A Possible Explanation of the Origin of the Second Kind of Magnetic Fields of Neutron Stars

Details A Possible Explanation of the Origin of the Second Kind of Magnetic Fields of Neutron Stars A Possible Explanation of the Origin of the Second Kind of Magnetic Fields of Neutron Stars

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...275..192l&link_type=abstract

Astronomy and Astrophysics, Vol.275, NO. 1/AUG(I), P. 192, 1993

Astronomy and Astrophysics

Astrophysics

Neutron Star, Magnetic Field, Dense Matter

Scientific paper

A possible explanation of the origin of the second kind of magnetic
fields (not decaying, with strength 109-1010 G) of
neutron stars is proposed which is related to the quark cluster phase of
superdense matter in the core of the neutron star.

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