Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5494828 | Physics Letters B | 2017 | 6 Pages |
Abstract
The calculation of the energy-, density-, and isospin-dependent Î production cross sections in nucleon-nucleon (NN) scattering ÏNNâNÎâ has been performed within the framework of the relativistic BUU approach. The NÎ cross sections are calculated in Born approximation taking into account the effective mass splitting of the nucleons and Îs in asymmetric matter. Due to the different mass splitting for neutron, proton and differently charged Îs, it is shown that, similar to the NN elastic ones, the reductions of NÎ inelastic cross sections in isospin-asymmetric nuclear medium are different from each other for all the individual channels and the effect is largest and of opposite sign for the Î++ and Îâ states. This approach is also compared to calculations without effective mass splitting and with splitting derived from Dirac-Brueckerner (DB) calculations. The isospin dependence of the NÎ cross sections is expected to influence the production of Ï+ and Ïâ mesons as well as their yield ratio, and thus affect the use of the latter quantity as a probe of the stiffness of the symmetry energy at supranormal densities.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Qingfeng Li, Zhuxia Li,