Corequake Model of Pulsar Glitches for Neutron Stars with Pion-Condensed Core

Details Corequake Model of Pulsar Glitches for Neutron Stars with Pion-Condensed Core Corequake Model of Pulsar Glitches for Neutron Stars with Pion-Condensed Core

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pthph..79..274t&link_type=abstract

Progress of Theoretical Physics, Vol. 79, No. 2, pp. 274-279

Physics

12

Scientific paper

From the viewpoint that combined (charged plus neutral) pion condensates
come into play in the core of massive ((1.4 - 1.6)M_{sun}) neutron
stars, a possible explanation for the remarkable difference in glitches
of Vela and Crab pulsars is given by applying a new version of corequake
model to Vela glitches.

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