Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13..217d&link_type=abstract
Astronomical Society of India, Bulletin, vol. 13, Sept. 1985, p. 217-224.
Astronomy and Astrophysics
Astronomy
Pulsars, Space-Time Functions, Stellar Radiation, Stellar Rotation, Electromagnetic Pulses, Time Lag
Scientific paper
Propagation of photons in the space-time exterior of a rapidly rotating neutron star is investigated, using a rotationally perturbed spherical metric, to determine the pulse profile of fast pulsars. It is found that space-time curvature produces a substantial amount of divergence in the pulse beam width accompanied by a reduction in the pulse intensity. Effects due to rotation are comparatively smaller, but rotation has the qualitatively important feature of producing a tilt of the pulse cone in the direction of rotation and a deformation of the cone. The asymmetry in the resultant pulse profile introduces a time delay in the arrival of photons emitted within the cone, which in turn affects the duty cycle of the pulsar.
Datta Bhaskar
Kapoor Ramesh Chander
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