摘要
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.
基金
The project supported by National Natural Science Foundation of China under Grant Nos.10347008 and 10778719
the Scientific Research Fund of the Education Department of Sichuan Province under Grant No.2006A079
the Science and Technological Foundation of China West Normal University
