A Model for Simulating Realistic Profiles of Pulsars

Details A Model for Simulating Realistic Profiles of Pulsars A Model for Simulating Realistic Profiles of Pulsars

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1357..297t&link_type=abstract

RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP Conference Proceedings, Volume 1357, pp. 297-298

Astronomy and Astrophysics

Astrophysics

Stellar Rotation, Gamma-Rays, Simulation, Angular Measurement, Stellar Rotation, Gamma-Ray, Numerical Simulation, Solution Of Equations, Spatial Dimensions

Scientific paper

We devise an accurate method to compute the emission profile
corresponding to a given set of pulsar emission parameters, for eg.
inclination angle α, impact angle β, frequency of emission
ω, Lorentz factor γ, and pulsar spin-period P. The intensity
of emission is simulated, and compared with the observed profiles.

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