Neutron star magnetism

Details Neutron star magnetism Neutron star magnetism

Jun 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972zphy..250..254h&link_type=abstract

Zeitschrift für Physik, Volume 250, Issue 3, pp.254-262

Physics

6

Scientific paper

It is shown that
1.
an appreciable change of magnetic moment of a neutron star cannot occur via ohmic dissipation
2.
pulsars provide evidence for large internal magnetic fields in main sequence stars. If pulsars are born from stars with masses exceeding 3 ℳ&sun; the internal field must be of the order of 103-104 Gauss while if they derived from less massive urstars 102 Gauss are sufficient to give rise to a magnetic moment of M˜1030 Gauss cm3.

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