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Accelerating Cosmologies and Inflation from M/Superstring Theories

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arxiv hep-th/0411230 v4 pith:34KVIKAO submitted 2004-11-25 hep-th astro-phhep-ph

classification hep-thastro-phhep-ph
keywords theoriesacceleratingcosmologiesinflationm-theorysuperstringdimensionsinflationary
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We review the recent developments in obtaining accelerating cosmologies and/or inflation from higher-dimensional gravitational theories, in particular superstring theories in ten dimensions and M-theory in eleven dimensions. We first discuss why it is difficult to obtain inflationary behavior in the effective low-energy theories of superstring/M-theory, i. e. supergravity theories. We then summarize interesting solutions including S-branes that give rise to accelerating cosmologies and inflationary solutions in M-theory with higher order corrections. Other approaches to inflation in the string context are also briefly discussed.

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  1. Universal Cosmologies

    hep-th 2025-05 conditional novelty 5.0 of 10

    For open FLRW universes in two-scalar exponential-potential models from 10d IIA supergravity, the late-time attractor sets the effective exponent to the shortest vector to the convex hull of potential exponents, givin...

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