Quantum Radiation from a 5-Dimensional Rotating Black Hole
By Valeri P. Frolov, D. Stojkovic. 2002
154 citations recorded by the source corpus.
We study a massless scalar field propagating in the background of a five-dimensional rotating black hole. We show that in the Myers-Perry metric describing such a black hole the massless field equation allows the separation of variables. The obtained angular equation is a generalization of the equation for spheroidal functions. The radial equation is similar to the radial Teukolsky equation for the 4-dimensional Kerr metric. We use these results to quantize the massless scalar field in the space-time of the 5-dimensional rotating black hole and to derive expressions for energy and angular momentum fluxes from such a black hole.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/0bcc432337cdc1c031fe1f348b9ee7e11b95034f
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- Paolo Pani
- V. Cardoso
- R. Brito
- Harvey Reall
- Roberto Emparan
- James Lucietti
- Jorge E Santos
- Hari K. Kunduri
In Nuclear and High Energy Physics
- R. Brito
- Paolo Pani
- V. Cardoso
- Harvey Reall
- Roberto Emparan
- James Lucietti
- Hari K. Kunduri
- Jorge E Santos
Citations in the corpus
- Rotating black holes at future colliders: Greybody factors for brane fields (2002, background): “[ 55 ] for the study of bulk scalar emission of five dimensional black hole.”
- Superradiance (2015, methodology): “[296]; using the area theorem this condition was generalized to arbitrary dimensions for Myers-Perry BHs with a single angular momentum parameter [297] and finally with multiple angular momentum parameters in Ref.”
- Black Holes in Higher Dimensions (2008, background): “It turns out that the general Myers–Perry solution also possesses hidden symmetries [174, 91] (this was first realized for the special case of d = 5 [93, 94]).”
- GRAVITATIONAL PERTURBATIONS OF HIGHER DIMENSIONAL ROTATING BLACK HOLES (2006, background): “It is known that this separability property of the Kerr metric does extend to some of the higher-dimensional MP metrics [17, 18, 19], and MP metrics with a cosmological constant [20].”