On inner structure of cold superdense stars with a frozen-in magnetic field

Details On inner structure of cold superdense stars with a frozen-in magnetic field On inner structure of cold superdense stars with a frozen-in magnetic field

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52.1166s&link_type=abstract

Astronomicheskii Zhurnal, vol. 52, Nov.-Dec. 1975, p. 1166-1172. In Russian.

Astronomy and Astrophysics

Astronomy

7

Magnetic Stars, Pulsars, Stellar Magnetic Fields, Stellar Structure, Electron Density (Concentration), Pair Production, Proton Density (Concentration), Thermodynamic Equilibrium, Trapped Magnetic Fields

Scientific paper

It is shown that the concentration of protons (electrons) at the
densities near the nuclear density depends on magnetic field, the
strength of which has a value of at least ten to the eighteenth gs. The
limits of the applicability of anomalous magnetic moment of electron are
discussed.

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