The effect of deconfinement phase transition on rotochemical deviations in stars containing mixed phase matter

Details The effect of deconfinement phase transition on rotochemical deviations in stars containing mixed phase matter The effect of deconfinement phase transition on rotochemical deviations in stars containing mixed phase matter

2011-04-16

arxiv.org/abs/1104.3223v3

MNRAS, 415(2011), 2665-2669

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

Scientific paper

10.1111/j.1365-2966.2011.18893.x

As a neutron star spins down, its core density increase, changing the relative equilibrium concentration, and causing deconfinement phase transition as well. hadron matter are converted into quark matter in the interior, which enhances the deviation of chemical equilibrium state. We study such deviations and its chemical energy release.Applying to the simulation of cooling neutron stars, we find the surface effective temperature of neutron stars is promoted obviously. This implies that the deconfinement phase transition is able to raise the chemical heating efficiency.

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