Hawking radiation via Gauss–Bonnet theorem

A. Övgün; Sakallı

doi:10.1016/j.aop.2020.168071

Hawking radiation via Gauss–Bonnet theorem

A. Övgün, Sakallı

INSTITUTE OF PHYSICS

Research output: Contribution to journal › Article › peer-review

18 Scopus citations

Abstract

In this paper, we apply the topological method to the various black holes to derive their Hawking temperature. We show that the this method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology. Therefore, we conclude that the topological method provides a consistent formula to achieve the Hawking temperature.

Original language	English
Article number	168071
Journal	Annals of Physics
Volume	413
DOIs	https://doi.org/10.1016/j.aop.2020.168071
State	Published - Feb 2020

Keywords

Black hole
Euler characteristic
Gauss–Bonnet theorem
Hawking radiation
Temperature
Thermodynamics

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10.1016/j.aop.2020.168071

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title = "Hawking radiation via Gauss–Bonnet theorem",

abstract = "In this paper, we apply the topological method to the various black holes to derive their Hawking temperature. We show that the this method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology. Therefore, we conclude that the topological method provides a consistent formula to achieve the Hawking temperature.",

keywords = "Black hole, Euler characteristic, Gauss–Bonnet theorem, Hawking radiation, Temperature, Thermodynamics",

author = "A. {\"O}vg{\"u}n and Sakallı",

year = "2020",

month = feb,

doi = "10.1016/j.aop.2020.168071",

language = "English",

volume = "413",

journal = "Annals of Physics",

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T1 - Hawking radiation via Gauss–Bonnet theorem

AU - Övgün, A.

AU - Sakallı,

PY - 2020/2

Y1 - 2020/2

N2 - In this paper, we apply the topological method to the various black holes to derive their Hawking temperature. We show that the this method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology. Therefore, we conclude that the topological method provides a consistent formula to achieve the Hawking temperature.

AB - In this paper, we apply the topological method to the various black holes to derive their Hawking temperature. We show that the this method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology. Therefore, we conclude that the topological method provides a consistent formula to achieve the Hawking temperature.

KW - Black hole

KW - Euler characteristic

KW - Gauss–Bonnet theorem

KW - Hawking radiation

KW - Temperature

KW - Thermodynamics

UR - http://www.scopus.com/inward/record.url?scp=85077653649&partnerID=8YFLogxK

U2 - 10.1016/j.aop.2020.168071

DO - 10.1016/j.aop.2020.168071

M3 - Article

AN - SCOPUS:85077653649

SN - 0003-4916

VL - 413

JO - Annals of Physics

JF - Annals of Physics

M1 - 168071

ER -

Hawking radiation via Gauss–Bonnet theorem

Abstract

Keywords

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