoherent cathodoluminescence. While those effects have been at
    the heart of many fundamental discoveries and technological developments in high-energy
    physics in the past century, their recent demonstration in photonic and nanophotonic
    systems has attracted a lot of attention. Those developments arose from predictions
    that exploit nanophotonics for novel radiation regimes, now becoming accessible
    thanks to advances in nanofabrication. In general, the proper design of nanophotonic
    structures can enable shaping, control, and enhancement of free-electron radiation,
    for any of the above-mentioned effects. Free-electron radiation in nanophotonics
    opens the way to promising applications, such as widely-tunable integrated light
    sources from x-ray to THz frequencies, miniaturized particle accelerators, and
    highly sensitive high-energy particle detectors. Here, we review the emerging
    field of free-electron radiation in nanophotonics. We first present a general,
    unified framework to describe free-electron light-matter interaction in arbitrary
    nanophotonic systems. We then show how this framework sheds light on the physical
    underpinnings of many methods in the field used to control and enhance free-electron
    radiation. Namely, the framework points to the central role played by the photonic
    eigenmodes in controlling the output properties of free-electron radiation (e.g.,
    frequency, directionality, and polarization). [... see full abstract in paper]'
article_number: '2208.02368'
article_processing_charge: No
arxiv: 1
author:
- first_name: Charles
  full_name: Roques-Carmes, Charles
  id: e2e68fc9-6505-11ef-a541-eb4e72cc3e82
  last_name: Roques-Carmes
- first_name: Steven E.
  full_name: Kooi, Steven E.
  last_name: Kooi
- first_name: Yi
  full_name: Yang, Yi
  last_name: Yang
- first_name: Nicholas
  full_name: Rivera, Nicholas
  last_name: Rivera
- first_name: Phillip D.
  full_name: Keathley, Phillip D.
  last_name: Keathley
- first_name: John D.
  full_name: Joannopoulos, John D.
  last_name: Joannopoulos
- first_name: Steven G.
  full_name: Johnson, Steven G.
  last_name: Johnson
- first_name: Ido
  full_name: Kaminer, Ido
  last_name: Kaminer
- first_name: Karl K.
  full_name: Berggren, Karl K.
  last_name: Berggren
- first_name: Marin
  full_name: Soljačić, Marin
  last_name: Soljačić
citation:
  ama: Roques-Carmes C, Kooi SE, Yang Y, et al. Free-electron-light interactions in
    nanophotonics. <i>arXiv</i>. doi:<a href="https://doi.org/10.48550/arXiv.2208.02368">10.48550/arXiv.2208.02368</a>
  apa: Roques-Carmes, C., Kooi, S. E., Yang, Y., Rivera, N., Keathley, P. D., Joannopoulos,
    J. D., … Soljačić, M. (n.d.). Free-electron-light interactions in nanophotonics.
    <i>arXiv</i>. <a href="https://doi.org/10.48550/arXiv.2208.02368">https://doi.org/10.48550/arXiv.2208.02368</a>
  chicago: Roques-Carmes, Charles, Steven E. Kooi, Yi Yang, Nicholas Rivera, Phillip
    D. Keathley, John D. Joannopoulos, Steven G. Johnson, Ido Kaminer, Karl K. Berggren,
    and Marin Soljačić. “Free-Electron-Light Interactions in Nanophotonics.” <i>ArXiv</i>,
    n.d. <a href="https://doi.org/10.48550/arXiv.2208.02368">https://doi.org/10.48550/arXiv.2208.02368</a>.
  ieee: C. Roques-Carmes <i>et al.</i>, “Free-electron-light interactions in nanophotonics,”
    <i>arXiv</i>. .
  ista: Roques-Carmes C, Kooi SE, Yang Y, Rivera N, Keathley PD, Joannopoulos JD,
    Johnson SG, Kaminer I, Berggren KK, Soljačić M. Free-electron-light interactions
    in nanophotonics. arXiv, 2208.02368.
  mla: Roques-Carmes, Charles, et al. “Free-Electron-Light Interactions in Nanophotonics.”
    <i>ArXiv</i>, 2208.02368, doi:<a href="https://doi.org/10.48550/arXiv.2208.02368">10.48550/arXiv.2208.02368</a>.
  short: C. Roques-Carmes, S.E. Kooi, Y. Yang, N. Rivera, P.D. Keathley, J.D. Joannopoulos,
    S.G. Johnson, I. Kaminer, K.K. Berggren, M. Soljačić, ArXiv (n.d.).
date_created: 2026-04-09T09:10:41Z
date_published: 2022-08-03T00:00:00Z
date_updated: 2026-04-13T09:42:12Z
day: '03'
doi: 10.48550/arXiv.2208.02368
extern: '1'
external_id:
  arxiv:
  - '2208.02368'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2208.02368
month: '08'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
scopus_import: '1'
status: public
title: Free-electron-light interactions in nanophotonics
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2022'
...
---
OA_type: closed access
_id: '21809'
abstract:
- lang: eng
  text: Controlling the multistage photoresponsivity remains a challenge, in part,
    due to the spontaneous tautomerization between isomers. Herein, we present a strategy
    to access three independent states (linear, cyclic keto, and cyclic enolate) of
    crown ether (CE)-substituted donor–acceptor Stenhouse adducts (DASAs) by limiting
    the tautomerization of the closed isomers. The linear–cyclic keto isomerization
    is reversibly triggered by treatment with metal ions (Na+ or K+) and CE, while
    the linear–cyclic enolate isomerization is induced by green light and heat. Density
    functional theory and molecular dynamics calculation results suggest that the
    steric effect and supramolecular interaction between the electron-donating and
    electron-withdrawing moieties play an important role in hindering the tautomerization
    between cyclic keto and cyclic enolate DASA-CE. The strategy to influence key
    steps in the photoswitching process inspires well-controlled multistage isomerization
    of photoresponsive molecules.
article_processing_charge: No
article_type: original
author:
- first_name: Yongli
  full_name: Duan, Yongli
  last_name: Duan
- first_name: Haiquan
  full_name: Zhao, Haiquan
  last_name: Zhao
- first_name: Guodong
  full_name: Xue, Guodong
  last_name: Xue
- first_name: Fanxi
  full_name: Sun, Fanxi
  last_name: Sun
- first_name: Friedrich J
  full_name: Stricker, Friedrich J
  id: 7aca2cfc-46cf-11f0-abd3-8c96b5186745
  last_name: Stricker
- first_name: Zhen
  full_name: Wang, Zhen
  last_name: Wang
- first_name: Lijun
  full_name: Mao, Lijun
  last_name: Mao
- first_name: Chao
  full_name: He, Chao
  last_name: He
- first_name: Javier Read
  full_name: de Alaniz, Javier Read
  last_name: de Alaniz
- first_name: Yonghao
  full_name: Zheng, Yonghao
  last_name: Zheng
- first_name: Dongsheng
  full_name: Wang, Dongsheng
  last_name: Wang
citation:
  ama: Duan Y, Zhao H, Xue G, et al. Controlling the isomerization of photoresponsive
    molecules through a limiting tautomerization strategy. <i>The Journal of Physical
    Chemistry B</i>. 2022;126(17):3347-3354. doi:<a href="https://doi.org/10.1021/acs.jpcb.2c02005">10.1021/acs.jpcb.2c02005</a>
  apa: Duan, Y., Zhao, H., Xue, G., Sun, F., Stricker, F. J., Wang, Z., … Wang, D.
    (2022). Controlling the isomerization of photoresponsive molecules through a limiting
    tautomerization strategy. <i>The Journal of Physical Chemistry B</i>. American
    Chemical Society. <a href="https://doi.org/10.1021/acs.jpcb.2c02005">https://doi.org/10.1021/acs.jpcb.2c02005</a>
  chicago: Duan, Yongli, Haiquan Zhao, Guodong Xue, Fanxi Sun, Friedrich J Stricker,
    Zhen Wang, Lijun Mao, et al. “Controlling the Isomerization of Photoresponsive
    Molecules through a Limiting Tautomerization Strategy.” <i>The Journal of Physical
    Chemistry B</i>. American Chemical Society, 2022. <a href="https://doi.org/10.1021/acs.jpcb.2c02005">https://doi.org/10.1021/acs.jpcb.2c02005</a>.
  ieee: Y. Duan <i>et al.</i>, “Controlling the isomerization of photoresponsive molecules
    through a limiting tautomerization strategy,” <i>The Journal of Physical Chemistry
    B</i>, vol. 126, no. 17. American Chemical Society, pp. 3347–3354, 2022.
  ista: Duan Y, Zhao H, Xue G, Sun F, Stricker FJ, Wang Z, Mao L, He C, de Alaniz
    JR, Zheng Y, Wang D. 2022. Controlling the isomerization of photoresponsive molecules
    through a limiting tautomerization strategy. The Journal of Physical Chemistry
    B. 126(17), 3347–3354.
  mla: Duan, Yongli, et al. “Controlling the Isomerization of Photoresponsive Molecules
    through a Limiting Tautomerization Strategy.” <i>The Journal of Physical Chemistry
    B</i>, vol. 126, no. 17, American Chemical Society, 2022, pp. 3347–54, doi:<a
    href="https://doi.org/10.1021/acs.jpcb.2c02005">10.1021/acs.jpcb.2c02005</a>.
  short: Y. Duan, H. Zhao, G. Xue, F. Sun, F.J. Stricker, Z. Wang, L. Mao, C. He,
    J.R. de Alaniz, Y. Zheng, D. Wang, The Journal of Physical Chemistry B 126 (2022)
    3347–3354.
date_created: 2026-05-06T10:45:18Z
date_published: 2022-04-26T00:00:00Z
date_updated: 2026-05-11T07:28:38Z
day: '26'
ddc:
- '540'
doi: 10.1021/acs.jpcb.2c02005
extern: '1'
external_id:
  pmid:
  - '35471969'
intvolume: '       126'
issue: '17'
language:
- iso: eng
month: '04'
oa_version: None
page: 3347-3354
pmid: 1
publication: The Journal of Physical Chemistry B
publication_identifier:
  eissn:
  - 1520-5207
  issn:
  - 1520-6106
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Controlling the isomerization of photoresponsive molecules through a limiting
  tautomerization strategy
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 126
year: '2022'
...
---
OA_type: closed access
_id: '21819'
abstract:
- lang: eng
  text: The ability of molecular photoswitches to convert on/off responses into large
    macroscale property change is fundamental to light-responsive materials. However,
    moving beyond simple binary responses necessitates the introduction of new elements
    that control the chemistry of the photoswitching process at the molecular scale.
