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O$(d,d)$ covariant String Cosmology to all orders in $\alpha^{\prime}$

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arxiv 1911.00088 v2 pith:DDJ7GJQG submitted 2019-10-31 hep-th astro-ph.COgr-qchep-ph

classification hep-thastro-ph.COgr-qchep-ph
keywords equationsmatteralphastringcorrectionscosmologycovariantorders
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abstract

Recently, all duality invariant $\alpha'$-corrections to the massless NS-NS sector of string theory on time-dependent backgrounds were classified and the form of their contribution to the action were calculated. In this paper we introduce matter sources in the resulting equations of motion in an O$(d,d)$ covariant way. We show that either starting with the corrected equations and sourcing them with matter or considering corrections to the matter sourced lowest order equations give the same set of equations that defines string cosmology to all orders in $\alpha'$. We also discuss perturbative and non-perturbative de Sitter solutions including matter.

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Cited by 1 Pith paper

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  1. Higher co-dimension de Sitter branes

    hep-th 2025-06 conditional novelty 6.0 of 10

    A no-go theorem shows that thin co-dimension-two branes cannot support de Sitter vacua in compactified supergravity, and higher co-dimensions need negative tension.

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