Non-trivial, static, geodesically complete space-times with a negative cosmological constant II. $n\ge 5$

Simple item page
dc.creatorAnderson, M.
dc.creatorChrusciel, P. T.
dc.creatorDelay, E.
dc.date2004-01-19
dc.date2005-01-25
dc.date.accessioned2026-07-07T03:28:25Z
dc.date.available2026-07-07T03:28:25Z
dc.descriptionWe show that the recent work of Lee [23] implies existence of a large class of new singularity-free strictly static Lorentzian vacuum solutions of the Einstein equations with a negative cosmological constant. This holds in all space-time dimensions greater than or equal to four, and leads both to strictly static solutions and to black hole solutions. The construction allows in principle for metrics (whether black hole or not) with Yang-Mills-dilaton fields interacting with gravity through a Kaluza-Klein coupling.
dc.descriptionProceedings of the Strasbourg Meeting on AdS-CFT correspondence, O.Biquard, V.Turaev, Eds., IRMA Lectures in Mathematics and Theoretical Physics, de Gruyter, Berlin, New York, in press; latex2e, 39 pages in A4; minor corrections
dc.identifierhttps://arxiv.org/abs/gr-qc/0401081
dc.identifierhttp://arxiv.org/abs/gr-qc/0401081
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34824
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.subjectDifferential Geometry
dc.titleNon-trivial, static, geodesically complete space-times with a negative cosmological constant II. $n\ge 5$
dc.typetext

Files

Collections

arXiv