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Recently, many works have tried to realize cosmological accelerated expansion in string theory models in the asymptotic regions of field space, with a typical scalar potential $V(\varphi)$ having an exponential fall-off $e^{-\gamma\,…

High Energy Physics - Theory · Physics 2023-11-17 David Andriot , Dimitrios Tsimpis , Timm Wrase

Intrinsic and extrinsic geometric properties of string world sheets in curved space-time background are explored. In our formulation, the only dynamical degrees of freedom of the string are its immersion coordinates. Classical equation of…

High Energy Physics - Theory · Physics 2009-10-30 K. S. Viswanathan , R. Parthasarathy

We discuss the hypothesis of a fixed point for quantum gravity coupled to a scalar, in the limit where the scalar field goes to infinity, accompanied by a suitable scaling of the metric. We propose that no scalar potential is present for…

High Energy Physics - Theory · Physics 2010-05-25 C. Wetterich

We study two classes of static uniform black string solutions in a (4+1)-dimensional SU(2) Einstein-Yang-Mills model. These configurations possess a regular event horizon and corresponds in a 4-dimensional picture to axially symmetric black…

High Energy Physics - Theory · Physics 2013-05-29 Y. Brihaye , B. Hartmann , E. Radu

We classify almost all classical string configurations, considered in the framework of the semi-classical limit of the string/gauge theory duality. Then, we describe a procedure for obtaining the conserved quantities and the exact classical…

High Energy Physics - Theory · Physics 2007-05-23 D. Aleksandrova , P. Bozhilov

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

String theory, if it describes nature, is probably strongly coupled. In light of recent developments in string duality, this means that the ``real world'' should correspond to a region of the classical moduli space which admits no weak…

High Energy Physics - Theory · Physics 2009-10-30 Michael Dine , Yuri Shirman

We consider general approach to exactly solvable 2D dilaton cosmology with one-loop backreaction from conformal fields taken into account. It includes as particular cases previous models discussed in literature. We list different types of…

High Energy Physics - Theory · Physics 2009-11-10 O. B. Zaslavskii

The question of whether the universe is eternal or if it had a singular moment of creation is deeply intriguing. Although different versions of steady state and oscillatory models of eternal universe have been envisaged, empirical evidence…

General Relativity and Quantum Cosmology · Physics 2020-03-09 Karthik H. Shankar

When applying T-duality to a generic, non-extreme Killing horizon, T-duality is spacelike on one side and timelike on the other. We show, using simple examples from four-dimensional Einstein-Maxwell theory, that the image of the horizon is…

High Energy Physics - Theory · Physics 2024-09-27 Maxime Medevielle , Thomas Mohaupt

We propose a theory in electromagnetic dynamics, in which time and space are equivalent with each other and have totally twelve dimensions. Then, we solve that with realistic assumptions and find a steady state as a solution. The solution…

General Physics · Physics 2011-08-30 Yoshiro Nohara

A string theory in $3$ euclidean spacetime dimensions is found to describe the semiclassical behavior of a certain exact physical state of quantum general relativity in $4$ dimensions. Both the worldsheet and the three dimensional metric…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Lee Smolin

We find all the classical solutions (minimal surfaces) of open or closed strings in {\it any} two dimensional curved spacetime. As examples we consider the SL(2,R)/R two dimensional black hole, and any 4D black hole in the Schwarzschild…

High Energy Physics - Theory · Physics 2009-10-28 Itzhak Bars , Jürgen Schulze

We study N=2(4) superstring backgrounds which are four-dimensional non-\Kahlerian with non-trivial dilaton and torsion fields. In particular we consider the case that the backgrounds possess at least one $U(1)$ isometry and are…

High Energy Physics - Theory · Physics 2015-06-26 Makoto SAKAGUCHI

A general framework for studying a large class of cosmological solutions of the low-energy limit of type II string theory and of M-theory, with non-trivial Ramond form fields excited, is presented. The framework is applicable to spacetimes…

High Energy Physics - Theory · Physics 2009-10-30 Andre Lukas , Burt A. Ovrut , Daniel Waldram

There is great interest in the construction of brane worlds, where matter and gravity are forced to be effective only in a lower dimensional surface , the brane . How these could appear as a consequence of string theory is a crucial…

High Energy Physics - Theory · Physics 2022-05-04 E. I. Guendelman , J. Portnoy

We describe string frame bouncing universe scenarios involving the creation and annihilation of a non-BPS D9-brane in type IIA superstring theory. We find several classes of solutions, in which the bounce is driven by the tachyon dynamics…

High Energy Physics - Theory · Physics 2014-11-20 Philipp Höffer v. Loewenfeld , Jin U Kang , Nicolas Moeller , Ivo Sachs

The past year has seen enormous progress in string theory. It has become clear that all of the different string theories are different limits of a single theory. Moreover, in certain limits, one obtains a new, eleven-dimensional structure…

High Energy Physics - Theory · Physics 2007-05-23 Michael Dine

We demonstrate that string consistency in four spacetime dimensions leads to a spectrum of string states which satisfies the supertrace constraints Str(M^0)=0 and Str(M^2)=\Lambda at tree level, where \Lambda is the one-loop string…

High Energy Physics - Theory · Physics 2009-10-28 Keith R. Dienes , Moshe Moshe , Robert C. Myers

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
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