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We address the problem of describing different closed string backgrounds in background independent open string field theory: A shift in the closed string background corresponds to a collective excitation of open strings. As an illustration…

High Energy Physics - Theory · Physics 2009-01-30 Marco Baumgartl , Ivo Sachs

String cosmology models predict a stochastic cosmic background of gravitational waves with a characteristic spectrum. I describe the background, present astrophysical and cosmological bounds on it, and outline how it may be possible to…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Ram Brustein

We start a systematic study of string theory in AdS_3 black hole backgrounds. Firstly, we analyse in detail the geodesic structure of the BTZ black hole, including spacelike geodesics. Secondly, we study the spectrum for massive and…

High Energy Physics - Theory · Physics 2009-11-07 Jan Troost

The cosmological constant is an unexplained until now phenomena of nature that requires an explanation through string effects. The apparent discrepancy between theory and experiment is enourmous and has already been explained several times…

General Physics · Physics 2007-05-23 Gordon Chalmers

We study the cosmological implications of the one-loop terms in the string expansion. In particular, we find non-singular solutions which interpolate between a contracting universe and an expanding universe, and show that these solutions…

High Energy Physics - Theory · Physics 2009-10-30 Richard Easther , Kei-ichi Maeda

In the first part of the present paper, we show that O(d,d)-invariance usually known in a homogeneous cosmological background written in terms of proper time can be extended to backgrounds depending on one or several coordinates (which may…

General Relativity and Quantum Cosmology · Physics 2015-06-25 Jacques Demaret , Elisa Di Pietro

The strong coupling dynamics of string theories in dimension $d\geq 4$ are studied. It is argued, among other things, that eleven-dimensional supergravity arises as a low energy limit of the ten-dimensional Type IIA superstring, and that a…

High Energy Physics - Theory · Physics 2010-04-07 Edward Witten

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 explore the cosmological dynamics of a minimalistic yet generic string-inspired model for multifield dark energy. Adopting a supergravity four-dimensional viewpoint, we motivate the model's structure arising from superstring…

High Energy Physics - Theory · Physics 2024-02-16 Diego Gallego , J. Bayron Orjuela-Quintana , César A. Valenzuela-Toledo

This article reviews recent developments in the study of universes with a positive cosmological constant in string theory.

High Energy Physics - Theory · Physics 2009-11-10 Vijay Balasubramanian

The 1--loop string background equations with axion and dilaton fields are shown to be integrable in four dimensions in the presence of two commuting Killing symmetries and $\delta c = 0$. Then, in analogy with reduced gravity, there is an…

High Energy Physics - Theory · Physics 2009-10-28 I. Bakas

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 paper we investigate compactifications of the type II and heterotic string on four-dimensional spaces with nongeometric monodromies. We explicitly construct backgrounds which contain the "Duality Twists" discussed by Dabholkar and…

High Energy Physics - Theory · Physics 2014-11-18 Alex Flournoy , Brian Wecht , Brook Williams

We briefly review certain aspects of cosmic microwave background anisotropies as generated in passive and active models of structure formation. We then focus on cosmic strings based models and discuss their status in the light of current…

Astrophysics · Physics 2009-11-07 Alejandro Gangui , Levon Pogosian , Serge Winitzki

We present mechanisms for generating conical singularities both in three and four-dimensions in the systems with copies of scalar or chiral multiplets coupled to $N=2$ or $N=1$ supergravity. Our mechanisms are useful for supersymmetry…

High Energy Physics - Theory · Physics 2009-10-28 Hitoshi Nishino

A new class of spatially homogeneous 4D string backgrounds, the $X(d\rightarrow)$ according to a recent classification, is presented and shown to contain only five generic types. In contrast to the case of $X(d\uparrow)$ (which contains as…

High Energy Physics - Theory · Physics 2009-10-28 Nikolaos A. Batakis

We present exact solutions of string cosmological models characterized by five dimensional metrics (with four-dimensional real Lie groups as isometry groups), space independent dilaton and vanishing torsion. As an example we consider VII 0…

High Energy Physics - Theory · Physics 2012-03-27 B. Mojaveri , A. Rezaei-Aghdam

We investigate cosmologies where the accelerated expansion of the Universe is driven by a field with an anisotropic equation of state. We model such scenarios within the Bianchi I framework, introducing two skewness parameters to quantify…

Astrophysics · Physics 2009-06-23 Tomi Koivisto , David F. Mota

There is evidence that string theory possesses a large discretuum of stable and/or metastable ground states, with zero or four supersymmetries in four dimensions. I discuss critically the nature of this evidence. Assuming this "landscape"…

High Energy Physics - Theory · Physics 2017-08-23 Michael Dine

We present some phenomenological aspects of the pre-big-bang cosmological model inspired by the duality properties of string theory. In particular, assuming the spatial sections of the homogeneous background geometry to be isotropic, we…

Astrophysics · Physics 2012-10-23 R. Durrer , K. E. Kunze , M. Sakellariadou
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