Nuclear forces and the properties of matter at high temperature and density

Details Nuclear forces and the properties of matter at high temperature and density Nuclear forces and the properties of matter at high temperature and density

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...116..183r&link_type=abstract

Astronomy and Astrophysics, vol. 116, no. 1, Dec. 1982, p. 183-187.

Astronomy and Astrophysics

Astrophysics

49

Gravitational Collapse, Neutron Stars, Nuclear Chemistry, Stellar Evolution, Supernovae, Temperature Effects, Adiabatic Conditions, Cores, Elementary Particle Interactions, High Temperature Environments, Stellar Structure

Scientific paper

An effective nuclear force of the Skyrme type is proposed that is well suited for describing the nuclear matter in the presupernova core of a nascent neutron star. Results obtained using the proposed Skyrme force, called RATP, are compared with those obtained through the use of three other Skyrme forces. It is shown that both RATP and the Skyrme force known as T6 are equally valuable in the study of hot and/or dense nuclear matter.

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