Equation of State of Symmetric And Asymmetric Nuclear Matter At Various Densities And Temperatures Conference Paper uri icon

abstract

  • The equation of state (EOS) of nuclear matter (NM) is an important ingredient in the study of properties of nuclei at and far from stability, of structures and evolution of compact astrophysical objects, such as neutron stars and core-collapse supernovae, and of heavy-ion collisions (HIC). We will review the current status of the EOS of NM, as deduced from theoretical and experimental studies of structure and reactions of nuclei.

published proceedings

  • NUCLEAR PHYSICS IN ASTROPHYSICS V

author list (cited authors)

  • Shlomo, S.

citation count

  • 4

complete list of authors

  • Shlomo, S

publication date

  • February 2012