Neutron star evolution with internal heating
Neutron star evolution with internal heating
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DOI：
10.1086/168062
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发表时间：
1989-11
期刊：
影响因子：
--
通讯作者：
N. Shibazaki;F. Lamb
中科院分区：
文献类型：
--
作者：
N. Shibazaki;F. Lamb
目前的模型预测的超流地壳相互作用的热演化的注意到显着不同的热演化模型预测没有内部加热以及以前的加热模型。加热速率接近目前模型预测的最大值，在中微子冷却时代增强了星星的光子光度，并显着改变光子冷却时代的热演化。标准的冷却模型与目前的脉冲星温度估计和上限是一致的，除了船帆座脉冲星的温度低于预测。参考文献77篇。
The thermal evolution predicted by current models of the superfluid-crust interaction is noted to differ substantially from the thermal evolution predicted by models without internal heating as well as previous models of heating. Heating rates approaching the maximum predicted by current models enhance the photon luminosity of the star in the neutrino cooling era, and dramatically alter the thermal evolution in the photon cooling era. Standard cooling models are consistent with current pulsar temperature estimates and upper limits, except those for the Vela pulsar, which are lower than predicted. 77 refs.