Dirac quasinormal modes of the deformed Hořava-Lifshitz black hole spacetime

Details Dirac quasinormal modes of the deformed Hořava-Lifshitz black hole spacetime Dirac quasinormal modes of the deformed Hořava-Lifshitz black hole spacetime

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.325...85w&link_type=abstract

Astrophysics and Space Science, Volume 325, Issue 1, pp.85-91

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

Using the third-order WKB approximation, we evaluate the quasinormal frequencies of massless Dirac field perturbation around a deformed black hole in the Hořava-Lifshitz gravity with coupling constant λ=1. Our result shows that the Hořava-Lifshitz parameter α plays an important role for the quasinormal frequencies and we discuss the variation of quasinormal frequencies with α. Moreover, we find that the massless Dirac field perturbations decay more slowly in the deformed Hořava-Lifshitz gravity.

Affiliated with

Also associated with

No associations

Rating

Dirac quasinormal modes of the deformed Hořava-Lifshitz black hole 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 Dirac quasinormal modes of the deformed Hořava-Lifshitz black hole spacetime, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dirac quasinormal modes of the deformed Hořava-Lifshitz black hole spacetime will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1888901