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A large class of cosmological solutions (of the Einstein equations) in string theory, in the presence of Maxwell fields, is obtained by $O(d,d)$ transformations of simple backgrounds with $d$ toroidal isometries. In all the examples in…

High Energy Physics - Theory · Physics 2011-07-19 Amit Giveon , Andrea Pasquinucci

We study a class of four dimensional, anisotropic string backgrounds and analyse their expansion and singularity structure. In particular we will see how O(3,3) duality acts on this class.

High Energy Physics - Theory · Physics 2010-02-03 B. Andreas

The elements of $O(d,d,\Z)$ are shown to be discrete symmetries of the space of curved string backgrounds that are independent of $d$ coordinates. The explicit action of the symmetries on the backgrounds is described. Particular attention…

High Energy Physics - Theory · Physics 2009-10-22 Amit Giveon , Martin Rocek

A new method for obtaining dual string theory backgrounds is presented. Preservation of the Hamiltonian density and the energy momentum tensor induced by O(d,d)-transformations leads to a relation between dual sets of coordinate one-forms…

High Energy Physics - Theory · Physics 2015-06-19 Felix Rennecke

I argue that string theory compactified on a Riemann surface crosses over at small volume to a higher dimensional background of supercritical string theory. Several concrete measures of the count of degrees of freedom of the theory yield…

High Energy Physics - Theory · Physics 2008-11-26 Eva Silverstein

The origin of Big Bang singularity in 3+1 dimensions can be understood in an exact string theory background obtained by an analytic continuation of a cigar like geometry with a nontrivial dilaton. In a T-dual conformal field theory picture…

High Energy Physics - Theory · Physics 2011-11-10 Shinji Hirano , Anupam Mazumdar

Two dimensional charged black hole solution is obtained by implementing an $O(2,2)$ transformation on the three dimensional black string solution. Two different monopole backgrounds in five dimensions are related through an $O(2,2)$…

High Energy Physics - Theory · Physics 2007-05-23 S. Pratik Khastgir , Jnanadeva Maharana

Proposals that $O(d,d)$ boosts of trivial backgrounds lead to non-trivial conformally invariant backgrounds are checked to two loop order. We find that conformal invariance can be achieved by adding simple higher order corrections to the…

High Energy Physics - Theory · Physics 2009-10-22 J. Panvel

A straightforward generalization of the celebrated uniqueness theorem to dimensions greater than four was recently found to fail in two pure gravity cases - the 5d rotating black ring and the black string on R^{3,1} * S^1. Two amendments…

High Energy Physics - Theory · Physics 2007-05-23 Barak Kol

$D$ dimensional neutral black strings wrapped on a circle are related to $(D-1)$ dimensional charged black holes by boosts. We show that the boost has to be performed in the covering space and the boosted coordinate has to be compactified…

High Energy Physics - Theory · Physics 2010-11-19 Sumit R. Das , Samir D. Mathur , S. Kalyana Rama , P. Ramadevi

We present exact solutions characterised by Bianchi-type I,II,III,V,VI four-dimensional metric, space-independent dilaton, and vanishing torsion background, for the low energy string effective action with zero central charge deficit. We…

High Energy Physics - Theory · Physics 2010-04-06 M. Gasperini , R. Ricci

We compute string scattering amplitudes in an orbifold of Minkowski space by a boost, and show how certain divergences in the four point function are associated with graviton exchange near the singularity. These divergences reflect large…

High Energy Physics - Theory · Physics 2009-11-07 Micha Berkooz , Ben Craps , David Kutasov , Govindan Rajesh

We study the classical dynamics of a bosonic string in the $D$--dimensional flat Friedmann--Robertson--Walker and Schwarzschild backgrounds. We make a perturbative development in the string coordinates around a {\it null} string…

General Relativity and Quantum Cosmology · Physics 2009-10-28 Carlos O. Lousto , N. Sanchez

We evolve a scalar field in a fixed Kerr-Schild background geometry to test simple $(3+1)$-dimensional algorithms for singularity excision. We compare both centered and upwind schemes for handling the shift (advection) terms, as well as…

General Relativity and Quantum Cosmology · Physics 2009-11-07 H. J. Yo , T. W. Baumgarte , S. L. Shapiro

We examine background solutions of black hole type arising from the string effective action in five dimensions. We derive the unique metric - dilaton vacuum which is a Schwarzschild type black hole. It is found that it can be extended to…

High Energy Physics - Theory · Physics 2014-11-18 C. Chiou-Lahanas , G. A. Diamandis , B. C. Georgalas

We study higher order corrections to extremal black holes/black string in five dimensions. These higher order corrections are due to supersymmetric completion of R**2 term in five dimensions. By making use of the results we extend the…

High Energy Physics - Theory · Physics 2008-11-26 Mohsen Alishahiha

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

We test whether static charged dilaton black holes in 2+1 dimensions can be turned into naked singularities, by sending in test particles from infinity. We derive that overcharging is possible and generic for both extremal and nearly…

General Relativity and Quantum Cosmology · Physics 2020-12-01 Koray Düztaş , Mubasher Jamil

It is shown that perturbations around backgrounds with one non-homogeneous dimension, namely of co-homogeneity 1, can be canonically simplified, a property that is shown to hold to any order in perturbation theory. Recalling that the…

High Energy Physics - Theory · Physics 2007-09-21 Barak Kol

We present arguments for the existence of charged, rotating black holes in $d=2N+1$ dimensions, with $d\geq 5$ with a positive cosmological constant. These solutions posses both, a regular horizon and a cosmological horizon of spherical…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Y. Brihaye , T. Delsate
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