Pion condensates in the VELA pulsar and the energetics of its glitch events

Details Pion condensates in the VELA pulsar and the energetics of its glitch events Pion condensates in the VELA pulsar and the energetics of its glitch events

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.187..329h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 187, no. 2, Jan. 1992, p. 329-332. Research supported by CNPq.

Astronomy and Astrophysics

Astrophysics

Nuclear Astrophysics, Pions, Pulsars, Stellar Interiors, X Ray Astronomy, Astronomical Models, Heao 2, Luminosity, Starquakes, Temperature Distribution

Scientific paper

The suggestion of Shapiro and Teukolsky (1983) that the peculiar features of pion condensates could provide a theoretical explanation for the glitch phenomenon is addressed. The arguments leading to this possibility are summarized and the way in which the existing data already constrain the viability of this model for the specific case of the Vela pulsar is discussed.

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