Nucleosynthesis in strong magnetic fields at statistical equilibrium

Details Nucleosynthesis in strong magnetic fields at statistical equilibrium Nucleosynthesis in strong magnetic fields at statistical equilibrium

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mnras.359..927k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 359, Issue 3, pp. 927-929.

Astronomy and Astrophysics

Astronomy

2

Magnetic Fields, Nuclear Reactions, Nucleosynthesis, Abundances, Supernovae: General

Scientific paper

The atomic mass distribution of nuclides in an ultramagnetized
astrophysical plasma is considered by employing a model of nuclear
statistical equilibrium. The magnetization of atomic nuclei is shown to
enhance the portion of light nuclear species in the iron region.

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