    To achieve this goal, we designed, synthesized and developed a single photochrome,
    based on a modified donor–acceptor Stenhouse adduct (DASA), capable of independently
    addressing multiple molecular states. The multi-stage photoswitch enables complex
    switching phenomena. To demonstrate this, we show spatial control of the transformation
    of a three-stage photoswitch by tuning the population of intermediates along the
    multi-step reaction pathway of the DASAs without interfering with either the first
    or final stage. This allows for a photonic three-stage logic gate where the secondary
    wavelength solely negates the input of the primary wavelength. These results provide
    a new strategy to move beyond traditional on/off binary photochromic systems and
    enable the design of future molecular logic systems.
article_processing_charge: No
article_type: original
author:
- first_name: Friedrich J
  full_name: Stricker, Friedrich J
  id: 7aca2cfc-46cf-11f0-abd3-8c96b5186745
  last_name: Stricker
- first_name: David M.
  full_name: Sanchez, David M.
  last_name: Sanchez
- first_name: Umberto
  full_name: Raucci, Umberto
  last_name: Raucci
- first_name: Neil D.
  full_name: Dolinski, Neil D.
  last_name: Dolinski
- first_name: Manuel S.
  full_name: Zayas, Manuel S.
  last_name: Zayas
- first_name: Jan
  full_name: Meisner, Jan
  last_name: Meisner
- first_name: Craig. J.
  full_name: Hawker, Craig. J.
  last_name: Hawker
- first_name: Todd. J.
  full_name: Martínez, Todd. J.
  last_name: Martínez
- first_name: Javier
  full_name: Read de Alaniz, Javier
  last_name: Read de Alaniz
citation:
  ama: Stricker FJ, Sanchez DM, Raucci U, et al. A multi-stage single photochrome
    system for controlled photoswitching responses. <i>Nature Chemistry</i>. 2022;14:942-948.
    doi:<a href="https://doi.org/10.1038/s41557-022-00947-8">10.1038/s41557-022-00947-8</a>
  apa: Stricker, F. J., Sanchez, D. M., Raucci, U., Dolinski, N. D., Zayas, M. S.,
    Meisner, J., … Read de Alaniz, J. (2022). A multi-stage single photochrome system
    for controlled photoswitching responses. <i>Nature Chemistry</i>. Springer Nature.
    <a href="https://doi.org/10.1038/s41557-022-00947-8">https://doi.org/10.1038/s41557-022-00947-8</a>
  chicago: Stricker, Friedrich J, David M. Sanchez, Umberto Raucci, Neil D. Dolinski,
    Manuel S. Zayas, Jan Meisner, Craig. J. Hawker, Todd. J. Martínez, and Javier
    Read de Alaniz. “A Multi-Stage Single Photochrome System for Controlled Photoswitching
    Responses.” <i>Nature Chemistry</i>. Springer Nature, 2022. <a href="https://doi.org/10.1038/s41557-022-00947-8">https://doi.org/10.1038/s41557-022-00947-8</a>.
  ieee: F. J. Stricker <i>et al.</i>, “A multi-stage single photochrome system for
    controlled photoswitching responses,” <i>Nature Chemistry</i>, vol. 14. Springer
    Nature, pp. 942–948, 2022.
  ista: Stricker FJ, Sanchez DM, Raucci U, Dolinski ND, Zayas MS, Meisner J, Hawker
    CJ, Martínez TJ, Read de Alaniz J. 2022. A multi-stage single photochrome system
    for controlled photoswitching responses. Nature Chemistry. 14, 942–948.
  mla: Stricker, Friedrich J., et al. “A Multi-Stage Single Photochrome System for
    Controlled Photoswitching Responses.” <i>Nature Chemistry</i>, vol. 14, Springer
    Nature, 2022, pp. 942–48, doi:<a href="https://doi.org/10.1038/s41557-022-00947-8">10.1038/s41557-022-00947-8</a>.
  short: F.J. Stricker, D.M. Sanchez, U. Raucci, N.D. Dolinski, M.S. Zayas, J. Meisner,
    C.J. Hawker, T.J. Martínez, J. Read de Alaniz, Nature Chemistry 14 (2022) 942–948.
date_created: 2026-05-06T10:56:14Z
date_published: 2022-06-09T00:00:00Z
date_updated: 2026-05-18T09:13:44Z
day: '09'
ddc:
- '540'
doi: 10.1038/s41557-022-00947-8
extern: '1'
external_id:
  pmid:
  - '35681046'
intvolume: '        14'
language:
- iso: eng
month: '06'
oa_version: None
page: 942-948
pmid: 1
publication: Nature Chemistry
publication_identifier:
  eissn:
  - 1755-4349
  issn:
  - 1755-4330
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: A multi-stage single photochrome system for controlled photoswitching responses
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 14
year: '2022'
...
---
OA_type: green
_id: '21823'
abstract:
- lang: eng
  text: DFT calculations were used to find an optimal substitution site on the triene
    backbone of a donor–acceptor Stenhouse adduct photoswitch to tune the equillibrium
    and switching kinetics of DASA without modifying the donor and acceptor groups.
    Using this approach we demonstrate a new means to tuning DASA based photoswitches
    by increasing the energy of the closed form relative to the open form. To highlight
    the potential of this approach a new DASA derivative bearing a methyl substituent
    on the 5-position of the triene was synthesized and the effect of this substitution
    was studied using 1H NMR spectroscopy, time-dependent UV-Vis and solvatochromic
    analysis. The new DASA derivative shows a higher dark equillibrium, favoring the
    open form, and drastically faster thermal recovery than the unsubstituted derivative
    with the same donor and acceptor.
article_processing_charge: No
article_type: original
author:
- first_name: Julie A.
  full_name: Peterson, Julie A.
  last_name: Peterson
- first_name: Friedrich J
  full_name: Stricker, Friedrich J
  id: 7aca2cfc-46cf-11f0-abd3-8c96b5186745
  last_name: Stricker
- first_name: Javier
  full_name: Read de Alaniz, Javier
  last_name: Read de Alaniz
citation:
  ama: Peterson JA, Stricker FJ, Read de Alaniz J. Improving the kinetics and dark
    equilibrium of donor-acceptor Stenhouse adduct by triene backbone design. <i>Chemical
    Communications</i>. 2022;58(14):2303-2306. doi:<a href="https://doi.org/10.1039/d1cc06235b">10.1039/d1cc06235b</a>
  apa: Peterson, J. A., Stricker, F. J., &#38; Read de Alaniz, J. (2022). Improving
    the kinetics and dark equilibrium of donor-acceptor Stenhouse adduct by triene
    backbone design. <i>Chemical Communications</i>. Royal Society of Chemistry. <a
    href="https://doi.org/10.1039/d1cc06235b">https://doi.org/10.1039/d1cc06235b</a>
  chicago: Peterson, Julie A., Friedrich J Stricker, and Javier Read de Alaniz. “Improving
    the Kinetics and Dark Equilibrium of Donor-Acceptor Stenhouse Adduct by Triene
    Backbone Design.” <i>Chemical Communications</i>. Royal Society of Chemistry,
    2022. <a href="https://doi.org/10.1039/d1cc06235b">https://doi.org/10.1039/d1cc06235b</a>.
  ieee: J. A. Peterson, F. J. Stricker, and J. Read de Alaniz, “Improving the kinetics
    and dark equilibrium of donor-acceptor Stenhouse adduct by triene backbone design,”
    <i>Chemical Communications</i>, vol. 58, no. 14. Royal Society of Chemistry, pp.
    2303–2306, 2022.
  ista: Peterson JA, Stricker FJ, Read de Alaniz J. 2022. Improving the kinetics and
    dark equilibrium of donor-acceptor Stenhouse adduct by triene backbone design.
    Chemical Communications. 58(14), 2303–2306.
  mla: Peterson, Julie A., et al. “Improving the Kinetics and Dark Equilibrium of
    Donor-Acceptor Stenhouse Adduct by Triene Backbone Design.” <i>Chemical Communications</i>,
    vol. 58, no. 14, Royal Society of Chemistry, 2022, pp. 2303–06, doi:<a href="https://doi.org/10.1039/d1cc06235b">10.1039/d1cc06235b</a>.
  short: J.A. Peterson, F.J. Stricker, J. Read de Alaniz, Chemical Communications
    58 (2022) 2303–2306.
date_created: 2026-05-06T10:59:03Z
date_published: 2022-01-17T00:00:00Z
date_updated: 2026-05-18T09:46:30Z
day: '17'
ddc:
- '540'
doi: 10.1039/d1cc06235b
extern: '1'
external_id:
  pmid:
  - '35075464'
intvolume: '        58'
issue: '14'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1039/D1CC06235B
month: '01'
oa: 1
oa_version: Accepted Version
page: 2303-2306
pmid: 1
publication: Chemical Communications
publication_identifier:
  eissn:
  - 1364-548X
  issn:
  - 1359-7345
publication_status: published
publisher: Royal Society of Chemistry
quality_controlled: '1'
scopus_import: '1'
status: public
title: Improving the kinetics and dark equilibrium of donor-acceptor Stenhouse adduct
  by triene backbone design
type: journal_article
user_id: ba8df636-2132-11f1-aed0-ed93e2281fdd
volume: 58
year: '2022'
...
---
OA_type: closed access
_id: '21824'
abstract:
- lang: eng
  text: We investigate the influence of the host matrix on the photothermally driven
    actuation performance of negatively photochromic, donor−acceptor Stenhouse adduct
    (DASA)-based polymers. Using a modular Diels−Alder “click” platform, we designed
    polymeric materials with varying DASA incorporation and investigated the relationships
    between the material composition and the resulting physical, mechanical, and photoswitching
    properties. We demonstrate that increasing the DASA concentration in polymer conjugates
    has a dramatic effect on the material’s physical and mechanical properties, such
    as the glass transition temperature (Tg) and elastic modulus, as well as the photoswitching
    properties, which are found to be highly dependent on Tg. We establish using a
    simple photoresponsive bilayer that actuation performance is controlled by the
    bilayer stiffness rather than the photochrome incorporation of DASA. Finally,
    we report and compare the light-induced property changes in Tg and the elastic
    modulus between the materials comprising the open or closed forms of DASAs. Our
    results demonstrate the importance of designing a material that is stiff enough
    to provide the mechanical strength required for actuation under load, but soft
    enough to reversibly switch at the operational temperature and provide key considerations
    for the development of application-geared photoswitchable materials.
article_processing_charge: No
article_type: original
author:
- first_name: Miranda M.
  full_name: Sroda, Miranda M.
  last_name: Sroda
- first_name: Jaejun
  full_name: Lee, Jaejun
  last_name: Lee
- first_name: Younghoon
  full_name: Kwon, Younghoon
  last_name: Kwon
- first_name: Friedrich J
  full_name: Stricker, Friedrich J
  id: 7aca2cfc-46cf-11f0-abd3-8c96b5186745
  last_name: Stricker
- first_name: Minwook
  full_name: Park, Minwook
  last_name: Park
- first_name: Megan T.
  full_name: Valentine, Megan T.
  last_name: Valentine
- first_name: Javier
  full_name: Read de Alaniz, Javier
  last_name: Read de Alaniz
citation:
  ama: Sroda MM, Lee J, Kwon Y, et al. Role of material composition in photothermal
    actuation of DASA-based polymers. <i>ACS Applied Polymer Materials</i>. 2022;4(1):141-149.
    doi:<a href="https://doi.org/10.1021/acsapm.1c01108">10.1021/acsapm.1c01108</a>
  apa: Sroda, M. M., Lee, J., Kwon, Y., Stricker, F. J., Park, M., Valentine, M. T.,
    &#38; Read de Alaniz, J. (2022). Role of material composition in photothermal
    actuation of DASA-based polymers. <i>ACS Applied Polymer Materials</i>. American
    Chemical Society. <a href="https://doi.org/10.1021/acsapm.1c01108">https://doi.org/10.1021/acsapm.1c01108</a>
  chicago: Sroda, Miranda M., Jaejun Lee, Younghoon Kwon, Friedrich J Stricker, Minwook
    Park, Megan T. Valentine, and Javier Read de Alaniz. “Role of Material Composition
    in Photothermal Actuation of DASA-Based Polymers.” <i>ACS Applied Polymer Materials</i>.
