The neutrino emissivity of Urca process of strange quark matter in weak and ultra strong magnetic field

Details The neutrino emissivity of Urca process of strange quark matter in weak and ultra strong magnetic field The neutrino emissivity of Urca process of strange quark matter in weak and ultra strong magnetic field

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006acasn..47..247l&link_type=abstract

Acta Astronomica Sinica, vol. 47, no. 3, p.247-255

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Magnetic Fields, Dense Matter, Nuclear Reactions, Neutrinos, Stars: Neutron

Scientific paper

The effect of magnetic field on the neutrino emissivity of quark direct Urca process in strange stars is investigated. Firstly, calculating approach in weak magnetic field is improved, and it may be generalized to other weak interactions. Furthermore the neutino emissivity computed strictly for ultra magnetic field shows a strong dependence on magnetic field (proportion to the second power of magnetic field), and the emissivity depends on T5 instead of conventional T6.

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