Black hole spacetimes and pulsar timing

Details Black hole spacetimes and pulsar timing Black hole spacetimes and pulsar timing

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..aprx12002p&link_type=abstract

American Physical Society, 2009 APS April Meeting, May 2-5, 2009, abstract #X12.002

Physics

Scientific paper

A pulsar in a relativistic orbit around a supermassive black hole will exhibit potentially observable strong field effects in the times of arrival of its pulses. We present a simple formalism for computing these effects. This formalism is applied to illustrate the several types of strong field effects, to give explicit examples for the simple case of equatorial pulse beaming and to present a more general discussion for nonequatorial beaming.

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