    American Chemical Society, 2022. <a href="https://doi.org/10.1021/acsapm.1c01108">https://doi.org/10.1021/acsapm.1c01108</a>.
  ieee: M. M. Sroda <i>et al.</i>, “Role of material composition in photothermal actuation
    of DASA-based polymers,” <i>ACS Applied Polymer Materials</i>, vol. 4, no. 1.
    American Chemical Society, pp. 141–149, 2022.
  ista: Sroda MM, Lee J, Kwon Y, Stricker FJ, Park M, Valentine MT, Read de Alaniz
    J. 2022. Role of material composition in photothermal actuation of DASA-based
    polymers. ACS Applied Polymer Materials. 4(1), 141–149.
  mla: Sroda, Miranda M., et al. “Role of Material Composition in Photothermal Actuation
    of DASA-Based Polymers.” <i>ACS Applied Polymer Materials</i>, vol. 4, no. 1,
    American Chemical Society, 2022, pp. 141–49, doi:<a href="https://doi.org/10.1021/acsapm.1c01108">10.1021/acsapm.1c01108</a>.
  short: M.M. Sroda, J. Lee, Y. Kwon, F.J. Stricker, M. Park, M.T. Valentine, J. Read
    de Alaniz, ACS Applied Polymer Materials 4 (2022) 141–149.
date_created: 2026-05-06T10:59:35Z
date_published: 2022-01-05T00:00:00Z
date_updated: 2026-05-11T07:46:45Z
day: '05'
ddc:
- '540'
doi: 10.1021/acsapm.1c01108
extern: '1'
intvolume: '         4'
issue: '1'
keyword:
- donor−acceptor Stenhouse adducts
- photothermal actuation
- photo-induced property changes
- negative photochromism
- glass transition temperature
language:
- iso: eng
month: '01'
oa_version: None
page: 141-149
publication: ACS Applied Polymer Materials
publication_identifier:
  eissn:
  - 2637-6105
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Role of material composition in photothermal actuation of DASA-based polymers
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 4
year: '2022'
...
---
OA_type: closed access
_id: '21827'
article_processing_charge: No
article_type: original
author:
- first_name: Friedrich J
  full_name: Stricker, Friedrich J
  id: 7aca2cfc-46cf-11f0-abd3-8c96b5186745
  last_name: Stricker
- first_name: Peterson
  full_name: Julie, Peterson
  last_name: Julie
- first_name: Read de Alaniz
  full_name: Javier, Read de Alaniz
  last_name: Javier
citation:
  ama: 'Stricker FJ, Julie P, Javier R de A. Preparation of a donor-acceptor Stenhouse
    Adduct (DASA): 5-((2Z,4E)-5-(diethylamino)-2-hydroxypenta-2,4-dien-1-ylidene)-2,2-dimethyl-1,3-dioxane-4,6-dione.
    <i>Organic Syntheses</i>. 2022;99:79-91. doi:<a href="https://doi.org/10.15227/orgsyn.099.0079">10.15227/orgsyn.099.0079</a>'
  apa: 'Stricker, F. J., Julie, P., &#38; Javier, R. de A. (2022). Preparation of
    a donor-acceptor Stenhouse Adduct (DASA): 5-((2Z,4E)-5-(diethylamino)-2-hydroxypenta-2,4-dien-1-ylidene)-2,2-dimethyl-1,3-dioxane-4,6-dione.
    <i>Organic Syntheses</i>. Organic Syntheses. <a href="https://doi.org/10.15227/orgsyn.099.0079">https://doi.org/10.15227/orgsyn.099.0079</a>'
  chicago: 'Stricker, Friedrich J, Peterson Julie, and Read de Alaniz Javier. “Preparation
    of a Donor-Acceptor Stenhouse Adduct (DASA): 5-((2Z,4E)-5-(Diethylamino)-2-Hydroxypenta-2,4-Dien-1-Ylidene)-2,2-Dimethyl-1,3-Dioxane-4,6-Dione.”
    <i>Organic Syntheses</i>. Organic Syntheses, 2022. <a href="https://doi.org/10.15227/orgsyn.099.0079">https://doi.org/10.15227/orgsyn.099.0079</a>.'
  ieee: 'F. J. Stricker, P. Julie, and R. de A. Javier, “Preparation of a donor-acceptor
    Stenhouse Adduct (DASA): 5-((2Z,4E)-5-(diethylamino)-2-hydroxypenta-2,4-dien-1-ylidene)-2,2-dimethyl-1,3-dioxane-4,6-dione,”
    <i>Organic Syntheses</i>, vol. 99. Organic Syntheses, pp. 79–91, 2022.'
  ista: 'Stricker FJ, Julie P, Javier R de A. 2022. Preparation of a donor-acceptor
    Stenhouse Adduct (DASA): 5-((2Z,4E)-5-(diethylamino)-2-hydroxypenta-2,4-dien-1-ylidene)-2,2-dimethyl-1,3-dioxane-4,6-dione.
    Organic Syntheses. 99, 79–91.'
  mla: 'Stricker, Friedrich J., et al. “Preparation of a Donor-Acceptor Stenhouse
    Adduct (DASA): 5-((2Z,4E)-5-(Diethylamino)-2-Hydroxypenta-2,4-Dien-1-Ylidene)-2,2-Dimethyl-1,3-Dioxane-4,6-Dione.”
    <i>Organic Syntheses</i>, vol. 99, Organic Syntheses, 2022, pp. 79–91, doi:<a
    href="https://doi.org/10.15227/orgsyn.099.0079">10.15227/orgsyn.099.0079</a>.'
  short: F.J. Stricker, P. Julie, R. de A. Javier, Organic Syntheses 99 (2022) 79–91.
date_created: 2026-05-06T11:10:35Z
date_published: 2022-05-23T00:00:00Z
date_updated: 2026-05-12T06:52:08Z
day: '23'
ddc:
- '540'
doi: 10.15227/orgsyn.099.0079
extern: '1'
intvolume: '        99'
language:
- iso: eng
month: '05'
oa_version: None
page: 79-91
publication: Organic Syntheses
publication_identifier:
  eissn:
  - 2333-3553
  issnl:
  - 0078-6209
publication_status: published
publisher: Organic Syntheses
quality_controlled: '1'
status: public
title: 'Preparation of a donor-acceptor Stenhouse Adduct (DASA): 5-((2Z,4E)-5-(diethylamino)-2-hydroxypenta-2,4-dien-1-ylidene)-2,2-dimethyl-1,3-dioxane-4,6-dione'
type: journal_article
user_id: ba8df636-2132-11f1-aed0-ed93e2281fdd
volume: 99
year: '2022'
...
---
OA_type: closed access
_id: '21828'
abstract:
- lang: eng
  text: Donor–acceptor Stenhouse adducts (DASA) are a reported class of visible-light-activated
    photoswitches. DASA synthesis involves two steps using furfural as starting material,
    while their complex photoswitching mechanism consists both of actinic and thermal
    steps. As a result of their visible-light activation, negative photochromism,
    large volume and polarity change, and wavelength tunability, DASAs present significant
    promise toward light-activated materials. In the years since their first report
    in 2014, a number of applications have utilized DASA ranging from selective cargo
    release over controlled phase transfer to directed flow in solution.
article_processing_charge: No
author:
- first_name: Friedrich J
  full_name: Stricker, Friedrich J
  id: 7aca2cfc-46cf-11f0-abd3-8c96b5186745
  last_name: Stricker
- first_name: Serena
  full_name: Seshadri, Serena
  last_name: Seshadri
- first_name: Javier Read
  full_name: de Alaniz, Javier Read
  last_name: de Alaniz
citation:
  ama: 'Stricker FJ, Seshadri S, de Alaniz JR. Donor-Acceptor Stenhouse Adducts. In:
    Pianowski Z, ed. <i>Molecular Photoswitches: Chemistry, Properties, and Applications</i>.
    Weinheim: Wiley; 2022:303-324. doi:<a href="https://doi.org/10.1002/9783527827626.ch14">10.1002/9783527827626.ch14</a>'
  apa: 'Stricker, F. J., Seshadri, S., &#38; de Alaniz, J. R. (2022). Donor-Acceptor
    Stenhouse Adducts. In Z. Pianowski (Ed.), <i>Molecular Photoswitches: Chemistry,
    Properties, and Applications</i> (pp. 303–324). Weinheim: Wiley. <a href="https://doi.org/10.1002/9783527827626.ch14">https://doi.org/10.1002/9783527827626.ch14</a>'
  chicago: 'Stricker, Friedrich J, Serena Seshadri, and Javier Read de Alaniz. “Donor-Acceptor
    Stenhouse Adducts.” In <i>Molecular Photoswitches: Chemistry, Properties, and
    Applications</i>, edited by Zbigniew Pianowski, 303–24. Weinheim: Wiley, 2022.
    <a href="https://doi.org/10.1002/9783527827626.ch14">https://doi.org/10.1002/9783527827626.ch14</a>.'
  ieee: 'F. J. Stricker, S. Seshadri, and J. R. de Alaniz, “Donor-Acceptor Stenhouse
    Adducts,” in <i>Molecular Photoswitches: Chemistry, Properties, and Applications</i>,
    Z. Pianowski, Ed. Weinheim: Wiley, 2022, pp. 303–324.'
  ista: 'Stricker FJ, Seshadri S, de Alaniz JR. 2022.Donor-Acceptor Stenhouse Adducts.
    In: Molecular Photoswitches: Chemistry, Properties, and Applications. , 303–324.'
  mla: 'Stricker, Friedrich J., et al. “Donor-Acceptor Stenhouse Adducts.” <i>Molecular
    Photoswitches: Chemistry, Properties, and Applications</i>, edited by Zbigniew
    Pianowski, Wiley, 2022, pp. 303–24, doi:<a href="https://doi.org/10.1002/9783527827626.ch14">10.1002/9783527827626.ch14</a>.'
  short: 'F.J. Stricker, S. Seshadri, J.R. de Alaniz, in:, Z. Pianowski (Ed.), Molecular
    Photoswitches: Chemistry, Properties, and Applications, Wiley, Weinheim, 2022,
    pp. 303–324.'
date_created: 2026-05-06T11:15:39Z
date_published: 2022-06-03T00:00:00Z
date_updated: 2026-05-12T08:16:46Z
day: '03'
doi: 10.1002/9783527827626.ch14
editor:
- first_name: Zbigniew
  full_name: Pianowski, Zbigniew
  last_name: Pianowski
extern: '1'
language:
- iso: eng
month: '06'
oa_version: None
page: 303-324
place: Weinheim
publication: 'Molecular Photoswitches: Chemistry, Properties, and Applications'
publication_identifier:
  eisbn:
  - '9783527827626'
  isbn:
  - '9783527347681'
publication_status: published
publisher: Wiley
quality_controlled: '1'
status: public
title: Donor-Acceptor Stenhouse Adducts
type: book_chapter
user_id: ba8df636-2132-11f1-aed0-ed93e2281fdd
year: '2022'
...
