(Non)-Abelian gauge field theories of the Fermi gas. Neutron-quark stars

Details (Non)-Abelian gauge field theories of the Fermi gas. Neutron-quark stars (Non)-Abelian gauge field theories of the Fermi gas. Neutron-quark stars

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phlb...72..381b&link_type=abstract

Physics Letters B, Volume 72, Issue 3, p. 381-384.

Physics

34

Scientific paper

It is indicated that the ground state of Fermi systems with (non)-Abelian gauge interactions has a well defined quantum theory devoid of infrared divergences and mass singularities. This is exploited to develop a systematic quantum theory of the quark gas. The equation of state of the quark gas is evaluated up to second order in the Gell-Mann-Low charge αS(μ). The analysis based on neutron matter models suggests that the matter in the neutron stars can be in the quark phase provided the color interaction is ``moderately'' strong i.e. αS (3 GeV) <~ 0.3.

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