Effect of Pion Condensation on Keplerian Angular Frequency of Rotating Neutron Stars

Details Effect of Pion Condensation on Keplerian Angular Frequency of Rotating Neutron Stars Effect of Pion Condensation on Keplerian Angular Frequency of Rotating Neutron Stars

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pthph..85..175t&link_type=abstract

Progress of Theoretical Physics, Vol. 85, No. 2, pp. 175-180

Physics

4

Scientific paper

Keplerian angular frequency Omega_{K} for neutron stars with and without pion condensation is investigated for various equations of state which sustain 1.44 M_{sun} mass and satisfy causality. The Omega_{K} of pion-condensed stars becomes remarkably larger; by about (20 ~ 50)% for the star with ~ 1.5 M_{sun} mass, for instance. The absolute maximum of Omega_{K} amounts to (1.3 ~ 1.4) x 10(4) rad/s.

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