Magnetars:. Internal Heating and Energy Budget

Details Magnetars:. Internal Heating and Energy Budget Magnetars:. Internal Heating and Energy Budget

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1189y&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

We develop models of magnetars as cooling neutron stars with an additional heating in a spherical internal layer. We show that in order to explain high observable thermal luminosities of magnetars and be consistent with the energy budget of neutron stars the heat source should be located in the outer neutron star crust and should have the heat intensity ~ 3 × 1020 erg cm-3 s-1.

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