Neutron-proton bremsstrahlung from intermediate energy heavy-ion reactions as a probe of the nuclear symmetry energy?


Autoria(s): Yong, GC (Yong, Gao-Chan); Li, BA (Li, Bao-An); Chen, LW (Chen, Lie-Wen)
Data(s)

2008

Resumo

Hard photons from neutron-proton bremsstrahlung in intermediate energy heavy-ion reactions are examined as a potential probe of the nuclear symmetry energy within a transport model. Effects of the symmetry energy on the yields and spectra of hard photons are found to be generally smaller than those due to the currently existing uncertainties of both the in-medium nucleon-nucleon cross sections and the photon production probability in the elementary process pn -> pn gamma. Very interestingly, nevertheless, the ratio of hard photon spectra R-1/2(gamma) from two reactions using isotopes of the same element is not only approximately independent of these uncertainties but also quite sensitive to the symmetry energy. For the head-on reactions of Sn-132 + Sn-124 and Sn-112 + Sn-112 at E-beam/A = 50 MeV, for example, the R-1/2(gamma) displays a rise up to 15% when the symmetry energy is reduced by about 20% at rho = 1.3 rho(0) which is the maximum density reached in these reactions. (C) 2008 Elsevier B.V. All rights reserved.

Identificador

http://ir.impcas.ac.cn/handle/113462/5607

http://www.irgrid.ac.cn/handle/1471x/132402

Idioma(s)

英语

Fonte

Yong, GC (Yong, Gao-Chan); Li, BA (Li, Bao-An); Chen, LW (Chen, Lie-Wen) .Neutron-proton bremsstrahlung from intermediate energy heavy-ion reactions as a probe of the nuclear symmetry energy? ,PHYSICS LETTERS B ,2008,661(2-3):82-87

Palavras-Chave #HARD-PHOTON EMISSION #GAMMA-RAYS #COLLISIONS #PHYSICS #MODELS #RADII #STARS
Tipo

期刊论文