Authors

L. Clark, University of Glasgow
B. McKinnon, University of Glasgow
D. G. Ireland, University of Glasgow
D. I. Glazier, University of Glasgow
K. Livingston, University of Glasgow
D. Rönchen, Institute for Advanced Simulation (IAS-4), Forschungszentrum Jülich
A. G. Acar, University of York
P. Achenbach, Thomas Jefferson National Accelerator Facility
J. S. Alvarado, Université Paris-Saclay
M. J. Amaryan, Old Dominion UniversityFollow
W. R. Armstrong, Argonne National Laboratory
H. Atac, Temple University
L. Baashen, Florida International University
L. Barion, INFN, Sezione di Ferrara
M. Battaglieri, INFN, Sezione di Genova
B. Benkel, INFN Sezione di Roma Tor Vergata
F. Benmokhtar, Duquesne University
A. Bianconi, INFN Sezione di Pavia
A. S. Biselli, Fairfield University
W. A. Booth, University of York
F. Bossù, Université Paris-Saclay
K. Th. Brinkmann, II Physikalisches Institut der Universität Giessen
W. J. Briscoe, The George Washington University
W. K. Brooks, Universidad Técnica Federico Santa María
S. Bueltmann, Old Dominion UniversityFollow
T. Cao, Thomas Jefferson National Accelerator Facility
R. Capobianco, University of Connecticut
D. S. Carman, Thomas Jefferson National Accelerator Facility
A. Celentano, INFN Sezione di Genova
P. Chatagnon, Thomas Jefferson National Accelerator Facility
G. Ciullo, Universita' di Ferrara
P. L. Cole, Lamar University
M. Contalbrigo, INFN Sezione di Ferrara
A. D' Angelo, INFN Sezione di Ferrara
N. Dashyan, Yerevan Physics Institute
R. De Vita, INFN, Sezione di Genova
M. Defurne, Université Paris-Saclay
A. Deur, Thomas Jefferson National Accelerator Facility
S. Diehl, University of Connecticut
C. Djalali, Ohio University
M. Dugger, Arizona State University
R. Dupre, Université Paris-Saclay
H. Egiyan, Thomas Jefferson National Accelerator University
A. El Alaoui, Universidad Técnica Federico Santa María
L. El Fassi, Mississippi State University
P. Eugenio, Florida State University
S. Fegan, University of York
R. F. Ferguson, University of Glasgow
A. Filippi, INFN Sezione di Torino
C. Fogler, Old Dominion University
K. Gates, University of Glasgow
G. Gavalian, University of New Hampshire
G. P. Gilfoyle, University of Richmond
A. A. Golubenko, Skobeltsyn Institute of Nuclear Physics
R. W. Gothe, University of South Carolina
M. Guidal, Université Paris-Saclay
H. Hakobyan, Universidad Técnica Federico Santa María
M. Hattawy, Old Dominion UniversityFollow
F. Hauenstein, Thomas Jefferson National Accelerator FacilityFollow
T. B. Hayward, University of Connecticut
D. Heddle, Christopher Newport University
A. Hobart, Université Paris-Saclay
M. Holtrop, University of New Hampshire
E. L. Isupov, Skobeltsyn Institute of Nuclear Physics
D. Jenkins, Virginia Tech
H. Jiang, University of Glasgow
H. S. Jo, Kyungpook National University
D. Keller, University of Virginia
M. Khandaker, Norfolk State University
W. Kim, Kyungpook National University
F. J. Klein, The Catholic University of America
V. Klimenko, University of Connecticut
A. Kripko, II Physikalisches Institut der Universität Giessen
V. Kubarovsky, Thomas Jefferson National Accelerator Facility
L. Lanza, INFN, Sezione di Roma Tor Vergata
P. Lenisa, INFN Sezione di Ferrara
X. Li, Massachusetts Institute of Technology
I. J. D. MacGregor, University of Glasgow
D. Marchand, Université Paris-Saclay
V. Mascagna, INFN Sezione di Pavia
D. Matamoros, Université Paris-Saclay
S. Migliorati, INFN Sezione di Pavia
V. Mokeev, Thomas Jefferson National Accelerator Facility
C. Munoz Camacho, Université Paris-Saclay
P. Nadel-Turonski, Thomas Jefferson National Accelerator Facility
K. Neupane, University of South Carolina
S. Niccolai, Université Paris-Saclay
G. Niculescu, James Madison University
M. Osipenko, INFN, Sezione di Genova
P. Pandey, Massachusetts Institute of Technology
M. Paolone, New Mexico State University
L. L. Pappalardo, Universita' di Ferrara
R. Paremuzyan, Thomas Jefferson National Accelerator Facility
E. Pasyuk, Arizona State University
S. J. Paul, University of California Riverside
W. Phelps, Christopher Newport University
N. Pilleux, Université Paris-Saclay
M. Pokhrel, Old Dominion UniversityFollow
S. Polcher Rafael, Université Paris-Saclay
Y. Prok, Old Dominion UniversityFollow
T. Reed, Florida International University
J. Richards, University of Connecticut
M. Ripani, INFN, Sezione di Genova
B. G. Ritchie, Arizona State University
J. Ritman, GSI Helmholtzzentrum für Schwerionenforschung GmbH
G. Rosner, University of Glasgow
C. Salgado, Norfolk State University
S. Schadmand, GSI Helmholtzzentrum für Schwerionenforschung GmbH
A. Schmidt, The George Washington University
R. A. Schumacher, Carnegie Mellon University
Y. G. Sharabian, Thomas Jefferson National Accelerator Facility
E. V. Shirokov, Skobeltsyn Institute of Nuclear Physics
U. Shrestha, University of Connecticut
D. Sokhan, University of Glasgow
N. Sparveris, Temple University
M. Spreafico, INFN, Sezione di Genova
S. Stepanyan, Thomas Jefferson National Accelerator Facility
I. I. Strakovsky, The George Washington University
S. Stauch, University of South Carolina
J. A. Tan, Kyungpook National University
M. Tenorio, Old Dominion UniversityFollow
N. Trotta, University of Connecticut
R. Tyson, Thomas Jefferson National Accelerator Facility
M. Ungaro, Thomas Jefferson National Accelerator Facility
L. Venturelli, INFN Sezione di Pavia
H. Voskanyan, Yerevan Physics Institute
E. Voutier, Université Paris-Saclay
D. P. Watts, University of York
X. Wei, Thomas Jefferson National Accelerator Facility
R. Williams, University of York
L. Xu, Université Paris-Saclay
N. Zachariou, University of York
Z. W. Zhao, Duke University
M. Zurek, Argonne National Laboratory

