Multidimensional cosmological and spherically symmetric solutions with intersecting p-branes

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dc.creatorIvashchuk, V. D.
dc.creatorMelnikov, V. N.
dc.date1999-01-02
dc.date2002-02-25
dc.date.accessioned2026-07-07T03:32:52Z
dc.date.available2026-07-07T03:32:52Z
dc.descriptionMultidimensional model describing the "cosmological" and/or spherically symmetric configuration with n+1 Einstein spaces in the theory with several scalar fields and forms is considered. When electro-magnetic composite p-brane ansatz is adopted, n "internal" spaces are Ricci-flat, one space M_0 has a non-zero curvature, and all p-branes do not "live" in M_0, a class of exact solutions is obtained if certain block-orthogonality relations on p-brane vectors are imposed. A subclass of spherically-symmetric solutions containing non-extremal p-brane black holes is considered. Post-Newtonian parameters are calculated and some examples are considered.
dc.description33 pages, Latex., several typos and paragraphs are eliminated Publ.: Proc. of 2nd Samos meeting (1999), Lect. Notes in Phys., Vol. 537, Springer, 2000
dc.identifierhttps://arxiv.org/abs/gr-qc/9901001
dc.identifierhttp://arxiv.org/abs/gr-qc/9901001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36401
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleMultidimensional cosmological and spherically symmetric solutions with intersecting p-branes
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