Neutron star corequake implied by pion condensation - Dynamic, neutrino and thermal effects

Details Neutron star corequake implied by pion condensation - Dynamic, neutrino and thermal effects Neutron star corequake implied by pion condensation - Dynamic, neutrino and thermal effects

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...240...78h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 240, no. 1, Dec. 1990, p. 78-84.

Physics

Condensed Matter

7

Gravitational Collapse, Neutrinos, Neutron Stars, Pions, Starquakes, Condensed Matter Physics, Phase Transformations, Stellar Cores, Stellar Models, Stellar Oscillations

Scientific paper

Pion condensation near the center of a massive neutron star can induce a dynamic instability, leading to collapse to a new configuration with a pion condensed core. The hydrodynamics of the mini-collapse, and ensuing radial pulsations are studied for a realistic model of pion condensation. The neutrino burst and subsequent cooling of neutron star heated by the corequake are also studied.

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