The relativistic time delay of pulsar radiation in the gravitational field of the globular cluster stars

Details The relativistic time delay of pulsar radiation in the gravitational field of the globular cluster stars The relativistic time delay of pulsar radiation in the gravitational field of the globular cluster stars

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...6e..13l&link_type=abstract

Neutron Stars and Black Holes in Star Clusters, 26th meeting of the IAU, Joint Discussion 6, 17-18 August 2006, Prague, Czech Re

Physics

Scientific paper

The relativistic time delay of the pulsar signal in the curved space time of randomly distributed and moving globular cluster stars is discussed. Taking into account the aberration corrections that arise from the nonstationarity of the gravitational field of ensemble of stars, the expression of this delay is derived. This formula is used to calculate the statistical parameters of the pulsar noise caused by the random passages of stars near the line of sight to the pulsar. The obtained results are considered in the application to the globular clusters which contain the ceiling amount of observed pulsars.

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