The surface and inner temperatures of magnetars
classification
🌌 astro-ph.HE
keywords
effectivefieldinnerluminositymagneticneutrinosurfacetemperature
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Assuming that the timescale of the magnetic field decay is approximately equal to that of the stellar cooling via neutrino emission, we obtain a one-to-one relationship between the effective surface thermal temperature and the inner temperature. The ratio of the effective neutrino luminosity to the effective X-ray luminosity decreases with decaying magnetic field.
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