Thermal Evolution of Strange Stars
arXiv:0709.0214 · doi:10.1086/524711
Abstract
We investigated the thermal evolution of rotating strange stars with the deconfinement heating due to magnetic braking. We consider the stars consisting of either normal quark matter or color-flavor-locked phase. Combining deconfinement heating with magnetic field decay, we find that the thermal evolution curves are identical to pulsar data.
13 pages, 2 figures
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