On black hole temperature in Horndeski gravity

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autoren

  • K. Hajian
  • S. Liberati
  • M. M. Sheikh-Jabbari
  • M. H. Vahidinia

Externe Organisationen

  • Scuola Internazionale Superiore di Studi Avanzati
  • Istituto Nazionale di Fisica Nucleare (INFN)
  • Institute for Fundamental Physics of the Universe (IFPU)
  • Institute for Research in Fundamental Sciences (IPM)
  • Abdus Salam International Centre for Theoretical Physics
  • Institute for Advanced Studies in Basic Sciences, Zanjan
  • Middle East Technical University (METU)
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Details

OriginalspracheEnglisch
Aufsatznummer136002
FachzeitschriftPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Jahrgang812
Frühes Online-Datum11 Dez. 2020
PublikationsstatusVeröffentlicht - 10 Jan. 2021

Abstract

It has been observed that for black holes in certain family of Horndeski gravity theories Wald's entropy formula does not lead to the correct first law for black hole thermodynamics. For this family of Horndeski theories speeds of propagation of gravitons and photons are in general different and gravitons move on an effective metric different than the one seen by photons. We show that the temperature of the black hole should be modified from surface gravity over 2π to include effects of this effective metric. The modified temperature, with the entropy unambiguously computed by the solution phase space method, yields the correct first law. Our results have far reaching implications for the Hawking radiation and species problem, going beyond the Horndeski theories.

ASJC Scopus Sachgebiete

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On black hole temperature in Horndeski gravity. / Hajian, K.; Liberati, S.; Sheikh-Jabbari, M. M. et al.
in: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Jahrgang 812, 136002, 10.01.2021.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Hajian K, Liberati S, Sheikh-Jabbari MM, Vahidinia MH. On black hole temperature in Horndeski gravity. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 2021 Jan 10;812:136002. Epub 2020 Dez 11. doi: 10.48550/arXiv.2005.12985, 10.1016/j.physletb.2020.136002
Hajian, K. ; Liberati, S. ; Sheikh-Jabbari, M. M. et al. / On black hole temperature in Horndeski gravity. in: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 2021 ; Jahrgang 812.
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AU - Hajian, K.

AU - Liberati, S.

AU - Sheikh-Jabbari, M. M.

AU - Vahidinia, M. H.

N1 - Funding Information: We are grateful to Gary Gibbons, Harvey Reall and Bayram Tekin for comments. KH and MMShJ thank the hospitality of ICTP HECAP where this research carried out. MMShJ acknowledges the support by INSF junior research chair in black hole physics, grant No 950124 and Saramadan grant No. ISEF/M/98204. KH acknowledges support from TÜBITAK international researchers program 2221. SL acknowledges funding from the Ministry of Education and Scientific Research (MIUR) under the grant PRIN MIUR 2017-MB8AEZ.

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AB - It has been observed that for black holes in certain family of Horndeski gravity theories Wald's entropy formula does not lead to the correct first law for black hole thermodynamics. For this family of Horndeski theories speeds of propagation of gravitons and photons are in general different and gravitons move on an effective metric different than the one seen by photons. We show that the temperature of the black hole should be modified from surface gravity over 2π to include effects of this effective metric. The modified temperature, with the entropy unambiguously computed by the solution phase space method, yields the correct first law. Our results have far reaching implications for the Hawking radiation and species problem, going beyond the Horndeski theories.

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KW - Hawking radiation

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