The relativistic rotation transformation and the corotating source model

Details The relativistic rotation transformation and the corotating source model The relativistic rotation transformation and the corotating source model

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...371..277k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 371, April 10, 1991, p. 277-279.

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Astronomical Models, Pulsars, Relativistic Effects, Stellar Rotation, Computational Astrophysics, Pulsar Magnetospheres, Stellar Radiation, Stellar Spectra

Scientific paper

The characteristic parameters of pulsars are derived within the framework of the corotating source model, using the relativistic rotation transformation which respects the relativity of simultaneity at a distance, instead of the usual Galilean one which assumes t-prime = t. The resulting nonlinear relation between speed and angular rotation velocity avoids the use of the 'light cylinder' and the difficulties pertaining to it.

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