2006
DOI: 10.1103/physrevd.73.126006
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Matrix membrane big bangs andD-brane production

Abstract: We construct Matrix Membrane theory in pp wave backgrounds that have a null linear dilaton in Type IIB string theory. Such backgrounds can serve as toy models of big bang cosmologies. At late times only abelian degrees of freedom survive, and if the Kaluza-Klein modes along one of the directions of the membrane decouple, standard perturbative strings emerge. Near the "big bang", non-abelian configurations of fuzzy ellipsoids are present, as in the Type IIA theories. A generic configuration of these shrink to z… Show more

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Cited by 32 publications
(33 citation statements)
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“…where we have used the gauge condition to set g uv = −1, i.e., 17) and f α (u) and g(u) are given by 18) respectively. If we compactify y α , we may find a time-dependent cosmological solution.…”
Section: Asymptotic Structurementioning
confidence: 99%
“…where we have used the gauge condition to set g uv = −1, i.e., 17) and f α (u) and g(u) are given by 18) respectively. If we compactify y α , we may find a time-dependent cosmological solution.…”
Section: Asymptotic Structurementioning
confidence: 99%
“…The size of the ellipsoids is now time dependent : with some initial size the equations of motion may be used to examine the size at later times. Numerical results [2] show that with generic initial conditions, the size oscillates with an amplitude decaying fast with time. In other words, at late times we are left with only the abelian configurations which can be now interpreted as fundamental strings.…”
Section: Pp-wave Big Bangsmentioning
confidence: 99%
“…The Type IIB version of this background shows a richer structure [2]. The background is once again given by (1) and (2) where both x − and x 8 are compact,…”
Section: Iib Big Bangsmentioning
confidence: 99%
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