---
_id: '13445'
abstract:
- lang: eng
  text: Rotation is typically assumed to induce strictly symmetric rotational splitting
    into the rotational multiplets of pure p- and g-modes. However, for evolved stars
    exhibiting mixed modes, avoided crossings between different multiplet components
    are known to yield asymmetric rotational splitting, in particular for near-degenerate
    mixed-mode pairs, where notional pure p-modes are fortuitously in resonance with
    pure g-modes. These near-degeneracy effects have been described in subgiants,
    but their consequences for the characterization of internal rotation in red giants
    have not previously been investigated in detail, in part owing to theoretical
    intractability. We employ new developments in the analytic theory of mixed-mode
    coupling to study these near-resonance phenomena. In the vicinity of the most
    p-dominated mixed modes, the near-degenerate intrinsic asymmetry from pure rotational
    splitting increases dramatically over the course of stellar evolution, and it
    depends strongly on the mode-mixing fraction ζ. We also find that a linear treatment
    of rotation remains viable for describing the underlying p- and g-modes, even
    when it does not for the resulting mixed modes undergoing these avoided crossings.
    We explore observational consequences for potential measurements of asymmetric
    mixed-mode splitting, which has been proposed as a magnetic-field diagnostic.
    Finally, we propose improved measurement techniques for rotational characterization,
    exploiting the linearity of rotational effects on the underlying p/g-modes, while
    still accounting for these mixed-mode coupling effects.
article_number: '18'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: J. M. Joel
  full_name: Ong, J. M. Joel
  last_name: Ong
- 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: Sarbani
  full_name: Basu, Sarbani
  last_name: Basu
citation:
  ama: Ong JMJ, Bugnet LA, Basu S. Mode mixing and rotational splittings. I. Near-degeneracy
    effects revisited. <i>The Astrophysical Journal</i>. 2022;940(1). doi:<a href="https://doi.org/10.3847/1538-4357/ac97e7">10.3847/1538-4357/ac97e7</a>
  apa: Ong, J. M. J., Bugnet, L. A., &#38; Basu, S. (2022). Mode mixing and rotational
    splittings. I. Near-degeneracy effects revisited. <i>The Astrophysical Journal</i>.
    American Astronomical Society. <a href="https://doi.org/10.3847/1538-4357/ac97e7">https://doi.org/10.3847/1538-4357/ac97e7</a>
  chicago: Ong, J. M. Joel, Lisa Annabelle Bugnet, and Sarbani Basu. “Mode Mixing
    and Rotational Splittings. I. Near-Degeneracy Effects Revisited.” <i>The Astrophysical
    Journal</i>. American Astronomical Society, 2022. <a href="https://doi.org/10.3847/1538-4357/ac97e7">https://doi.org/10.3847/1538-4357/ac97e7</a>.
  ieee: J. M. J. Ong, L. A. Bugnet, and S. Basu, “Mode mixing and rotational splittings.
    I. Near-degeneracy effects revisited,” <i>The Astrophysical Journal</i>, vol.
    940, no. 1. American Astronomical Society, 2022.
  ista: Ong JMJ, Bugnet LA, Basu S. 2022. Mode mixing and rotational splittings. I.
    Near-degeneracy effects revisited. The Astrophysical Journal. 940(1), 18.
  mla: Ong, J. M. Joel, et al. “Mode Mixing and Rotational Splittings. I. Near-Degeneracy
    Effects Revisited.” <i>The Astrophysical Journal</i>, vol. 940, no. 1, 18, American
    Astronomical Society, 2022, doi:<a href="https://doi.org/10.3847/1538-4357/ac97e7">10.3847/1538-4357/ac97e7</a>.
  short: J.M.J. Ong, L.A. Bugnet, S. Basu, The Astrophysical Journal 940 (2022).
date_created: 2023-08-01T14:20:41Z
date_published: 2022-11-16T00:00:00Z
date_updated: 2023-09-06T07:27:45Z
day: '16'
doi: 10.3847/1538-4357/ac97e7
extern: '1'
external_id:
  arxiv:
  - '2210.01928'
intvolume: '       940'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2210.01928
month: '11'
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: Mode mixing and rotational splittings. I. Near-degeneracy effects revisited
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 940
year: '2022'
...
---
_id: '13451'
abstract:
- lang: eng
  text: 'We characterize massive stars (M > 8 M⊙) in the nearby (D ∼ 0.8 Mpc) extremely
    metal-poor (Z ∼ 5% Z⊙) galaxy Leo A using Hubble Space Telescope ultraviolet (UV),
    optical, and near-infrared (NIR) imaging along with Keck/Low-Resolution Imaging
    Spectrograph and MMT/Binospec optical spectroscopy for 18 main-sequence OB stars.
    We find that: (a) 12 of our 18 stars show emission lines, despite not being associated
    with an H ii region, suggestive of stellar activity (e.g., mass loss, accretion,
    binary star interaction), which is consistent with previous predictions of enhanced
    activity at low metallicity; (b) six are Be stars, which are the first to be spectroscopically
    studied at such low metallicity—these Be stars have unusual panchromatic SEDs;
    (c) for stars well fit by the TLUSTY nonlocal thermodynamic equilibrium models,
    the photometric and spectroscopic values of $\mathrm{log}({T}_{\mathrm{eff}})$
    and $\mathrm{log}(g)$ agree to within ∼0.01 dex and ∼0.18 dex, respectively, indicating
    that near-UV/optical/NIR imaging can be used to reliably characterize massive
    (M ∼ 8–30 M⊙) main-sequence star properties relative to optical spectroscopy;
    (d) the properties of the most-massive stars in H II regions are consistent with
    constraints from previous nebular emission line studies; and (e) 13 stars with
    M > 8M⊙ are >40 pc from a known star cluster or H II region. Our sample comprises
    ∼50% of all known massive stars at Z ≲ 10% Z⊙with derived stellar parameters,
    high-quality optical spectra, and panchromatic photometry.'
article_number: '206'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Maude
  full_name: Gull, Maude
  last_name: Gull
- first_name: Daniel R.
  full_name: Weisz, Daniel R.
  last_name: Weisz
- first_name: Peter
  full_name: Senchyna, Peter
  last_name: Senchyna
- first_name: Nathan R.
  full_name: Sandford, Nathan R.
  last_name: Sandford
- first_name: Yumi
  full_name: Choi, Yumi
  last_name: Choi
- first_name: Anna F.
  full_name: McLeod, Anna F.
  last_name: McLeod
- first_name: Kareem
  full_name: El-Badry, Kareem
  last_name: El-Badry
- 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: Karoline M.
  full_name: Gilbert, Karoline M.
  last_name: Gilbert
- first_name: Martha
  full_name: Boyer, Martha
  last_name: Boyer
- first_name: Julianne J.
  full_name: Dalcanton, Julianne J.
  last_name: Dalcanton
- first_name: Puragra
  full_name: GuhaThakurta, Puragra
  last_name: GuhaThakurta
- first_name: Steven
  full_name: Goldman, Steven
  last_name: Goldman
- first_name: Paola
  full_name: Marigo, Paola
  last_name: Marigo
- first_name: Kristen B. W.
  full_name: McQuinn, Kristen B. W.
  last_name: McQuinn
- first_name: Giada
  full_name: Pastorelli, Giada
  last_name: Pastorelli
- first_name: Daniel P.
  full_name: Stark, Daniel P.
  last_name: Stark
- first_name: Evan
  full_name: Skillman, Evan
  last_name: Skillman
- first_name: Yuan-sen
  full_name: Ting, Yuan-sen
  last_name: Ting
- first_name: Benjamin F.
  full_name: Williams, Benjamin F.
  last_name: Williams
citation:
  ama: Gull M, Weisz DR, Senchyna P, et al. A panchromatic study of massive stars
    in the extremely metal-poor local group dwarf galaxy Leo A. <i>The Astrophysical
    Journal</i>. 2022;941(2). doi:<a href="https://doi.org/10.3847/1538-4357/aca295">10.3847/1538-4357/aca295</a>
  apa: Gull, M., Weisz, D. R., Senchyna, P., Sandford, N. R., Choi, Y., McLeod, A.
    F., … Williams, B. F. (2022). A panchromatic study of massive stars in the extremely
    metal-poor local group dwarf galaxy Leo A. <i>The Astrophysical Journal</i>. American
    Astronomical Society. <a href="https://doi.org/10.3847/1538-4357/aca295">https://doi.org/10.3847/1538-4357/aca295</a>
  chicago: Gull, Maude, Daniel R. Weisz, Peter Senchyna, Nathan R. Sandford, Yumi
    Choi, Anna F. McLeod, Kareem El-Badry, et al. “A Panchromatic Study of Massive
    Stars in the Extremely Metal-Poor Local Group Dwarf Galaxy Leo A.” <i>The Astrophysical
    Journal</i>. American Astronomical Society, 2022. <a href="https://doi.org/10.3847/1538-4357/aca295">https://doi.org/10.3847/1538-4357/aca295</a>.
  ieee: M. Gull <i>et al.</i>, “A panchromatic study of massive stars in the extremely
    metal-poor local group dwarf galaxy Leo A,” <i>The Astrophysical Journal</i>,
    vol. 941, no. 2. American Astronomical Society, 2022.
  ista: Gull M, Weisz DR, Senchyna P, Sandford NR, Choi Y, McLeod AF, El-Badry K,
    Götberg YLL, Gilbert KM, Boyer M, Dalcanton JJ, GuhaThakurta P, Goldman S, Marigo
    P, McQuinn KBW, Pastorelli G, Stark DP, Skillman E, Ting Y, Williams BF. 2022.
    A panchromatic study of massive stars in the extremely metal-poor local group
    dwarf galaxy Leo A. The Astrophysical Journal. 941(2), 206.
  mla: Gull, Maude, et al. “A Panchromatic Study of Massive Stars in the Extremely
    Metal-Poor Local Group Dwarf Galaxy Leo A.” <i>The Astrophysical Journal</i>,
    vol. 941, no. 2, 206, American Astronomical Society, 2022, doi:<a href="https://doi.org/10.3847/1538-4357/aca295">10.3847/1538-4357/aca295</a>.
  short: M. Gull, D.R. Weisz, P. Senchyna, N.R. Sandford, Y. Choi, A.F. McLeod, K.
    El-Badry, Y.L.L. Götberg, K.M. Gilbert, M. Boyer, J.J. Dalcanton, P. GuhaThakurta,
    S. Goldman, P. Marigo, K.B.W. McQuinn, G. Pastorelli, D.P. Stark, E. Skillman,
    Y. Ting, B.F. Williams, The Astrophysical Journal 941 (2022).
date_created: 2023-08-03T10:10:25Z
date_published: 2022-12-27T00:00:00Z
date_updated: 2023-08-21T12:04:58Z
day: '27'
doi: 10.3847/1538-4357/aca295
extern: '1'
external_id:
  arxiv:
  - '2211.14349'
intvolume: '       941'
issue: '2'
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/aca295
month: '12'
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: A panchromatic study of massive stars in the extremely metal-poor local group
  dwarf galaxy Leo A
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 941
year: '2022'
...
