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- W2130402500 abstract "The impact of various competing heating processes on the thermal evolution of neutron stars is investigated. We show that internal heating leads to significantly enhanced sur- face temperatures for pulsars of middle and old age. The heating due to thermal creep of pinned vortices and due to outward mo- tion of proton vortices in the interior of the star leads to a better agreement with the observed data in the case of enhanced cool- ing. The strong pinning models are ruled out by a comparison with the cooling data on the old pulsars. For millisecond pul- sars, the heating due to thermal creep of pinned vortices and chemical heating of the core have the largest impact on the sur- face temperatures. The angular dependence of the heating rates require two dimensional cooling simulations in general. Such a simulation is performed for a selected case in order to check the applicability of one-dimensional codes used in the past." @default.
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- W2130402500 date "1999-06-01" @default.
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- W2130402500 title "Impact of Internal Heating on the Thermal Evolution of Neutron Stars" @default.
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