Vibrational damping by quark matter inside neutron stars

Details Vibrational damping by quark matter inside neutron stars Vibrational damping by quark matter inside neutron stars

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acaps...5...59w&link_type=abstract

(Acta Astrophysica Sinica, vol. 5, no. 1, 1985, p. 59-66) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 9, June 1985

Physics

2

Neutron Stars, Quarks, Stellar Cores, Stellar Models, Vibration Damping, Stellar Physics, Weak Interactions (Field Theory)

Scientific paper

A free quark state may exist in the central region of massive neutron stars. The damping of the vibration of such neutron stars through the quark weak interaction is discussed. The damping time scale may be as short as tens of milliseconds. Damping with such short time constant may possibly be reflected in some gamma ray burst phenomena. An attempt is made to explain the gamma-ray burst of 1979 March 5 by this mechanism.

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