High-spin effects in superdense matter

Details High-spin effects in superdense matter High-spin effects in superdense matter

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ncimb..65..427b&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 65 B, Oct. 11, 1981, p. 427-441.

Physics

Matter (Physics), Neutron Stars, Relativistic Effects, Space Density, Spin Dynamics, Supermassive Stars, Angular Velocity, Astronomical Models, Green'S Functions, Hartree Approximation, Self Consistent Fields, Stellar Rotation

Scientific paper

A model of relativistic interacting superdense matter with vector, scalar and symmetric second-rank tensor exchange is developed. The Green's functions of the model are solved in the self-consistent Hartree approximation. The contributions of the symmetric second-rank tensor are emphasized. It is found that these high-spin contributions affect the superdense matter at densities just beyond those predicted to occur in neutron star matter or nuclear collisions. The spin-two effects do produce an unusual asymptotic dependence, with pressure equal to -1/3 the energy density. This effect is examined in a simple model of the early universe.

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