The density- and isospin- dependent -formation cross section and its decay width
arXiv:1712.02062 · doi:10.1007/S11433-018-9336-Y
Abstract
The energy-, density-, and isospin-dependent -formation cross section and -decay width are calculated based on the relativistic BUU approach in which the effective mass splitting of nucleon and baryons in isospin-asymmetric matter is considered by the inclusion of the meson exchange in the effective Lagrangian density. With the density-dependent couplings for baryons of F. Hofmann et al., the is decreased (increased) moderately with increasing density with (without) the consideration of the density dependent pion effective mass. Meanwhile, if the invariant mass of the system is not far from the pole mass, the -decay width is also weakly dependent on density. The mass splitting effect of differently charged nucleon and baryons on are found to be more obvious than that of pion mesons but much weaker than the mass splitting in the hard production channel . Further, the largest mass-splitting influence is seen in the and channels but not in the production of and isobars.
11 pages, 5 figures
References in corpus (7)
- Big-Bang Nucleosynthesis
- Symmetry energy from elliptic flow in 197Au + 197Au
- Systematics of central heavy ion collisions in the 1A GeV regime
- Comparison of heavy-ion transport simulations: Collision integral in a box
- In-medium effects on particle production in heavy ion collisions
- The width of the -resonance at two loop order in baryon chiral perturbation theory
- The effect of Lorentz-like force on collective flows of K in Au+Au collisions at 1.5 GeV/nucleon}{The effect of Lorentz-like force on collective flows of in Au+Au collisions at 1.5 GeV/nucleon