---
_id: '13452'
abstract:
- lang: eng
  text: Magnetic fields can drastically change predictions of evolutionary models
    of massive stars via mass-loss quenching, magnetic braking, and efficient angular
    momentum transport, which we aim to quantify in this work. We use the MESA software
    instrument to compute an extensive main-sequence grid of stellar structure and
    evolution models, as well as isochrones, accounting for the effects attributed
    to a surface fossil magnetic field. The grid is densely populated in initial mass
    (3–60 M⊙), surface equatorial magnetic field strength (0–50 kG), and metallicity
    (representative of the Solar neighbourhood and the Magellanic Clouds). We use
    two magnetic braking and two chemical mixing schemes and compare the model predictions
    for slowly rotating, nitrogen-enriched (‘Group 2’) stars with observations in
    the Large Magellanic Cloud. We quantify a range of initial field strengths that
    allow for producing Group 2 stars and find that typical values (up to a few kG)
    lead to solutions. Between the subgrids, we find notable departures in surface
    abundances and evolutionary paths. In our magnetic models, chemical mixing is
    always less efficient compared to non-magnetic models due to the rapid spin-down.
    We identify that quasi-chemically homogeneous main sequence evolution by efficient
    mixing could be prevented by fossil magnetic fields. We recommend comparing this
    grid of evolutionary models with spectropolarimetric and spectroscopic observations
    with the goals of (i) revisiting the derived stellar parameters of known magnetic
    stars, and (ii) observationally constraining the uncertain magnetic braking and
    chemical mixing schemes.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Z
  full_name: Keszthelyi, Z
  last_name: Keszthelyi
- first_name: A
  full_name: de Koter, A
  last_name: de Koter
- 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: G
  full_name: Meynet, G
  last_name: Meynet
- first_name: S A
  full_name: Brands, S A
  last_name: Brands
- first_name: V
  full_name: Petit, V
  last_name: Petit
- first_name: M
  full_name: Carrington, M
  last_name: Carrington
- first_name: A
  full_name: David-Uraz, A
  last_name: David-Uraz
- first_name: S T
  full_name: Geen, S T
  last_name: Geen
- first_name: C
  full_name: Georgy, C
  last_name: Georgy
- first_name: R
  full_name: Hirschi, R
  last_name: Hirschi
- first_name: J
  full_name: Puls, J
  last_name: Puls
- first_name: K J
  full_name: Ramalatswa, K J
  last_name: Ramalatswa
- first_name: M E
  full_name: Shultz, M E
  last_name: Shultz
- first_name: A
  full_name: ud-Doula, A
  last_name: ud-Doula
citation:
  ama: 'Keszthelyi Z, de Koter A, Götberg YLL, et al. The effects of surface fossil
    magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC,
    and SMC metallicities. <i>Monthly Notices of the Royal Astronomical Society</i>.
    2022;517(2):2028-2055. doi:<a href="https://doi.org/10.1093/mnras/stac2598">10.1093/mnras/stac2598</a>'
  apa: 'Keszthelyi, Z., de Koter, A., Götberg, Y. L. L., Meynet, G., Brands, S. A.,
    Petit, V., … ud-Doula, A. (2022). The effects of surface fossil magnetic fields
    on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities.
    <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press.
    <a href="https://doi.org/10.1093/mnras/stac2598">https://doi.org/10.1093/mnras/stac2598</a>'
  chicago: 'Keszthelyi, Z, A de Koter, Ylva Louise Linsdotter Götberg, G Meynet, S
    A Brands, V Petit, M Carrington, et al. “The Effects of Surface Fossil Magnetic
    Fields on Massive Star Evolution: IV. Grids of Models at Solar, LMC, and SMC Metallicities.”
    <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press,
    2022. <a href="https://doi.org/10.1093/mnras/stac2598">https://doi.org/10.1093/mnras/stac2598</a>.'
  ieee: 'Z. Keszthelyi <i>et al.</i>, “The effects of surface fossil magnetic fields
    on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities,”
    <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 517, no. 2. Oxford
    University Press, pp. 2028–2055, 2022.'
  ista: 'Keszthelyi Z, de Koter A, Götberg YLL, Meynet G, Brands SA, Petit V, Carrington
    M, David-Uraz A, Geen ST, Georgy C, Hirschi R, Puls J, Ramalatswa KJ, Shultz ME,
    ud-Doula A. 2022. The effects of surface fossil magnetic fields on massive star
    evolution: IV. Grids of models at Solar, LMC, and SMC metallicities. Monthly Notices
    of the Royal Astronomical Society. 517(2), 2028–2055.'
  mla: 'Keszthelyi, Z., et al. “The Effects of Surface Fossil Magnetic Fields on Massive
    Star Evolution: IV. Grids of Models at Solar, LMC, and SMC Metallicities.” <i>Monthly
    Notices of the Royal Astronomical Society</i>, vol. 517, no. 2, Oxford University
    Press, 2022, pp. 2028–55, doi:<a href="https://doi.org/10.1093/mnras/stac2598">10.1093/mnras/stac2598</a>.'
  short: Z. Keszthelyi, A. de Koter, Y.L.L. Götberg, G. Meynet, S.A. Brands, V. Petit,
    M. Carrington, A. David-Uraz, S.T. Geen, C. Georgy, R. Hirschi, J. Puls, K.J.
    Ramalatswa, M.E. Shultz, A. ud-Doula, Monthly Notices of the Royal Astronomical
    Society 517 (2022) 2028–2055.
date_created: 2023-08-03T10:10:37Z
date_published: 2022-12-01T00:00:00Z
date_updated: 2023-08-21T12:02:17Z
day: '01'
doi: 10.1093/mnras/stac2598
extern: '1'
external_id:
  arxiv:
  - '2209.06350'
intvolume: '       517'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2209.06350
month: '12'
oa: 1
oa_version: Preprint
page: 2028-2055
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: 'The effects of surface fossil magnetic fields on massive star evolution: IV.
  Grids of models at Solar, LMC, and SMC metallicities'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 517
year: '2022'
...
---
_id: '13991'
abstract:
- lang: eng
  text: The prediction and realization of topological insulators have sparked great
    interest in experimental approaches to the classification of materials1,2,3. The
    phase transition between non-trivial and trivial topological states is important,
    not only for basic materials science but also for next-generation technology,
    such as dissipation-free electronics4. It is therefore crucial to develop advanced
    probes that are suitable for a wide range of samples and environments. Here we
    demonstrate that circularly polarized laser-field-driven high-harmonic generation
    is distinctly sensitive to the non-trivial and trivial topological phases in the
    prototypical three-dimensional topological insulator bismuth selenide5. The phase
    transition is chemically initiated by reducing the spin–orbit interaction strength
    through the substitution of bismuth with indium atoms6,7. We find strikingly different
    high-harmonic responses of trivial and non-trivial topological surface states
    that manifest themselves as a conversion efficiency and elliptical dichroism that
    depend both on the driving laser ellipticity and the crystal orientation. The
    origins of the anomalous high-harmonic response are corroborated by calculations
    using the semiconductor optical Bloch equations with pairs of surface and bulk
    bands. As a purely optical approach, this method offers sensitivity to the electronic
    structure of the material, including its nonlinear response, and is compatible
    with a wide range of samples and sample environments.
article_processing_charge: No
article_type: original
author:
- first_name: Christian
  full_name: Heide, Christian
  last_name: Heide
- first_name: Yuki
  full_name: Kobayashi, Yuki
  last_name: Kobayashi
- first_name: Denitsa Rangelova
  full_name: Baykusheva, Denitsa Rangelova
  id: 71b4d059-2a03-11ee-914d-dfa3beed6530
  last_name: Baykusheva
- first_name: Deepti
  full_name: Jain, Deepti
  last_name: Jain
- first_name: Jonathan A.
  full_name: Sobota, Jonathan A.
  last_name: Sobota
- first_name: Makoto
  full_name: Hashimoto, Makoto
  last_name: Hashimoto
- first_name: Patrick S.
  full_name: Kirchmann, Patrick S.
  last_name: Kirchmann
- first_name: Seongshik
  full_name: Oh, Seongshik
  last_name: Oh
- first_name: Tony F.
  full_name: Heinz, Tony F.
  last_name: Heinz
- first_name: David A.
  full_name: Reis, David A.
  last_name: Reis
- first_name: Shambhu
  full_name: Ghimire, Shambhu
  last_name: Ghimire
citation:
  ama: Heide C, Kobayashi Y, Baykusheva DR, et al. Probing topological phase transitions
    using high-harmonic generation. <i>Nature Photonics</i>. 2022;16(9):620-624. doi:<a
    href="https://doi.org/10.1038/s41566-022-01050-7">10.1038/s41566-022-01050-7</a>
  apa: Heide, C., Kobayashi, Y., Baykusheva, D. R., Jain, D., Sobota, J. A., Hashimoto,
    M., … Ghimire, S. (2022). Probing topological phase transitions using high-harmonic
    generation. <i>Nature Photonics</i>. Springer Nature. <a href="https://doi.org/10.1038/s41566-022-01050-7">https://doi.org/10.1038/s41566-022-01050-7</a>
  chicago: Heide, Christian, Yuki Kobayashi, Denitsa Rangelova Baykusheva, Deepti
    Jain, Jonathan A. Sobota, Makoto Hashimoto, Patrick S. Kirchmann, et al. “Probing
    Topological Phase Transitions Using High-Harmonic Generation.” <i>Nature Photonics</i>.
    Springer Nature, 2022. <a href="https://doi.org/10.1038/s41566-022-01050-7">https://doi.org/10.1038/s41566-022-01050-7</a>.
  ieee: C. Heide <i>et al.</i>, “Probing topological phase transitions using high-harmonic
    generation,” <i>Nature Photonics</i>, vol. 16, no. 9. Springer Nature, pp. 620–624,
    2022.
  ista: Heide C, Kobayashi Y, Baykusheva DR, Jain D, Sobota JA, Hashimoto M, Kirchmann
    PS, Oh S, Heinz TF, Reis DA, Ghimire S. 2022. Probing topological phase transitions
    using high-harmonic generation. Nature Photonics. 16(9), 620–624.
  mla: Heide, Christian, et al. “Probing Topological Phase Transitions Using High-Harmonic
    Generation.” <i>Nature Photonics</i>, vol. 16, no. 9, Springer Nature, 2022, pp.
    620–24, doi:<a href="https://doi.org/10.1038/s41566-022-01050-7">10.1038/s41566-022-01050-7</a>.
  short: C. Heide, Y. Kobayashi, D.R. Baykusheva, D. Jain, J.A. Sobota, M. Hashimoto,
    P.S. Kirchmann, S. Oh, T.F. Heinz, D.A. Reis, S. Ghimire, Nature Photonics 16
    (2022) 620–624.
date_created: 2023-08-09T13:07:51Z
date_published: 2022-09-01T00:00:00Z
date_updated: 2023-08-22T07:20:09Z
day: '01'
doi: 10.1038/s41566-022-01050-7
extern: '1'
intvolume: '        16'
issue: '9'
keyword:
- Atomic and Molecular Physics
- and Optics
- Electronic
- Optical and Magnetic Materials
language:
- iso: eng
month: '09'
oa_version: None
page: 620-624
publication: Nature Photonics
publication_identifier:
  eissn:
  - 1749-4893
  issn:
  - 1749-4885
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Probing topological phase transitions using high-harmonic generation
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 16
year: '2022'
...
