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

Publishing date

Apr 1977

URL

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

Journals

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

Science

Physics

Additional info 2

27

Type

Scientific paper

Abstract

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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