Dense stellar matter in asymptotically free gauge theories: I. The high density limit

Details Dense stellar matter in asymptotically free gauge theories: I. The high density limit Dense stellar matter in asymptotically free gauge theories: I. The high density limit

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phlb...67..371k&link_type=abstract

Physics Letters B, Volume 67, Issue 3, p. 371-376.

Physics

27

Scientific paper

In asymptotically free gauge theories perturbation theory may be used to
obtain the behavior of dense stellar matter. The criteria for the
determination of ϱcrit, the minimum density above which
perturbation theory is valid, are presented. The asymptotic form for the
quark-gluon thermodynamic potential is given.

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