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Constraints on String Cosmology

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arxiv 1110.0545 v4 pith:KVKUQWYI submitted 2011-10-03 hep-th astro-ph.COgr-qc

Constraints on String Cosmology

classification hep-th astro-ph.COgr-qc
keywords possiblestringforbiddeninteractionssittersolutionsacceleratinganti-de
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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String theory contains sources like orientifold planes that support higher derivative interactions. These interactions make possible static flux compactifications which are forbidden in supergravity. They can also lead to violations of the strong energy condition (SEC) which is needed for an accelerating universe. We examine how large a violation is possible in the context of the heterotic string compactified to four dimensions. We find that de Sitter solutions are still not possible but that classically forbidden anti-de Sitter solutions are possible.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. de Sitter in String Theory vs. Gibbons & Hawking

    hep-th 2026-04 conditional novelty 5.0

    Perturbative string theory forbids de Sitter times closed manifold solutions under the assumption that the Euclidean sphere partition function receives a nonzero 1/G_N contribution.

  2. Dark energy from string theory: an introductory review

    hep-th 2026-03 unverdicted novelty 2.0

    String theory imposes constraints on dark energy but permits various construction attempts for de Sitter vacua and single-field exponential quintessence models despite obstructions.