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Multidimensional Cosmological and Spherically Symmetric Solutions with Intersecting p-Branes

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Mathematical and Quantum Aspects of Relativity and Cosmology

Part of the book series: Lecture Notes in Physics ((LNP,volume 537))

Abstract

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 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.

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  1. Center for Gravitation and Fundamental Metrology VNIIMS, 3-1 M. Ulyanovoy Str., 117313, Moscow, Russia

    V.D. Ivashchuk & V.N. Melnikov

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  1. V.D. Ivashchuk
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  1. Research Laboratory for Geometry, Dynamical System and Cosmology Department of Mathematics, University of the Aegean, 83 200, Karlovassi, Greece

    Spiros Cotsakis

  2. DAMTP, University of Cambridge, Silver Street, CB3 9EW, Cambridge, UK

    Gary W. Gibbons

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Ivashchuk, V., Melnikov, V. (2000). Multidimensional Cosmological and Spherically Symmetric Solutions with Intersecting p-Branes. In: Cotsakis, S., Gibbons, G.W. (eds) Mathematical and Quantum Aspects of Relativity and Cosmology. Lecture Notes in Physics, vol 537. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-46671-1_9

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