Pulsar magnetic moment decay due to radiation damping and the pulsar in SN 1987 A

Details Pulsar magnetic moment decay due to radiation damping and the pulsar in SN 1987 A Pulsar magnetic moment decay due to radiation damping and the pulsar in SN 1987 A

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ncimc..12..625i&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 12 C, Sept.-Oct. 1989, p. 625-637.

Astronomy and Astrophysics

Astronomy

2

Magnetic Moments, Pulsars, Stellar Magnetic Fields, Stellar Radiation, Supernova 1987A, Astronomical Models, Magnetic Dipoles, Radio Sources (Astronomy), Stellar Evolution

Scientific paper

A new theory is proposed to account for the decay of the pulsar magnetic moment in terms of radiation damping mechanism. Detailed comparisons with the up-to-date pulsar observations are made. The theory is then applied to binary radio pulsars thereby resolving the dilemma concerning the ages and the magnetic fields of the pulsars PSR 0655 + 64 and PSR 1855 + 09. Finally, a prediction is made concerning the period and period derivative of the pulsar in SN 1987 A.

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