Possible role of strongly interacting fields in astrophysics and relativistic cosmology

Details Possible role of strongly interacting fields in astrophysics and relativistic cosmology Possible role of strongly interacting fields in astrophysics and relativistic cosmology

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....49..387k&link_type=abstract

Astronomy and Astrophysics, vol. 49, no. 3, June 1976, p. 387, 388.

Physics

Cosmology, Field Theory (Physics), Relativistic Theory, Stellar Evolution, Astronomical Models, Gravitational Collapse, Nucleons, Relativity, Saturation, Space Density

Scientific paper

A renormalizable scalar field theory with strong self-coupling and interaction with nucleons is considered. At a sufficiently high density, about twice the nuclear matter density, nucleons become massless. Saturation occurs at a slightly higher density, about 10 to the 15th power g/cu cm and matter is at the saturation point in a bound state. Possibilities are discussed for a third family of degenerate stars, 'clumps' of matter in cosmic rays, and possible violation of the energy condition for collapse to a singularity.

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