Document Type

Article

Publication Date

2025

DOI

10.1103/PhysRevC.111.025204

Publication Title

Physical Review C

Volume

111

Issue

2

Pages

025204 (1-10)

Abstract

Background: Measurements of the polarization observables Σ, P, T, Ox, Ozfor the reaction 𝛾p →K⁰SΣ⁺ using a linearly polarized photon beam of energy 1.1 to 2.1 GeV are reported.

Purpose: The measured data provide information on a channel that has not been studied extensively, but is required for a full coupled-channel analysis in the nucleon resonance region.

Method: Observables have been simultaneously extracted using likelihood sampling with a Markov-Chain Monte Carlo process.

Results: Angular distributions in bins of photon energy Eγ are produced for each polarization observable. T,Ox,and Ozare first time measurements of these observables in this reaction. The extraction of Σ extends the energy range beyond a previous measurement. The measurement of P, the recoil polarization, is consistent with previous measurements.

Conclusions: The measured data are shown to be significant enough to affect the estimation of the nucleonresonance parameters when fitted within a coupled-channels model.

Rights

© The Authors 2025.

Published under the terms of the Creative Commons Attribution 4.0 International (CC BY 4.0) License. Further distribution must maintain attribution to the authors and the published article's title, journal citation, and DOI.

Original Publication Citation

Clark, L., McKinnon, B., Ireland, D. G., Glazier, D. I., Livingston, K., Rönchen, D., Acar, A. G., Achenbach, P., Alvarado, J. S., Amaryan, M. J., Armstrong, W. R., Atac, H., Baashen, L., Barion, L., Battaglieri, M., Benkel, B., Benmokhtar, F., Bianconi, A., Biselli, A. S.,…Zurek, M. (2025). Photoproduction of the Σ⁺ hyperon using linearly polarized photons with CLAS. Physical Review C, 111(2), 1-10, Article 025204. https://doi.org/10.1103/PhysRevC.111.025204

ORCID

0000-0003-2086-2807 (Hattawy)

Included in

Nuclear Commons

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