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Related papers: Towards a Stringy Resolution of the Cosmological S…

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We study the effect of higher-curvature terms in the string low-energy effective actions on the cosmological solutions of the theory, up to corrections quartic in the curvatures, for the bosonic and heterotic strings as well as the type II…

General Relativity and Quantum Cosmology · Physics 2009-10-16 M. C. Bento , O. Bertolami

The possibility of obtaining singularity free cosmological solutions in four dimensional effective actions motivated by string theory is investigated. In these effective actions, in addition to the Einstein-Hilbert term, the dilatonic and…

High Energy Physics - Theory · Physics 2009-11-07 J. C. Fabris , R. G. Furtado , Patrick Peter , N. Pinto-Neto

We investigate quantum corrections for a cosmological solution of the string effective action. Starting point is a classical solution containing an antisymmetric tensor field, a dilaton and a modulus field which has singularities in the…

High Energy Physics - Theory · Physics 2007-05-23 K. Behrndt

We obtain cosmological four dimensional solutions of the low energy effective string theory by reducing a five dimensional black hole, and black hole--de Sitter solution of the Einstein gravity down to four dimensions. The appearance of a…

High Energy Physics - Theory · Physics 2008-02-03 K. Behrndt , S. Foerste

FRW solutions of the string theory low-energy effective actions are described, yielding a dilaton which first decreases and then increases. We study string creation in these backgrounds and find an exponential divergence due to an initial…

High Energy Physics - Theory · Physics 2010-04-05 Joshua J. Friess , Steven S. Gubser , Indrajit Mitra

An important element in a model of non-singular string cosmology is a phase in which classical corrections saturate the growth of curvature in a deSitter-like phase with a linearly growing dilaton (an `algebraic fixed point'). As the form…

High Energy Physics - Theory · Physics 2009-10-31 Ram Brustein , Richard Madden

In this work cosmological models are considered for the low energy string cosmological effective action (tree level) in the absence of dilaton potential. A two parametric non-diagonal family of analytic solutions is found. The curvature is…

General Relativity and Quantum Cosmology · Physics 2016-08-31 Luis O. Pimentel

We obtain cosmological four dimensional solutions of the low energy effective string theory by reducing a five dimensional black hole, and black hole--de Sitter solution of Einstein gravity down to four dimensions. The appearance of a…

High Energy Physics - Theory · Physics 2009-10-22 K. Behrndt , S. Foerste

We discuss time - dependent solutions of the leading order string effective equations for a non-zero central charge deficit and curved maximally symmetric space. Some regular solutions are found for the case of non-trivial antisymmetric…

High Energy Physics - Theory · Physics 2009-09-17 A. A. Tseytlin

Singularity-free cosmological solutions may be obtained from the string action at tree level if the dimension of the space-time is greater than 10 and if brane configurations are taken into account. The behaviour of the dilaton field in…

General Relativity and Quantum Cosmology · Physics 2007-05-23 J. C. Fabris , R. G. Furtado

We consider, in five dimensions, the effective action from heterotic string which includes quantum gravity corrections up to (a')^2. The expansion, in the string frame, is in terms of |a'R|, where R is the scalar curvature and uses the…

High Energy Physics - Theory · Physics 2010-11-05 A. Kuiroukidis

We study nonsingular cosmological scenarios in a general $D$-dimensional string effective action of the dilaton-modulus-axion system in the presence of the matter source. In the standard dilatonic Brans-Dicke parameter ($\omega=-1$) with…

High Energy Physics - Theory · Physics 2014-11-18 Shinji Tsujikawa

We review various aspects of de Sitter spacetime in string theory: its status as an effective field theory spacetime solution, its relation to the vacuum energy problem in string theory, its (global) holographic definition in terms of two…

High Energy Physics - Theory · Physics 2023-08-30 Per Berglund , Tristan Hübsch , Djordje Minic

We study cosmologies based on low-energy effective string theory with higher-order string corrections to a tree-level action and with a modulus scalar field (dilaton or compactification modulus). In the presence of such corrections it is…

High Energy Physics - Theory · Physics 2009-11-11 Shinji Tsujikawa

We introduce a Wheeler-De Witt approach to quantum cosmology based on the low-energy string effective action, with an effective dilaton potential included to account for non-perturbative effects and, possibly, higher-order corrections. We…

High Energy Physics - Theory · Physics 2011-04-15 M. Gasperini

In these notes we address the canonical quantization of the cosmological models which appear as solutions of the low energy effective action of closed bosonic string theory (dilaton models). The analysis is restricted to the quantization of…

Mathematical Physics · Physics 2007-05-23 Gabriel Catren , Claudio Simeone

We have investigated the cosmological scenarios with a four dimensional effective action which is connected with multidimensional, supergravity and string theories. The solution for the scale factor is such that initially universe undergoes…

General Relativity and Quantum Cosmology · Physics 2014-11-17 A. A. Sen , S. Sen

It has been shown a specific Horndeski theory of gravity arises from a consistent Kaluza-Klein reduction of the gravi-dilaton sector of the low-energy effective heterotic string action with a first $\alpha'$ correction. Here we provide a…

High Energy Physics - Theory · Physics 2021-11-03 Damien A. Easson , Tucker Manton , Andrew Svesko

We first make more precise a recent "Hamiltonian" reformulation of the Hohm-Zwiebach approach to the tree-level, $O(d,d)$-invariant string cosmology equations at all orders in the $\alpha'$ expansion, and recall how it allows to give a…

High Energy Physics - Theory · Physics 2025-02-24 P. Conzinu , G. Fanizza , M. Gasperini , E. Pavone , L. Tedesco , G. Veneziano

We consider new cosmological solutions with a collapsing, an intermediate and an expanding phase. The boundary between the expanding (collapsing) phase and the intermediate phase is seen by comoving observers as a cosmological past (future)…

High Energy Physics - Theory · Physics 2009-11-07 L. Cornalba , Miguel S. Costa
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