---
_id: '13992'
abstract:
- lang: eng
  text: Understanding the chirality of molecular reaction pathways is essential for
    a broad range of fundamental and applied sciences. However, the current ability
    to probe chirality on the time scale of primary processes underlying chemical
    reactions remains very limited. Here, we demonstrate time-resolved photoelectron
    circular dichroism (TRPECD) with ultrashort circularly polarized vacuum-ultraviolet
    (VUV) pulses from a tabletop source. We demonstrate the capabilities of VUV-TRPECD
    by resolving the chirality changes in time during the photodissociation of atomic
    iodine from two chiral molecules. We identify several general key features of
    TRPECD, which include the ability to probe dynamical chirality along the complete
    photochemical reaction path, the sensitivity to the local chirality of the evolving
    scattering potential, and the influence of electron scattering off dissociating
    photofragments. Our results are interpreted by comparison with high-level ab-initio
    calculations of transient PECDs from molecular photoionization calculations. Our
    experimental and theoretical techniques define a general approach to femtochirality.
article_number: abq2811
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Vít
  full_name: Svoboda, Vít
  last_name: Svoboda
- first_name: Niraghatam Bhargava
  full_name: Ram, Niraghatam Bhargava
  last_name: Ram
- first_name: Denitsa Rangelova
  full_name: Baykusheva, Denitsa Rangelova
  id: 71b4d059-2a03-11ee-914d-dfa3beed6530
  last_name: Baykusheva
- first_name: Daniel
  full_name: Zindel, Daniel
  last_name: Zindel
- first_name: Max D. J.
  full_name: Waters, Max D. J.
  last_name: Waters
- first_name: Benjamin
  full_name: Spenger, Benjamin
  last_name: Spenger
- first_name: Manuel
  full_name: Ochsner, Manuel
  last_name: Ochsner
- first_name: Holger
  full_name: Herburger, Holger
  last_name: Herburger
- first_name: Jürgen
  full_name: Stohner, Jürgen
  last_name: Stohner
- first_name: Hans Jakob
  full_name: Wörner, Hans Jakob
  last_name: Wörner
citation:
  ama: Svoboda V, Ram NB, Baykusheva DR, et al. Femtosecond photoelectron circular
    dichroism of chemical reactions. <i>Science Advances</i>. 2022;8(28). doi:<a href="https://doi.org/10.1126/sciadv.abq2811">10.1126/sciadv.abq2811</a>
  apa: Svoboda, V., Ram, N. B., Baykusheva, D. R., Zindel, D., Waters, M. D. J., Spenger,
    B., … Wörner, H. J. (2022). Femtosecond photoelectron circular dichroism of chemical
    reactions. <i>Science Advances</i>. American Association for the Advancement of
    Science. <a href="https://doi.org/10.1126/sciadv.abq2811">https://doi.org/10.1126/sciadv.abq2811</a>
  chicago: Svoboda, Vít, Niraghatam Bhargava Ram, Denitsa Rangelova Baykusheva, Daniel
    Zindel, Max D. J. Waters, Benjamin Spenger, Manuel Ochsner, Holger Herburger,
    Jürgen Stohner, and Hans Jakob Wörner. “Femtosecond Photoelectron Circular Dichroism
    of Chemical Reactions.” <i>Science Advances</i>. American Association for the
    Advancement of Science, 2022. <a href="https://doi.org/10.1126/sciadv.abq2811">https://doi.org/10.1126/sciadv.abq2811</a>.
  ieee: V. Svoboda <i>et al.</i>, “Femtosecond photoelectron circular dichroism of
    chemical reactions,” <i>Science Advances</i>, vol. 8, no. 28. American Association
    for the Advancement of Science, 2022.
  ista: Svoboda V, Ram NB, Baykusheva DR, Zindel D, Waters MDJ, Spenger B, Ochsner
    M, Herburger H, Stohner J, Wörner HJ. 2022. Femtosecond photoelectron circular
    dichroism of chemical reactions. Science Advances. 8(28), abq2811.
  mla: Svoboda, Vít, et al. “Femtosecond Photoelectron Circular Dichroism of Chemical
    Reactions.” <i>Science Advances</i>, vol. 8, no. 28, abq2811, American Association
    for the Advancement of Science, 2022, doi:<a href="https://doi.org/10.1126/sciadv.abq2811">10.1126/sciadv.abq2811</a>.
  short: V. Svoboda, N.B. Ram, D.R. Baykusheva, D. Zindel, M.D.J. Waters, B. Spenger,
    M. Ochsner, H. Herburger, J. Stohner, H.J. Wörner, Science Advances 8 (2022).
date_created: 2023-08-09T13:08:04Z
date_published: 2022-07-15T00:00:00Z
date_updated: 2023-08-22T07:24:01Z
day: '15'
doi: 10.1126/sciadv.abq2811
extern: '1'
external_id:
  arxiv:
  - '2206.04099'
  pmid:
  - '35857523'
intvolume: '         8'
issue: '28'
keyword:
- Multidisciplinary
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1126/sciadv.abq2811
month: '07'
oa: 1
oa_version: Published Version
pmid: 1
publication: Science Advances
publication_identifier:
  eissn:
  - 2375-2548
publication_status: published
publisher: American Association for the Advancement of Science
quality_controlled: '1'
scopus_import: '1'
status: public
title: Femtosecond photoelectron circular dichroism of chemical reactions
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 8
year: '2022'
...
---
_id: '13993'
abstract:
- lang: eng
  text: Photoionization is a process taking place on attosecond time scales. How its
    properties evolve from isolated particles to the condensed phase is an open question
    of both fundamental and practical relevance. Here, we review recent work that
    has advanced the study of photoionization dynamics from atoms to molecules, clusters
    and the liquid phase. The first measurements of molecular photoionization delays
    have revealed the attosecond dynamics of electron emission from a molecular shape
    resonance and their sensitivity to the molecular potential. Using electron-ion
    coincidence spectroscopy these measurements have been extended from isolated molecules
    to clusters. A continuous increase of the delays with the water-cluster size has
    been observed up to a size of 4-5 molecules, followed by a saturation towards
    larger clusters. Comparison with calculations has revealed a correlation of the
    time delay with the spatial extension of the created electron hole. Using cylindrical
    liquid-microjet techniques, these measurements have also been extended to liquid
    water, revealing a delay relative to isolated water molecules that was very similar
    to the largest water clusters studied. Detailed modeling based on Monte-Carlo
    simulations confirmed that these delays are dominated by the contributions of
    the first two solvation shells, which agrees with the results of the cluster measurements.
    These combined results open the perspective of experimentally characterizing the
    delocalization of electronic wave functions in complex systems and studying their
    evolution on attosecond time scales.
article_processing_charge: No
article_type: original
author:
- first_name: Xiaochun
  full_name: Gong, Xiaochun
  last_name: Gong
- first_name: Inga
  full_name: Jordan, Inga
  last_name: Jordan
- first_name: Martin
  full_name: Huppert, Martin
  last_name: Huppert
- first_name: Saijoscha
  full_name: Heck, Saijoscha
  last_name: Heck
- first_name: Denitsa Rangelova
  full_name: Baykusheva, Denitsa Rangelova
  id: 71b4d059-2a03-11ee-914d-dfa3beed6530
  last_name: Baykusheva
- first_name: Denis
  full_name: Jelovina, Denis
  last_name: Jelovina
- first_name: Axel
  full_name: Schild, Axel
  last_name: Schild
- first_name: Hans Jakob
  full_name: Wörner, Hans Jakob
  last_name: Wörner
citation:
  ama: 'Gong X, Jordan I, Huppert M, et al. Attosecond photoionization dynamics: from
    molecules over clusters to the liquid phase. <i>Chimia</i>. 2022;76(6):520-528.
    doi:<a href="https://doi.org/10.2533/chimia.2022.520">10.2533/chimia.2022.520</a>'
  apa: 'Gong, X., Jordan, I., Huppert, M., Heck, S., Baykusheva, D. R., Jelovina,
    D., … Wörner, H. J. (2022). Attosecond photoionization dynamics: from molecules
    over clusters to the liquid phase. <i>Chimia</i>. Swiss Chemical Society. <a href="https://doi.org/10.2533/chimia.2022.520">https://doi.org/10.2533/chimia.2022.520</a>'
  chicago: 'Gong, Xiaochun, Inga Jordan, Martin Huppert, Saijoscha Heck, Denitsa Rangelova
    Baykusheva, Denis Jelovina, Axel Schild, and Hans Jakob Wörner. “Attosecond Photoionization
    Dynamics: From Molecules over Clusters to the Liquid Phase.” <i>Chimia</i>. Swiss
    Chemical Society, 2022. <a href="https://doi.org/10.2533/chimia.2022.520">https://doi.org/10.2533/chimia.2022.520</a>.'
  ieee: 'X. Gong <i>et al.</i>, “Attosecond photoionization dynamics: from molecules
    over clusters to the liquid phase,” <i>Chimia</i>, vol. 76, no. 6. Swiss Chemical
    Society, pp. 520–528, 2022.'
  ista: 'Gong X, Jordan I, Huppert M, Heck S, Baykusheva DR, Jelovina D, Schild A,
    Wörner HJ. 2022. Attosecond photoionization dynamics: from molecules over clusters
    to the liquid phase. Chimia. 76(6), 520–528.'
  mla: 'Gong, Xiaochun, et al. “Attosecond Photoionization Dynamics: From Molecules
    over Clusters to the Liquid Phase.” <i>Chimia</i>, vol. 76, no. 6, Swiss Chemical
    Society, 2022, pp. 520–28, doi:<a href="https://doi.org/10.2533/chimia.2022.520">10.2533/chimia.2022.520</a>.'
  short: X. Gong, I. Jordan, M. Huppert, S. Heck, D.R. Baykusheva, D. Jelovina, A.
    Schild, H.J. Wörner, Chimia 76 (2022) 520–528.
date_created: 2023-08-09T13:08:15Z
date_published: 2022-06-29T00:00:00Z
date_updated: 2023-08-22T07:26:39Z
day: '29'
doi: 10.2533/chimia.2022.520
extern: '1'
intvolume: '        76'
issue: '6'
keyword:
- General Medicine
- General Chemistry
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.2533/chimia.2022.520
month: '06'
oa: 1
oa_version: Published Version
page: 520-528
publication: Chimia
publication_identifier:
  eissn:
  - 2673-2424
  issn:
  - 0009-4293
publication_status: published
publisher: Swiss Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Attosecond photoionization dynamics: from molecules over clusters to the liquid
  phase'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 76
year: '2022'
...
