Rotation of stars containing strange quark matter

Details Rotation of stars containing strange quark matter Rotation of stars containing strange quark matter

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phlb..243..175p&link_type=abstract

Physics Letters B, Volume 243, Issue 3, p. 175-180.

Physics

35

Scientific paper

We calculate the maximum keplerian frequencies of stars containing strange matter that are in uniform rotation. We consider both self-bound stars and stars containing quark matter cores but normal surfaces. For both cases studied, use of perturbative QCD results for the equation of state of quark matter implies a limit on the maximum keplerian frequency of ~1×104s-1.

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