Equation of State of Symmetric And Asymmetric Nuclear Matter At Various Densities And Temperatures

Details Equation of State of Symmetric And Asymmetric Nuclear Matter At Various Densities And Temperatures Equation of State of Symmetric And Asymmetric Nuclear Matter At Various Densities And Temperatures

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012jphcs.337a2014s&link_type=abstract

Journal of Physics: Conference Series, Volume 337, Issue 1, pp. 012014 (2012).

Physics

Scientific paper

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.

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