Time-Dependent Supersymmetric Solutions in M-Theory and the Compactification-Decompactification Transition

Simple item page
dc.creatorKodama, Hideo
dc.creatorOhta, Nobuyoshi
dc.date2006-05-18
dc.date2006-07-29
dc.date.accessioned2026-07-07T10:42:20Z
dc.date.available2026-07-07T10:42:20Z
dc.descriptionWe show that the diagonal light-like solution with 16 supersymmetries in eleven-dimensional supergravity derived in our previous paper (hep-th/0509173) can be generalised to non-diagonal solutions preserving the same number of supersymmetries. This class of solutions contains a subclass equivalent to the class of solutions found by Bin Chen that are dependent on the spatial-coordinates. Utilising these solutions, we construct toroidally compactified solutions that smoothly connect a static compactified region with a dynamically decompactifying region along a null hypersurface.
dc.description28 pages, 3 figures; the published version
dc.identifierhttps://arxiv.org/abs/hep-th/0605179
dc.identifierhttp://arxiv.org/abs/hep-th/0605179
dc.identifierProg.Theor.Phys.116:295-318,2006
dc.identifierdoi:10.1143/PTP.116.295
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181911
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTime-Dependent Supersymmetric Solutions in M-Theory and the Compactification-Decompactification Transition
dc.typetext

Files

Collections

arXiv