2012
DOI: 10.1007/jhep04(2012)125
|View full text |Cite
|
Sign up to set email alerts
|

Near-extremal black holes

Abstract: We present a new formulation of deriving Hawking temperature for near-extremal black holes using distributions. In this paper the nearextremal Reissner-Nordström and Kerr black holes are discussed. It is shown that the extremal solution as a limit of non-extremal metric is well-defined. The pure extremal case is also discussed separately.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
9
0

Year Published

2012
2012
2021
2021

Publication Types

Select...
4
2

Relationship

4
2

Authors

Journals

citations
Cited by 6 publications
(9 citation statements)
references
References 34 publications
0
9
0
Order By: Relevance
“…As was mentioned earlier, this formalism was introduced in [37,38] and applied to the stationary and dynamical black hole horizons including extremal ones. The present work is the first attempt to find horizon temperature in a cosmological scenario using this formalism.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…As was mentioned earlier, this formalism was introduced in [37,38] and applied to the stationary and dynamical black hole horizons including extremal ones. The present work is the first attempt to find horizon temperature in a cosmological scenario using this formalism.…”
Section: Discussionmentioning
confidence: 99%
“…This method of calculating temperature associated with a trapping horizon was previously been introduced in [37,38] in the case of a black hole. It was motivated by the work of Damour and Ruffini [39] and is found to work for different types of horizons just as well as the tunneling method.…”
Section: Introductionmentioning
confidence: 99%
“…To determine the temperature of the outer horizon we shall adopt the formalism discussed in [21] for static spherically symmetric black holes. Considering a scalar field, we shall construct the modes of the Killing vector across the horizon.…”
Section: Horizon Temperaturementioning
confidence: 99%
“…The method we have employed to calculate temperature of the dynamical horizon has been used to calculate temperature for the stationary (both non-extremal and extremal) [21] as well as dynamical horizons [22,23]. For dynamical horizons in 4-dimensions the symmetry of the spacetime plays an important role.…”
Section: E Heat Capacitymentioning
confidence: 99%
See 1 more Smart Citation