Cosmological and spherically symmetric solutions with intersecting p-branes

Details Cosmological and spherically symmetric solutions with intersecting p-branes Cosmological and spherically symmetric solutions with intersecting p-branes

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jmp....40.6558i&link_type=abstract

Journal of Mathematical Physics, Volume 40, Issue 12, pp. 6558-6576 (1999).

Physics

10

Strings And Branes, Particle-Theory And Field-Theory Models Of The Early Universe, Physics Of Black Holes, Exact Solutions, Einstein-Maxwell Spacetimes, Spacetimes With Fluids, Radiation Or Classical Fields

Scientific paper

Multidimensional model describing the cosmological evolution 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 M0 has a nonzero curvature, and all p-branes do not ``live'' in M0, 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 nonextremal p-brane black holes) is considered. Post-Newtonian parameters are calculated.

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