Physics – Nuclear Physics – Nuclear Theory
Scientific paper
1996-08-25
Phys.Rev.C54:2751-2759,1996
Physics
Nuclear Physics
Nuclear Theory
13 pages, 6 figures
Scientific paper
10.1103/PhysRevC.54.2751
We calculate the reaction cross-sections for the fusion of hydrogen and deuterium in strong magnetic fields as are believed to exist in the atmospheres of neutron stars. We find that in the presence of a strong magnetic field ($B \gsim 10^{12}$G), the reaction rates are many orders of magnitude higher than in the unmagnetized case. The fusion of both protons and deuterons are important over a neutron star's lifetime for ultrastrong magnetic fields ($B \sim 10^{16}$G). The enhancement may have dramatic effects on thermonuclear runaways and bursts on the surfaces of neutron stars.
Hernquist Lars
Heyl Jeremy S.
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