Direct URCA process in neutron stars with strong magnetic fields
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Direct URCA process in neutron stars with strong magnetic fields

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Direct URCA process in neutron stars with strong magnetic fields

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Leinson, L.B.; Pérez Cañellas, Armando
Aquest document és un/a article, creat/da en: 1998

Este documento está disponible también en : http://dx.doi.org/10.1088/1126-6708/1998/09/020
We calculate the emissivity for the direct URCA process in strongly magnetized, degenerate matter in neutron stars, under beta-equilibrium. We show that, if the magnetic field is large enough for protons and electrons to be confined to their ground Landau levels, the field-free threshold condition on proton concentration no longer holds, and direct URCA reactions are open for an arbitrary proton concentration. Direct URCA process leads to an early phase of fast neutron star cooling. This circumstance allows us to constrain the initial magnetic field inside observed pulsars.

    Leinson, L.B. Pérez Cañellas, Armando 1998 Direct URCA process in neutron stars with strong magnetic fields Journal of High Energy Physics 09 020
http://dx.doi.org/10.1088/1126-6708/1998/09/020
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