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https://doi.org/10.1088/0253-6102/49/4/55
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Cite Publication Date: Apr 10, 2008 | |
 Citations: 2 |
Affiliation: China West Normal University, Institute of Theoretical Physics
This paper shows that superstrong magnetic fields (such as those of magnetars) can increase the energy generation rate many times in the crust of neutron stars. This result undoubtedly not only influences the cooling of neutron stars and the X-ray luminosity observed of neutron stars but also the evolution of neutron stars.
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