Probing the EOS of dense neutron-rich matter with high-energy radioactive beams
arXiv:nucl-th/0312026 · doi:10.1016/j.nuclphysa.2004.01.109
Abstract
Nuclear reactions induced by high energy radioactive beams create a transient state of nuclear matter with high density and appreciable neutron to proton asymmetry. This will provide a unique opportunity to explore novel properties of dense neutron-rich matter and the isospin-dependence of the nuclear equation of state (EOS). Here we study the ratio as a probe of the EOS of dense neutron-rich matter.
Talk given at NN2003 to appear in the Proc. in Nucl. Phys. A (2004)
References in corpus (3)
Cited by in corpus (5)
- The influence of cluster emission and the symmetry energy on neutron-proton spectral double ratios
- The Influence of in-medium NN cross-sections, symmetry potential and impact parameter on the isospin observables
- Probing the density dependence of symmetry energy via multifragmentation at sub-saturation densities
- Influence of density dependent symmetry energy on Elliptical flow
- Temperature dependence of nuclear matter generalized isovector symmetry energy with Skyrme-type interactions