{ "id": "0709.3684", "version": "v2", "published": "2007-09-24T04:37:40.000Z", "updated": "2008-08-01T15:07:36.000Z", "title": "Hawking Radiation of Black p-Branes from Gravitational Anomaly", "authors": [ "Zheng Ze Ma" ], "comment": "19 pages Latex, some mistakes corrected", "journal": "Int.J.Mod.Phys.A23:2783-2800,2008", "doi": "10.1142/S0217751X08039918", "categories": [ "hep-th" ], "abstract": "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.", "revisions": [ { "version": "v2", "updated": "2008-08-01T15:07:36.000Z" } ], "analyses": { "subjects": [ "11.30.-j", "04.70.Dy", "04.50.+h", "04.62.+v" ], "keywords": [ "hawking radiation", "black p-branes", "gravitational anomaly", "original non-schwarzschild type spherically symmetric", "energy-momentum flux" ], "tags": [ "journal article" ], "publication": { "journal": "International Journal of Modern Physics A", "year": 2008, "volume": 23, "number": 18, "pages": 2783 }, "note": { "typesetting": "LaTeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable", "inspire": 761647, "adsabs": "2008IJMPA..23.2783M" } } }