Moving five-branes and membrane instantons in low energy heterotic M theory
Moving five-branes and membrane instantons in low energy heterotic M theory
We study cosmological solutions in the context of four-dimensional low energy heterotic M theory with moving bulk branes. First we present nontrivial, analytic axion solutions generated by new symmetries of the full potential-free action, and we discuss their relation to "triple axion" solutions found in Pre-Big-Bang cosmologies. Next we consider the presence of a nonperturbative superpotential with and without a background perfect fluid. In the absence of a fluid the dilaton and the T-modulus go to the potential-free solutions at late time, while the moving brane tries to avoid colliding with the boundary and stabilize within the bulk. When the fluid is included the dynamics of the fields change, and we study their behavior both numerically and analytically. In particular we examine the possibility of this setup being a realization of the quintessential scenario and the impact of the fluid on the cosmological stabilization of the moduli.
026004-[15pp.]
de Carlos, Beatriz
f2040a2d-52ce-4166-add7-60135ce21835
Roberts, Jonathan
f6dc4282-689f-49f2-8b1b-3c71cf74db6b
Schmöhe, Yaiza
b0d0ff8b-625d-4371-b7d6-3ae3ace7f861
11 January 2005
de Carlos, Beatriz
f2040a2d-52ce-4166-add7-60135ce21835
Roberts, Jonathan
f6dc4282-689f-49f2-8b1b-3c71cf74db6b
Schmöhe, Yaiza
b0d0ff8b-625d-4371-b7d6-3ae3ace7f861
de Carlos, Beatriz, Roberts, Jonathan and Schmöhe, Yaiza
(2005)
Moving five-branes and membrane instantons in low energy heterotic M theory.
Physical Review D, 71, .
(doi:10.1103/PhysRevD.71.026004).
Abstract
We study cosmological solutions in the context of four-dimensional low energy heterotic M theory with moving bulk branes. First we present nontrivial, analytic axion solutions generated by new symmetries of the full potential-free action, and we discuss their relation to "triple axion" solutions found in Pre-Big-Bang cosmologies. Next we consider the presence of a nonperturbative superpotential with and without a background perfect fluid. In the absence of a fluid the dilaton and the T-modulus go to the potential-free solutions at late time, while the moving brane tries to avoid colliding with the boundary and stabilize within the bulk. When the fluid is included the dynamics of the fields change, and we study their behavior both numerically and analytically. In particular we examine the possibility of this setup being a realization of the quintessential scenario and the impact of the fluid on the cosmological stabilization of the moduli.
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Published date: 11 January 2005
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Local EPrints ID: 64104
URI: http://eprints.soton.ac.uk/id/eprint/64104
ISSN: 1550-7998
PURE UUID: 6e40d54a-8ef5-4041-8b0b-9e96d773ef75
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Date deposited: 01 Dec 2008
Last modified: 15 Mar 2024 11:46
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Author:
Beatriz de Carlos
Author:
Jonathan Roberts
Author:
Yaiza Schmöhe
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