On the neutrino cooling of quark stars

Details On the neutrino cooling of quark stars On the neutrino cooling of quark stars

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236..241b&link_type=abstract

Astrophysical Journal, Part 1, vol. 236, Feb. 15, 1980, p. 241-244.

Astronomy and Astrophysics

Astrophysics

2

Astrophysics, Cooling, Neutrinos, Quarks, Stellar Temperature, Supernova Remnants, Nebulae, Neutron Stars, Stellar Models, Surface Temperature

Scientific paper

The neutrino cooling rate of 'neutron' stars composed predominantly of a quark phase in their interiors has been computed and it is found that the temperature dependence and rate are about the same as for neutron matter near nuclear densities, though the specific heat for the quark matter is somewhat higher. The resulting cooling relation between surface temperature and time is compared with recent X-ray observations of young supernova remnants, two of which (the Crab and Gum nebulae) are known to contain collapsed objects.

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