Neutronization of strongly magnetized matter

Details Neutronization of strongly magnetized matter Neutronization of strongly magnetized matter

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..531i&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 70, no. 3, p. 531-536.

Astronomy and Astrophysics

Astronomy

1

Degenerate Matter, Fermions, Magnetic Effects, Magnetic Flux, Neutron Distribution, White Dwarf Stars, Gas Ionization, Pulsars, Stellar Magnetic Fields

Scientific paper

In the approximation of extremely degenerate ideal Fermi gases, it is shown that superstrong magnetic fields raise the threshold of the neutronization of dense hydrogen. For fixed values of density exceeding this threshold, the neutron concentration significantly decreases with the growth of the superstrong magnetic field induction. The neutronization threshold of heavy nuclei in strongly magnetized matter is estimated within the framework of the nuclear Fermi-gas model.

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