{ "id": "1007.5002", "version": "v2", "published": "2010-07-28T15:04:56.000Z", "updated": "2010-10-26T04:06:20.000Z", "title": "Stability of Holographic Superconductors", "authors": [ "Sugumi Kanno", "Jiro Soda" ], "comment": "11 pages, published version", "journal": "Phys.Rev.D82:086003,2010", "doi": "10.1103/PhysRevD.82.086003", "categories": [ "hep-th", "gr-qc", "hep-ph" ], "abstract": "We study the dynamical stability of holographic superconductors. We first classify perturbations around black hole background solutions into vector and scalar sectors by means of a 2-dimensional rotational symmetry. We prove the stability of the vector sector by explicitly constructing the positive definite Hamiltonian. To reveal a mechanism for the stabilization of a superconducting phase, we construct a quadratic action for the scalar sector. From the action, we see the stability of black holes near a critical point is determined by the equation of motion for a charged scalar field. We show the effective mass of the charged scalar field in hairy black holes is always above the Breitenlohner-Freedman bound near the critical point due to the backreaction of a gauge field. It implies the stability of the superconducting phase. We also argue that the stability continues away from the critical point.", "revisions": [ { "version": "v2", "updated": "2010-10-26T04:06:20.000Z" } ], "analyses": { "subjects": [ "11.25.Tq", "04.70.Bw", "74.20.-z" ], "keywords": [ "holographic superconductors", "critical point", "charged scalar field", "scalar sector", "black hole background solutions" ], "tags": [ "journal article" ], "publication": { "publisher": "APS", "journal": "Physical Review D", "year": 2010, "month": "Oct", "volume": 82, "number": 8, "pages": "086003" }, "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable", "inspire": 863314, "adsabs": "2010PhRvD..82h6003K" } } }