---
_id: '13994'
abstract:
- lang: eng
  text: "Ultrafast lasers are an increasingly important tool to control and stabilize
    emergent phases in quantum materials. Among a variety of possible excitation protocols,
    a particularly intriguing route is the direct light engineering of microscopic
    electronic parameters, such as the electron hopping and the local Coulomb repulsion
    (Hubbard \r\nU). In this work, we use time-resolved x-ray absorption spectroscopy
    to demonstrate the light-induced renormalization of the Hubbard U in a cuprate
    superconductor, La1.905Ba0.095CuO4. We show that intense femtosecond laser pulses
    induce a substantial redshift of the upper Hubbard band while leaving the Zhang-Rice
    singlet energy unaffected. By comparing the experimental data to time-dependent
    spectra of single- and three-band Hubbard models, we assign this effect to an
    approximately 140-meV reduction of the on-site Coulomb repulsion on the copper
    sites. Our demonstration of a dynamical Hubbard U renormalization in a copper
    oxide paves the way to a novel strategy for the manipulation of superconductivity
    and magnetism as well as to the realization of other long-range-ordered phases
    in light-driven quantum materials."
article_number: '011013'
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: Hoyoung
  full_name: Jang, Hoyoung
  last_name: Jang
- first_name: Ali A.
  full_name: Husain, Ali A.
  last_name: Husain
- first_name: Sangjun
  full_name: Lee, Sangjun
  last_name: Lee
- first_name: Sophia F. R.
  full_name: TenHuisen, Sophia F. R.
  last_name: TenHuisen
- first_name: Preston
  full_name: Zhou, Preston
  last_name: Zhou
- first_name: Sunwook
  full_name: Park, Sunwook
  last_name: Park
- first_name: Hoon
  full_name: Kim, Hoon
  last_name: Kim
- first_name: Jin-Kwang
  full_name: Kim, Jin-Kwang
  last_name: Kim
- first_name: Hyeong-Do
  full_name: Kim, Hyeong-Do
  last_name: Kim
- first_name: Minseok
  full_name: Kim, Minseok
  last_name: Kim
- first_name: Sang-Youn
  full_name: Park, Sang-Youn
  last_name: Park
- first_name: Peter
  full_name: Abbamonte, Peter
  last_name: Abbamonte
- first_name: B. J.
  full_name: Kim, B. J.
  last_name: Kim
- first_name: G. D.
  full_name: Gu, G. D.
  last_name: Gu
- first_name: Yao
  full_name: Wang, Yao
  last_name: Wang
- first_name: Matteo
  full_name: Mitrano, Matteo
  last_name: Mitrano
citation:
  ama: Baykusheva DR, Jang H, Husain AA, et al. Ultrafast renormalization of the on-site
    Coulomb repulsion in a cuprate superconductor. <i>Physical Review X</i>. 2022;12(1).
    doi:<a href="https://doi.org/10.1103/physrevx.12.011013">10.1103/physrevx.12.011013</a>
  apa: Baykusheva, D. R., Jang, H., Husain, A. A., Lee, S., TenHuisen, S. F. R., Zhou,
    P., … Mitrano, M. (2022). Ultrafast renormalization of the on-site Coulomb repulsion
    in a cuprate superconductor. <i>Physical Review X</i>. American Physical Society.
    <a href="https://doi.org/10.1103/physrevx.12.011013">https://doi.org/10.1103/physrevx.12.011013</a>
  chicago: Baykusheva, Denitsa Rangelova, Hoyoung Jang, Ali A. Husain, Sangjun Lee,
    Sophia F. R. TenHuisen, Preston Zhou, Sunwook Park, et al. “Ultrafast Renormalization
    of the On-Site Coulomb Repulsion in a Cuprate Superconductor.” <i>Physical Review
    X</i>. American Physical Society, 2022. <a href="https://doi.org/10.1103/physrevx.12.011013">https://doi.org/10.1103/physrevx.12.011013</a>.
  ieee: D. R. Baykusheva <i>et al.</i>, “Ultrafast renormalization of the on-site
    Coulomb repulsion in a cuprate superconductor,” <i>Physical Review X</i>, vol.
    12, no. 1. American Physical Society, 2022.
  ista: Baykusheva DR, Jang H, Husain AA, Lee S, TenHuisen SFR, Zhou P, Park S, Kim
    H, Kim J-K, Kim H-D, Kim M, Park S-Y, Abbamonte P, Kim BJ, Gu GD, Wang Y, Mitrano
    M. 2022. Ultrafast renormalization of the on-site Coulomb repulsion in a cuprate
    superconductor. Physical Review X. 12(1), 011013.
  mla: Baykusheva, Denitsa Rangelova, et al. “Ultrafast Renormalization of the On-Site
    Coulomb Repulsion in a Cuprate Superconductor.” <i>Physical Review X</i>, vol.
    12, no. 1, 011013, American Physical Society, 2022, doi:<a href="https://doi.org/10.1103/physrevx.12.011013">10.1103/physrevx.12.011013</a>.
  short: D.R. Baykusheva, H. Jang, A.A. Husain, S. Lee, S.F.R. TenHuisen, P. Zhou,
    S. Park, H. Kim, J.-K. Kim, H.-D. Kim, M. Kim, S.-Y. Park, P. Abbamonte, B.J.
    Kim, G.D. Gu, Y. Wang, M. Mitrano, Physical Review X 12 (2022).
date_created: 2023-08-09T13:08:26Z
date_published: 2022-01-20T00:00:00Z
date_updated: 2024-10-14T12:23:26Z
day: '20'
doi: 10.1103/physrevx.12.011013
extern: '1'
external_id:
  arxiv:
  - '2109.13229'
intvolume: '        12'
issue: '1'
keyword:
- General Physics and Astronomy
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1103/PhysRevX.12.011013
month: '01'
oa: 1
oa_version: Published Version
publication: Physical Review X
publication_identifier:
  eissn:
  - 2160-3308
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Ultrafast renormalization of the on-site Coulomb repulsion in a cuprate superconductor
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 12
year: '2022'
...
---
_id: '14093'
abstract:
- lang: eng
  text: ' We propose a stochastic conditional gradient method (CGM) for minimizing
    convex finite-sum objectives formed as a sum of smooth and non-smooth terms. Existing
    CGM variants for this template either suffer from slow convergence rates, or require
    carefully increasing the batch size over the course of the algorithm’s execution,
    which leads to computing full gradients. In contrast, the proposed method, equipped
    with a stochastic average gradient (SAG) estimator, requires only one sample per
    iteration. Nevertheless, it guarantees fast convergence rates on par with more
    sophisticated variance reduction techniques. In applications we put special emphasis
    on problems with a large number of separable constraints. Such problems are prevalent
    among semidefinite programming (SDP) formulations arising in machine learning
    and theoretical computer science. We provide numerical experiments on matrix completion,
    unsupervised clustering, and sparsest-cut SDPs. '
alternative_title:
- PMLR
article_processing_charge: No
arxiv: 1
author:
- first_name: Gideon
  full_name: Dresdner, Gideon
  last_name: Dresdner
- first_name: Maria-Luiza
  full_name: Vladarean, Maria-Luiza
  last_name: Vladarean
- first_name: Gunnar
  full_name: Rätsch, Gunnar
  last_name: Rätsch
- first_name: Francesco
  full_name: Locatello, Francesco
  id: 26cfd52f-2483-11ee-8040-88983bcc06d4
  last_name: Locatello
  orcid: 0000-0002-4850-0683
- first_name: Volkan
  full_name: Cevher, Volkan
  last_name: Cevher
- first_name: Alp
  full_name: Yurtsever, Alp
  last_name: Yurtsever
citation:
  ama: 'Dresdner G, Vladarean M-L, Rätsch G, Locatello F, Cevher V, Yurtsever A.  Faster
    one-sample stochastic conditional gradient method for composite convex minimization.
    In: <i>Proceedings of the 25th International Conference on Artificial Intelligence
    and Statistics</i>. Vol 151. ML Research Press; 2022:8439-8457.'
  apa: 'Dresdner, G., Vladarean, M.-L., Rätsch, G., Locatello, F., Cevher, V., &#38;
    Yurtsever, A. (2022).  Faster one-sample stochastic conditional gradient method
    for composite convex minimization. In <i>Proceedings of the 25th International
    Conference on Artificial Intelligence and Statistics</i> (Vol. 151, pp. 8439–8457).
    Virtual: ML Research Press.'
  chicago: Dresdner, Gideon, Maria-Luiza Vladarean, Gunnar Rätsch, Francesco Locatello,
    Volkan Cevher, and Alp Yurtsever. “ Faster One-Sample Stochastic Conditional Gradient
    Method for Composite Convex Minimization.” In <i>Proceedings of the 25th International
    Conference on Artificial Intelligence and Statistics</i>, 151:8439–57. ML Research
    Press, 2022.
  ieee: G. Dresdner, M.-L. Vladarean, G. Rätsch, F. Locatello, V. Cevher, and A. Yurtsever,
    “ Faster one-sample stochastic conditional gradient method for composite convex
    minimization,” in <i>Proceedings of the 25th International Conference on Artificial
    Intelligence and Statistics</i>, Virtual, 2022, vol. 151, pp. 8439–8457.
  ista: 'Dresdner G, Vladarean M-L, Rätsch G, Locatello F, Cevher V, Yurtsever A.
    2022.  Faster one-sample stochastic conditional gradient method for composite
    convex minimization. Proceedings of the 25th International Conference on Artificial
    Intelligence and Statistics. AISTATS: Conference on Artificial Intelligence and
    Statistics, PMLR, vol. 151, 8439–8457.'
  mla: Dresdner, Gideon, et al. “ Faster One-Sample Stochastic Conditional Gradient
    Method for Composite Convex Minimization.” <i>Proceedings of the 25th International
    Conference on Artificial Intelligence and Statistics</i>, vol. 151, ML Research
    Press, 2022, pp. 8439–57.
  short: G. Dresdner, M.-L. Vladarean, G. Rätsch, F. Locatello, V. Cevher, A. Yurtsever,
    in:, Proceedings of the 25th International Conference on Artificial Intelligence
    and Statistics, ML Research Press, 2022, pp. 8439–8457.
conference:
  end_date: 2022-03-30
  location: Virtual
  name: 'AISTATS: Conference on Artificial Intelligence and Statistics'
  start_date: 2022-03-28
date_created: 2023-08-21T09:27:43Z
date_published: 2022-04-01T00:00:00Z
date_updated: 2023-09-06T10:28:17Z
day: '01'
department:
- _id: FrLo
extern: '1'
external_id:
  arxiv:
  - '2202.13212'
intvolume: '       151'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/2202.13212
month: '04'
oa: 1
oa_version: Preprint
page: 8439-8457
publication: Proceedings of the 25th International Conference on Artificial Intelligence
  and Statistics
publication_identifier:
  issn:
  - 2640-3498
publication_status: published
publisher: ML Research Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: ' Faster one-sample stochastic conditional gradient method for composite convex
  minimization'
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 151
year: '2022'
...
---
_id: '14098'
abstract:
- lang: eng
  text: Magnetic fields can drastically change predictions of evolutionary models
    of massive stars via mass-loss quenching, magnetic braking, and efficient angular
    momentum transport, which we aim to quantify in this work. We use the MESA software
    instrument to compute an extensive main-sequence grid of stellar structure and
    evolution models, as well as isochrones, accounting for the effects attributed
    to a surface fossil magnetic field. The grid is densely populated in initial mass
    (3–60 M⊙), surface equatorial magnetic field strength (0–50 kG), and metallicity
    (representative of the Solar neighbourhood and the Magellanic Clouds). We use
    two magnetic braking and two chemical mixing schemes and compare the model predictions
    for slowly rotating, nitrogen-enriched (‘Group 2’) stars with observations in
    the Large Magellanic Cloud. We quantify a range of initial field strengths that
    allow for producing Group 2 stars and find that typical values (up to a few kG)
    lead to solutions. Between the subgrids, we find notable departures in surface
    abundances and evolutionary paths. In our magnetic models, chemical mixing is
    always less efficient compared to non-magnetic models due to the rapid spin-down.
