Black Hole with Non-Commutative Hair

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dc.creatorKlimcik, C.
dc.creatorKolnik, P.
dc.creatorPompos, A.
dc.date1993-06-25
dc.date.accessioned2026-07-07T03:30:07Z
dc.date.available2026-07-07T03:30:07Z
dc.descriptionThe specific nonlinear vector $σ$-model coupled to Einstein gravity is investigated. The model arises in the studies of the gravitating matter in non-commutative geometry. The static spherically symmetric spacetimes are identified by direct solving of the field equations. The asymptotically flat black hole with the ``non-commutative'' vector hair appears for the special choice of the integration constants, giving thus another counterexample to the famous ``no-hair'' theorem.
dc.description10 pages, LaTeX, PRA-HEP-93/9
dc.identifierhttps://arxiv.org/abs/gr-qc/9306032
dc.identifierhttp://arxiv.org/abs/gr-qc/9306032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35430
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleBlack Hole with Non-Commutative Hair
dc.typetext

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