Dirac quasinormal modes of a black hole with quintessence-like matter and a deficit solid angle

Details Dirac quasinormal modes of a black hole with quintessence-like matter and a deficit solid angle Dirac quasinormal modes of a black hole with quintessence-like matter and a deficit solid angle

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.325..119w&link_type=abstract

Astrophysics and Space Science, Volume 325, Issue 1, pp.119-125

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using the third-order WKB approximation, we evaluate the quasinormal frequencies of massless Dirac field perturbation around a black hole with quintessence-like matter and a deficit solid angle. We discuss carefully the properties of quasinormal frequencies with the change of quintessential state parameter w q , the deficit solid angle parameter ɛ, the energy density of quintessence-like matter ρ 0, and the total angular momentum number | k| and the overtone number n, respectively.

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