Multidimensional cosmological and spherically symmetric solutions with intersecting p-branes
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Multidimensional 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.
33 pages, Latex., several typos and paragraphs are eliminated Publ.: Proc. of 2nd Samos meeting (1999), Lect. Notes in Phys., Vol. 537, Springer, 2000
33 pages, Latex., several typos and paragraphs are eliminated Publ.: Proc. of 2nd Samos meeting (1999), Lect. Notes in Phys., Vol. 537, Springer, 2000