Release of Energy from Test Particles Falling onto a Rotating Neutron Star

Details Release of Energy from Test Particles Falling onto a Rotating Neutron Star Release of Energy from Test Particles Falling onto a Rotating Neutron Star

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet..945s&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

The energy of test particles orbiting the marginally stable orbits around a rotating neutron star (in the equatorial plane) is calculated. Assuming that all the energy is radiated when the particles fall and hit the surface of a neutron star, the energy release is estimated by using a new exact solution of Einstein-Maxwell equations with arbitrary deformation parameter. The calculations show that the amount of energy emitted depends on this parameter. The same calculations are made for the Kerr solution as reference.

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