Effect of Superstrong Magnetic Fields on Nuclear Energy Generation Rate in the Crust of Neutron Stars

Details Effect of Superstrong Magnetic Fields on Nuclear Energy Generation Rate in the Crust of Neutron Stars Effect of Superstrong Magnetic Fields on Nuclear Energy Generation Rate in the Crust of Neutron Stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cotph..49.1069l&link_type=abstract

Communications in Theoretical Physics, Volume 49, Issue 4, pp. 1069-1072 (2008).

Physics

2

Scientific paper

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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