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Related papers: String cosmology and dilaton

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Supersymmetry breaking in string theory is expected to occur when moduli fields acquire non-trivial expectation values. In the early universe these fields start out displaced from their final destinations. I present some recent ideas about…

High Energy Physics - Theory · Physics 2007-05-23 R. Brustein

We propose a new method for identifying new physics imprints on present observational data in cosmology whereby signatures of string theory are clearly distinguished from imprints of possible features on the inflaton potential. Our method…

High Energy Physics - Phenomenology · Physics 2009-11-10 Steen Hannestad , Laura Mersini-Houghton

Super--inflation driven by dilaton/moduli kinetic energy is naturally realized in compactified string theory. Discussed are selected topics of recent development in string inflationary cosmology: kinematics of super-inflation, graceful exit…

High Energy Physics - Theory · Physics 2008-02-03 Soo-Jong Rey

We review recent developments in the field of string cosmology with particular emphasis on open problems having to do mainly with geometric asymptotics and singularities. We discuss outstanding issues in a variety of currently popular…

High Energy Physics - Theory · Physics 2017-02-22 Ignatios Antoniadis , Spiros Cotsakis

The dynamics of the early universe may have been profoundly influenced by spatial anisotropies. A search for such backgrounds in the context of string cosmology has uncovered the existence of an entire class of (spatatially) homogeneous but…

High Energy Physics - Theory · Physics 2016-09-06 N. A. Batakis , A. A. Kehagias

This is a pedagogical introduction to the basics of the cosmic string theory and also a review of the recent progress made with respect to the macrophysical predictions of the theory. Topics covered include, string formation and evolution,…

Astrophysics · Physics 2009-09-25 L. Perivolaropoulos

We generalize a five dimensional black hole solution of low energy effective string theory to arbitrary constant spatial curvature. After interchanging the signature of time and radius we reduce the 5d solution to four dimensions and obtain…

High Energy Physics - Theory · Physics 2011-08-17 K. Behrndt , S. Foerste

In these lectures, I review the current status of cosmic strings and cosmic superstrings. I first discuss topological defects in the context of Grand Unified Theories, focusing in particular in cosmic strings arising as gauge theory…

High Energy Physics - Theory · Physics 2009-10-06 Mairi Sakellariadou

A pedagogical introduction to aspects of string cosmology, including the landscape (BPBT) solution to the cosmological constant problem, brane-antibrane inflation, warped compactification, the KKLMMT model, the eta problem of SUGRA models,…

High Energy Physics - Theory · Physics 2016-09-22 James M. Cline

It has long been known that strings wound around incontractible cycles can play a vital role in cosmology. In particular, in a spacetime with toroidal spatial hypersurfaces, the dynamics of the winding modes may help yield three large…

High Energy Physics - Theory · Physics 2010-11-19 Richard Easther , Brian R. Greene , Mark G. Jackson

A review is attempted of physical motivations, theoretical and phenomenological aspects, as well as outstanding problems, of the pre-big bang scenario in string cosmology.

High Energy Physics - Theory · Physics 2015-06-25 G. Veneziano

This article, written for Scolarpedia, provides a brief introduction into the subject of cosmic strings, together with a review of their main properties, cosmological evolution and observational signatures.

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Tanmay Vachaspati , Levon Pogosian , Daniele Steer

In string theory, the traditional picture of a Universe that emerges from the inflation of a very small and highly curved space-time patch is a possibility, not a necessity: quite different initial conditions are possible, and not…

High Energy Physics - Theory · Physics 2017-06-01 M. Gasperini , G. Veneziano

Scale factor duality, a truncated form of time dependent T-duality, is a symmetry of string effective action in cosmological backgrounds interchanging small and large scale factors. The symmetry suggests a cosmological scenario…

High Energy Physics - Theory · Physics 2009-10-31 Ram Brustein

We study two-dimensional string theory on a time-dependent background, whose worldsheet description consists of Liouville theory at central charge c = 1 and Liouville theory at central charge c = 25, together with the conformal ghosts. We…

High Energy Physics - Theory · Physics 2024-05-21 Victor A. Rodriguez

String gas cosmology is rewritten in the Einstein frame. In an effective theory in which a gas of closed strings is coupled to a dilaton gravity background without any potential for the dilaton, the Hagedorn phase which is quasi-static in…

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 construct cosmological spacetimes with null Kasner-like singularities as purely gravitational solutions with no other background fields turned on. These can be recast as anisotropic plane-wave spacetimes by coordinate transformations. We…

High Energy Physics - Theory · Physics 2009-07-30 Kallingalthodi Madhu , K. Narayan

The chameleonic behaviour of the String theory dilaton is suggested. Some of the possible consequences of the chameleonic string dilaton are analyzed in detail. In particular, (1) we suggest a new stringy solution to the cosmological…

High Energy Physics - Theory · Physics 2011-11-10 Andrea Zanzi

D-branes are fundamental in all scenarios where there are large extra dimensions and the string scale is much smaller than the four-dimensional Planck mass. We show that this current picture leads to a new approach to string cosmology where…

High Energy Physics - Phenomenology · Physics 2009-10-31 Antonio Riotto
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