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This paper shows that superstrong magnetic fields (such as those of magnetars) can increase the energygeneration rate many times in the crust of neutron stars.This result undoubtedly not only influences the cooling ofneutron stars and the X-ray luminosity observed of neutron stars but also the evolution of neutron stars.
This paper shows that superstrong magnetic fields (such as those of magnetars) can increase the energygeneration rate many many in the crust of neutron stars. This result undoubtedly not only influences the cooling ofneutron stars and the X-ray luminosity observed of neutron stars but also the evolution of neutron stars.