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Electroweak Form Factors of Baryons in Dense Nuclear Matter
by
G. Ramalho
G. Ramalho 1,*
,
K. Tsushima
K. Tsushima 2
and
Myung-Ki Cheoun
Myung-Ki Cheoun 1
1
Department of Physics and OMEG Institute, Soongsil University, Seoul 06978, Republic of Korea
2
Laboratório de Física Teórica e Computacional—LFTC, Programa de Posgraduação em Astrofísica e Física Computacional, Universidade Cidade de São Paulo, São Paulo 01506-000, SP, Brazil
*
Author to whom correspondence should be addressed.
Symmetry 2025, 17(5), 681; https://doi.org/10.3390/sym17050681 (registering DOI)
Submission received: 21 March 2025
/
Revised: 13 April 2025
/
Accepted: 18 April 2025
/
Published: 29 April 2025
Abstract
There is evidence that the properties of hadrons are modified in a nuclear medium. Information about the medium modifications of the internal structure of hadrons is fundamental for the study of dense nuclear matter and high-energy processes, including heavy-ion and nucleus–nucleus collisions. At the moment, however, empirical information about medium modifications of hadrons is limited; therefore, theoretical studies are essential for progress in the field. In the present work, we review theoretical studies of the electromagnetic and axial form factors of octet baryons in symmetric nuclear matter. The calculations are based on a model that takes into account the degrees of freedom revealed in experimental studies of low and intermediate square transfer momentum : valence quarks and meson cloud excitations of baryon cores. The formalism combines a covariant constituent quark model, developed for a free space (vacuum) with the quark–meson coupling model for extension to the nuclear medium. We conclude that the nuclear medium modifies the baryon properties differently according to the flavor content of the baryons and the medium density. The effects of the medium increase with density and are stronger (quenched or enhanced) for light baryons than for heavy baryons. In particular, the in-medium neutrino–nucleon and antineutrino–nucleon cross-sections are reduced compared to the values in free space. The proposed formalism can be extended to densities above the normal nuclear density and applied to neutrino–hyperon and antineutrino–hyperon scattering in dense nuclear matter.
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MDPI and ACS Style
Ramalho, G.; Tsushima, K.; Cheoun, M.-K.
Electroweak Form Factors of Baryons in Dense Nuclear Matter. Symmetry 2025, 17, 681.
https://doi.org/10.3390/sym17050681
AMA Style
Ramalho G, Tsushima K, Cheoun M-K.
Electroweak Form Factors of Baryons in Dense Nuclear Matter. Symmetry. 2025; 17(5):681.
https://doi.org/10.3390/sym17050681
Chicago/Turabian Style
Ramalho, G., K. Tsushima, and Myung-Ki Cheoun.
2025. "Electroweak Form Factors of Baryons in Dense Nuclear Matter" Symmetry 17, no. 5: 681.
https://doi.org/10.3390/sym17050681
APA Style
Ramalho, G., Tsushima, K., & Cheoun, M.-K.
(2025). Electroweak Form Factors of Baryons in Dense Nuclear Matter. Symmetry, 17(5), 681.
https://doi.org/10.3390/sym17050681
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