Angular momentum distribution in Kerr-Newman spacetime

Details Angular momentum distribution in Kerr-Newman spacetime Angular momentum distribution in Kerr-Newman spacetime

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvd..42.1066v&link_type=abstract

Physical Review D (Particles and Fields), Volume 42, Issue 4, 15 August 1990, pp.1066-1067

Physics

78

Scientific paper

The components of the momentum density in Kerr-Newman spacetime are evaluated using the energy-momentum pseudotensor of Landau and Lifshitz and then are used to find the angular momentum distribution in spacetime. Switching off the charge parameter (i.e., Q=0), one finds that no angular momentum is associated with the exterior of the Kerr black hole.

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