    We identify that quasi-chemically homogeneous main sequence evolution by efficient
    mixing could be prevented by fossil magnetic fields. We recommend comparing this
    grid of evolutionary models with spectropolarimetric and spectroscopic observations
    with the goals of (i) revisiting the derived stellar parameters of known magnetic
    stars, and (ii) observationally constraining the uncertain magnetic braking and
    chemical mixing schemes.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Z.
  full_name: Keszthelyi, Z.
  last_name: Keszthelyi
- first_name: A. de
  full_name: Koter, A. de
  last_name: Koter
- 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: G.
  full_name: Meynet, G.
  last_name: Meynet
- first_name: S. A.
  full_name: Brands, S. A.
  last_name: Brands
- first_name: V.
  full_name: Petit, V.
  last_name: Petit
- first_name: M.
  full_name: Carrington, M.
  last_name: Carrington
- first_name: A. David-Uraz
  full_name: A. David-Uraz, A. David-Uraz
  last_name: A. David-Uraz
- first_name: S. T.
  full_name: Geen, S. T.
  last_name: Geen
- first_name: C.
  full_name: Georgy, C.
  last_name: Georgy
- first_name: R.
  full_name: Hirschi, R.
  last_name: Hirschi
- first_name: J.
  full_name: Puls, J.
  last_name: Puls
- first_name: K. J.
  full_name: Ramalatswa, K. J.
  last_name: Ramalatswa
- first_name: M. E.
  full_name: Shultz, M. E.
  last_name: Shultz
- first_name: A. ud-Doula
  full_name: A. ud-Doula, A. ud-Doula
  last_name: A. ud-Doula
citation:
  ama: 'Keszthelyi Z, Koter A de, Götberg YLL, et al. The effects of surface fossil
    magnetic fields on massive star evolution: IV. Grids of models at solar, LMC,
    and SMC metallicities. <i>Monthly Notices of the Royal Astronomical Society</i>.
    2022;517(2):2028-2055. doi:<a href="https://doi.org/10.1093/mnras/stac2598">10.1093/mnras/stac2598</a>'
  apa: 'Keszthelyi, Z., Koter, A. de, Götberg, Y. L. L., Meynet, G., Brands, S. A.,
    Petit, V., … A. ud-Doula, A. ud-Doula. (2022). The effects of surface fossil magnetic
    fields on massive star evolution: IV. Grids of models at solar, LMC, and SMC metallicities.
    <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford Academic. <a
    href="https://doi.org/10.1093/mnras/stac2598">https://doi.org/10.1093/mnras/stac2598</a>'
  chicago: 'Keszthelyi, Z., A. de Koter, Ylva Louise Linsdotter Götberg, G. Meynet,
    S. A. Brands, V. Petit, M. Carrington, et al. “The Effects of Surface Fossil Magnetic
    Fields on Massive Star Evolution: IV. Grids of Models at Solar, LMC, and SMC Metallicities.”
    <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford Academic, 2022.
    <a href="https://doi.org/10.1093/mnras/stac2598">https://doi.org/10.1093/mnras/stac2598</a>.'
  ieee: 'Z. Keszthelyi <i>et al.</i>, “The effects of surface fossil magnetic fields
    on massive star evolution: IV. Grids of models at solar, LMC, and SMC metallicities,”
    <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 517, no. 2. Oxford
    Academic, pp. 2028–2055, 2022.'
  ista: 'Keszthelyi Z, Koter A de, Götberg YLL, Meynet G, Brands SA, Petit V, Carrington
    M, A. David-Uraz AD-U, Geen ST, Georgy C, Hirschi R, Puls J, Ramalatswa KJ, Shultz
    ME, A. ud-Doula A ud-Doula. 2022. The effects of surface fossil magnetic fields
    on massive star evolution: IV. Grids of models at solar, LMC, and SMC metallicities.
    Monthly Notices of the Royal Astronomical Society. 517(2), 2028–2055.'
  mla: 'Keszthelyi, Z., et al. “The Effects of Surface Fossil Magnetic Fields on Massive
    Star Evolution: IV. Grids of Models at Solar, LMC, and SMC Metallicities.” <i>Monthly
    Notices of the Royal Astronomical Society</i>, vol. 517, no. 2, Oxford Academic,
    2022, pp. 2028–55, doi:<a href="https://doi.org/10.1093/mnras/stac2598">10.1093/mnras/stac2598</a>.'
  short: Z. Keszthelyi, A. de Koter, Y.L.L. Götberg, G. Meynet, S.A. Brands, V. Petit,
    M. Carrington, A.D.-U. A. David-Uraz, S.T. Geen, C. Georgy, R. Hirschi, J. Puls,
    K.J. Ramalatswa, M.E. Shultz, A. ud-Doula A. ud-Doula, Monthly Notices of the
    Royal Astronomical Society 517 (2022) 2028–2055.
date_created: 2023-08-21T10:11:21Z
date_published: 2022-12-01T00:00:00Z
date_updated: 2023-08-22T13:18:34Z
day: '01'
doi: 10.1093/mnras/stac2598
extern: '1'
external_id:
  arxiv:
  - '2209.06350'
intvolume: '       517'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1093/mnras/stac2598
month: '12'
oa: 1
oa_version: Published Version
page: 2028-2055
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
  eissn:
  - 1365-2966
  issn:
  - 0035-8711
publication_status: published
publisher: Oxford Academic
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The effects of surface fossil magnetic fields on massive star evolution: IV.
  Grids of models at solar, LMC, and SMC metallicities'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 517
year: '2022'
...
---
_id: '14099'
abstract:
- lang: eng
  text: Magnetism can greatly impact the evolution of stars. In some stars with OBA
    spectral types there is direct evidence via the Zeeman effect for stable, large-scale
    magnetospheres, which lead to the spin-down of the stellar surface and reduced
    mass loss. So far, a comprehensive grid of stellar structure and evolution models
    accounting for these effects was lacking. For this reason, we computed and studied
    models with two magnetic braking and two chemical mixing schemes in three metallicity
    environments with the MESA software instrument. We find notable differences between
    the subgrids, which affects the model predictions and thus the detailed characterisation
    of stars. We are able to quantify the impact of magnetic fields in terms of preventing
    quasi-chemically homogeneous evolution and producing slowly-rotating, nitrogen-enriched
    ("Group 2") stars. Our model grid is fully open access and open source.
article_number: '2211.07060'
article_processing_charge: No
arxiv: 1
author:
- first_name: Z.
  full_name: Keszthelyi, Z.
  last_name: Keszthelyi
- first_name: A. de
  full_name: Koter, A. de
  last_name: Koter
- 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: G.
  full_name: Meynet, G.
  last_name: Meynet
- first_name: S. A.
  full_name: Brands, S. A.
  last_name: Brands
- first_name: V.
  full_name: Petit, V.
  last_name: Petit
- first_name: M.
  full_name: Carrington, M.
  last_name: Carrington
- first_name: A. David-Uraz
  full_name: A. David-Uraz, A. David-Uraz
  last_name: A. David-Uraz
- first_name: S. T.
  full_name: Geen, S. T.
  last_name: Geen
- first_name: C.
  full_name: Georgy, C.
  last_name: Georgy
- first_name: R.
  full_name: Hirschi, R.
  last_name: Hirschi
- first_name: J.
  full_name: Puls, J.
  last_name: Puls
- first_name: K. J.
  full_name: Ramalatswa, K. J.
  last_name: Ramalatswa
- first_name: M. E.
  full_name: Shultz, M. E.
  last_name: Shultz
- first_name: A. ud-Doula
  full_name: A. ud-Doula, A. ud-Doula
  last_name: A. ud-Doula
citation:
  ama: Keszthelyi Z, Koter A de, Götberg YLL, et al. Spin-down and reduced mass loss
    in early-type stars with large-scale magnetic fields. <i>arXiv</i>. doi:<a href="https://doi.org/10.48550/arXiv.2211.07060">10.48550/arXiv.2211.07060</a>
  apa: Keszthelyi, Z., Koter, A. de, Götberg, Y. L. L., Meynet, G., Brands, S. A.,
    Petit, V., … A. ud-Doula, A. ud-Doula. (n.d.). Spin-down and reduced mass loss
    in early-type stars with large-scale magnetic fields. <i>arXiv</i>. <a href="https://doi.org/10.48550/arXiv.2211.07060">https://doi.org/10.48550/arXiv.2211.07060</a>
  chicago: Keszthelyi, Z., A. de Koter, Ylva Louise Linsdotter Götberg, G. Meynet,
    S. A. Brands, V. Petit, M. Carrington, et al. “Spin-down and Reduced Mass Loss
    in Early-Type Stars with Large-Scale Magnetic Fields.” <i>ArXiv</i>, n.d. <a href="https://doi.org/10.48550/arXiv.2211.07060">https://doi.org/10.48550/arXiv.2211.07060</a>.
  ieee: Z. Keszthelyi <i>et al.</i>, “Spin-down and reduced mass loss in early-type
    stars with large-scale magnetic fields,” <i>arXiv</i>. .
  ista: Keszthelyi Z, Koter A de, Götberg YLL, Meynet G, Brands SA, Petit V, Carrington
    M, A. David-Uraz AD-U, Geen ST, Georgy C, Hirschi R, Puls J, Ramalatswa KJ, Shultz
    ME, A. ud-Doula A ud-Doula. Spin-down and reduced mass loss in early-type stars
    with large-scale magnetic fields. arXiv, 2211.07060.
  mla: Keszthelyi, Z., et al. “Spin-down and Reduced Mass Loss in Early-Type Stars
    with Large-Scale Magnetic Fields.” <i>ArXiv</i>, 2211.07060, doi:<a href="https://doi.org/10.48550/arXiv.2211.07060">10.48550/arXiv.2211.07060</a>.
  short: Z. Keszthelyi, A. de Koter, Y.L.L. Götberg, G. Meynet, S.A. Brands, V. Petit,
    M. Carrington, A.D.-U. A. David-Uraz, S.T. Geen, C. Georgy, R. Hirschi, J. Puls,
    K.J. Ramalatswa, M.E. Shultz, A. ud-Doula A. ud-Doula, ArXiv (n.d.).
date_created: 2023-08-21T10:11:37Z
date_published: 2022-11-14T00:00:00Z
date_updated: 2023-08-22T13:20:15Z
day: '14'
doi: 10.48550/arXiv.2211.07060
extern: '1'
external_id:
  arxiv:
  - '2211.07060'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.2211.07060
month: '11'
oa: 1
oa_version: Submitted Version
publication: arXiv
publication_status: submitted
status: public
title: Spin-down and reduced mass loss in early-type stars with large-scale magnetic
  fields
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2022'
...
