{ "id": "1401.0544", "version": "v3", "published": "2014-01-02T21:04:00.000Z", "updated": "2014-12-19T19:30:53.000Z", "title": "Quasi-Normal Modes for Subtracted Rotating and Magnetised Geometries", "authors": [ "M. Cvetic", "G. W. Gibbons", "Z. H. Saleem" ], "comment": "28 pages minor corrections, added references", "categories": [ "hep-th", "gr-qc" ], "abstract": "We obtain explicit separable solutions of the wave equation of massless minimally coupled scalar fields in the subtracted geometry of four-dimensional rotating and Melvin (magnetised) four-charge black holes of the STU model, a consistent truncation of maximally supersymmetric supergravity with four types of electromagnetic fields. These backgrounds possess a hidden SL(2,R) x SL(2,R) x SO(3) symmetry and faithfully model the near horizon geometry of these black holes, but locate them in a confining asymptotically conical box. For each subtracted geometry we obtain two branches of quasi-normal modes, given in terms of hypergeometric functions and spherical harmonics. One branch is over-damped and the other under-damped and they exhibit rotational splitting. No black hole bomb is possible because the Killing field which co-rotates with the horizon is everywhere timelike outside the black hole. A five-dimensional lift of these geometries is given locally by the product of a BTZ black hole with a two-sphere. This allows an explicit analysis of the minimally coupled massive five-dimensional scalar field. Again, there are two branches, both damped, however now their oscillatory parts are shifted by the quantised wave number $k$ along the fifth circle direction.", "revisions": [ { "version": "v2", "updated": "2014-01-17T21:00:04.000Z", "abstract": "We obtain explicit separable solutions of the wave equation of massless minimally coupled scalar fields in the subtracted geometry of four-dimensional rotating and Melvin (magnetised) four-charge black holes of the STU model, a consistent truncation of maximally supersymmetric supergravity with four types of electromagnetic fields. These backgrounds possess a hidden SL(2,R) x SL(2,R) x SO(3) symmetry and faithfully model the near horizon geometry of these black holes, but locate them in a confining asymptotically conical box. For each subtracted geometry we obtain two branches of quasi-normal modes, given in terms of hypergeometric functions and spherical harmonics. One branch is over-damped and the other under-damped and they exhibit rotational splitting. No black hole bomb is possible because the Killing field which co-rotates with the horizon is everywhere timelike outside the black hole. A five-dimensional lift of these geometries is given locally by the product of a BTZ black hole with a a two-sphere. This allows an explicit analysis of the minimally coupled massive five-dimensional scalar field. Again, there are two branches, both damped, however now their oscillatory parts are shifted by the quantised wave number $k$ along the fifth circle direction. We also comment on the dual field theory interpretation of these results in the context of the AdS_3/CFT_2 correspondence, and note a possible phase transition in dual CFT_2 when the subtracted rotating geometry is extremal.", "journal": null, "doi": null }, { "version": "v3", "updated": "2014-12-19T19:30:53.000Z" } ], "analyses": { "subjects": [ "04.20.Jb" ], "keywords": [ "black hole", "quasi-normal modes", "massive five-dimensional scalar field", "subtracted rotating", "magnetised geometries" ], "tags": [ "journal article" ], "publication": { "doi": "10.1103/PhysRevD.90.124046", "journal": "Physical Review D", "year": 2014, "month": "Dec", "volume": 90, "number": 12, "pages": 124046 }, "note": { "typesetting": "TeX", "pages": 28, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1275958, "adsabs": "2014PhRvD..90l4046C" } } }