On a possible mechanism of variation of pulsar periods

Details On a possible mechanism of variation of pulsar periods On a possible mechanism of variation of pulsar periods

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982afz....18..101p&link_type=abstract

(Astrofizika, vol. 18, Jan.-Mar. 1982, p. 101-106.) Astrophysics, vol. 18, no. 1, July 1982, p. 62-64. Translation.

Astronomy and Astrophysics

Astrophysics

Pulsars, Stellar Magnetic Fields, Stellar Oscillations, Electron Gas, Magnetohydrodynamic Stability, Neutron Stars, Relativistic Plasmas, Variability

Scientific paper

A mechanism is developed to explain the abrupt changes in the period of pulsars. It is found that instabilities in the magnetization of the electron component of neutron stars may be a result of oscillations in the magnetic susceptibility of a relativistic electron gas due to quantization in a magnetic field. It is shown that these instabilities must lead to abrupt changes in the pulsar period as the magnetic field changes or the star cools.

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