Free-quark phases in dense stars

Details Free-quark phases in dense stars Free-quark phases in dense stars

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976phlb...64..117k&link_type=abstract

Physics Letters B, Volume 64, Issue 1, p. 117-120.

Physics

52

Scientific paper

The possibility is examined that superdense matter can undergo a transition to a phase of free quarks within models which assume that the quark confinement potential is screened at high densities. The results imply that a phase of pure quarks of this type is unlikely to be found in stable stellar systems although they do not preclude the possible existence of a transition region which contains quarks and neutrons in equilibrium at the center of neutron stars.
Supported in part by National Science Foundation Grant PHY75-22555.

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