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Comments on Cosmological Singularities in String Theory

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arxiv hep-th/0212215 v2 pith:KBTWU6AW submitted 2002-12-18 hep-th

classification hep-th
keywords backreactiondivergencesnearsingularitysomestringcosmologicalexcitations
verification ladder T0 review T1 audit T2 compute T3 formal
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We compute string scattering amplitudes in an orbifold of Minkowski space by a boost, and show how certain divergences in the four point function are associated with graviton exchange near the singularity. These divergences reflect large tree-level backreaction of the gravitational field. Near the singularity, all excitations behave like massless fields on a 1+1 dimensional cylinder. For excitations that are chiral near the singularity, we show that divergences are avoided and that the backreaction is milder. We discuss the implications of this for some cosmological spacetimes. Finally, in order to gain some intuition about what happens when backreaction is taken into account, we study an open string rolling tachyon background as a toy model that shares some features with R^{1,1}/Z.

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  1. On Cosmological Singularities in String Theory

    hep-th 2026-01 unverdicted novelty 5.0 of 10

    Perturbations in string theory on a three-sphere spacetime cause big-bang/crunch singularities or unbounded expansion, which string theory may resolve.

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