Pulsar magnetosphere resulting from torsional magneto-elastic pulsations of permanently magnetized neutron stars

Details Pulsar magnetosphere resulting from torsional magneto-elastic pulsations of permanently magnetized neutron stars Pulsar magnetosphere resulting from torsional magneto-elastic pulsations of permanently magnetized neutron stars

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002hpa..conf..206b&link_type=abstract

Proc. of International Workshop: Hot Points in Astrophysics (JINR, Dubna, Russia 22-26 August 2000), p. 206.

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Magnetosphere, Pulsations

Scientific paper

A newly born pulsar brougth to gravitational equilibrium in the state of permanent magnetization of neutron matter can undergo non-radial torsional pulsations resulting in periodic oscillating, with the same frequency, electric field that rip off charged particles in the surrounding space. The expected effect is long-periodic (30-50 second) modulation of radio emission caused by periodic changes in the beam direction due to fluctuations of magnetic field lines in the neutron star magnetosphere.

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