The Hawking temperature of expanding cosmological black holes
| dc.creator | Faraoni, Valerio | |
| dc.date | 2007-10-10 | |
| dc.date | 2007-11-13 | |
| dc.date.accessioned | 2026-07-07T11:37:59Z | |
| dc.date.available | 2026-07-07T11:37:59Z | |
| dc.description | In the context of a debate on the correct expression of the Hawking temperature of an expanding cosmological black hole, we show that the correct expression in terms of the Hawking-Hayward quasi-local energy m of the hole is T=1/(8πm(t)). This expression holds for comoving black holes and agrees with a recent proposal by Saida, Harada, and Maeda. | |
| dc.description | 5 latex pages, to appear in Phys. Rev. D. Some references added | |
| dc.identifier | https://arxiv.org/abs/0710.2122 | |
| dc.identifier | http://arxiv.org/abs/0710.2122 | |
| dc.identifier | Phys.Rev.D76:104042,2007 | |
| dc.identifier | doi:10.1103/PhysRevD.76.104042 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/199403 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | The Hawking temperature of expanding cosmological black holes | |
| dc.type | text |