Equatorial circular motion in Kerr spacetime

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

48 pages, 40 figures, 3 Tables. To be published PRD. This work follows the paper Phys. Rev. D Vol.83, No.2 with DOI: 10.1103

Scientific paper

10.1103/PhysRevD.84.044030

We analyze the properties of circular orbits of test particles on the equatorial plane of a rotating central mass whose gravitational field is described by the Kerr spacetime. For rotating black holes and naked singularities we explore all the spatial regions where circular orbits can exist and analyze the behavior of the energy and the angular momentum of the corresponding test particles. In particular, we find all the radii at which a test particle can have zero angular momentum due to the repulsive gravity effects generated by naked singularities. We classify all the stability zones of circular orbits. It is shown that the geometric structure of the stability zones of black holes is completely different from that of naked singularities.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Equatorial circular motion in Kerr spacetime does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Equatorial circular motion in Kerr spacetime, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Equatorial circular motion in Kerr spacetime will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-241567

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.