Published December 2005 | Version v1
Journal article

Nucleon-nucleon cross sections in neutron-rich matter and isospin transport in heavy-ion reactions at intermediate energies

  • 1. Department of Chemistry and Physics, P.O. Box 419, Arkansas State University, State University, Arkansas 72467-0419 (United States)
  • 2. Center of Theoretical Nuclear Physics, National Laboratory of Heavy Ion Accelerator, Lanzhou 730000 (China)
  • 3. Institute of Theoretical Physics, Shanghai Jiao Tong University, Shanghai 200240 (China)

Description

Nucleon-nucleon (NN) cross sections are evaluated in neutron-rich matter using a scaling model according to density, momentum, and isospin dependent nucleon effective masses. It is found that the in-medium NN cross sections are not only reduced but also have a different isospin dependence compared with the free-space ones. Because of the neutron-proton effective mass splitting the difference between nn and pp scattering cross sections increases with the increasing isospin asymmetry of the medium. Within the transport model IBUU04, the in-medium NN cross sections are found to influence significantly the isospin transport in heavy-ion reactions. With the in-medium NN cross sections, a symmetry energy of Esym(ρ)≅31.6(ρ/ρ0)0.69 was found most acceptable compared with both the MSU isospin diffusion data and the presently acceptable neutron-skin thickness in 208Pb. The isospin dependent part Kasy(ρ0) of isobaric nuclear incompressibility was further narrowed down to -500±50 MeV. The possibility of determining simultaneously the in-medium NN cross sections and the symmetry energy was also studied. The proton transverse flow, or even better the combined transverse flow of neutrons and protons, can be used as a probe of the in-medium NN cross sections without much hindrance from the uncertainties of the symmetry energy

Additional details

Publishing Information

Journal Title
Physical Review. C, Nuclear Physics
Journal Volume
72
Journal Issue
6
Journal Page Range
p. 064611-064611.12
ISSN
0556-2813
CODEN
PRVCAN

Optional Information

Notes
(c) 2005 The American Physical Society