Equation of state of dense asymmetric nuclear matter

Details Equation of state of dense asymmetric nuclear matter Equation of state of dense asymmetric nuclear matter

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvl..59.1652t&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 59, Oct. 12, 1987, p. 1652-1655.

Statistics

Computation

41

Bosons, Dirac Equation, Equations Of State, Neutron Stars, Nuclear Physics, Supernovae, Computational Astrophysics, Lorentz Transformations, Nuclear Matter, Elementary Particle Processes

Scientific paper

Relativistic Dirac-Brueckner calculations, based on a one-boson-exchange interaction, are presented for the equation of state of asymmetric nuclear matter. For decreasing values of the ratio Z/A, it is shown that the saturation shifts to lower densities and the compression modulus at saturation drops. However, at high densities for all values of Z/A a stiff equation of state is observed, in contrast to the outcome of supernova calculations. The possibility of the occurrence of an antipion condensate is discussed.

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