Hawking Radiation of Black p-Branes from Gravitational Anomaly
| dc.creator | Ma, Zheng Ze | |
| dc.date | 2007-09-24 | |
| dc.date | 2008-08-01 | |
| dc.date.accessioned | 2026-07-07T11:53:13Z | |
| dc.date.available | 2026-07-07T11:53:13Z | |
| dc.description | We investigate the Hawking radiation of black $p$-branes of superstring theories using the method of anomaly cancelation, specially, we use the method of [S. Iso, H. Umetsu and F. Wilczek, {\sl Phys. Rev. Lett.} {\bf 96}, 151302 (2006); {\sl Phys. Rev. D} {\bf 74}, 044017 (2006)]. The metrics of black $p$-branes are spherically symmetric, but not the Schwarzschild type. In order to simplify the calculation, we first make a coordinate transformation to transform the metric to the Schwarzschild type. Then we calculate its energy-momentum flux from the method of anomaly cancelation of the above mentioned references. The obtained energy-momentum flux is equal to a black body radiation, the thermodynamic temperature of the radiation is equal to its Hawking temperature. And we find that the results are not changed for the original non-Schwarzschild type spherically symmetric metric. | |
| dc.description | 19 pages Latex, some mistakes corrected | |
| dc.identifier | https://arxiv.org/abs/0709.3684 | |
| dc.identifier | http://arxiv.org/abs/0709.3684 | |
| dc.identifier | Int.J.Mod.Phys.A23:2783-2800,2008 | |
| dc.identifier | doi:10.1142/S0217751X08039918 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/204462 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Hawking Radiation of Black p-Branes from Gravitational Anomaly | |
| dc.type | text |