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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…

高能物理 - 理论 · 物理学 2008-02-03 K. Behrndt , S. Foerste

We derive a class of solutions to the string sigma-model equations for the closed bosonic string. The tachyon field is taken to form a constant condensate and the beta-function equations at one-loop level are solved for the evolution of the…

高能物理 - 理论 · 物理学 2009-09-25 Alan Kostelecky , Malcolm Perry

We study string theory in supersymmetric time-dependent backgrounds. In the framework of general relativity, supersymmetry for spacetimes without flux implies the existence of a covariantly constant null vector, and a relatively simple form…

高能物理 - 理论 · 物理学 2007-05-23 Michal Fabinger , Simeon Hellerman

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…

高能物理 - 理论 · 物理学 2009-07-30 Kallingalthodi Madhu , K. Narayan

In dilaton gravity theories, we consider a string-like topological defect formed during U(1) gauge symmetry-breaking phase transition in the early Universe, and far from the cosmic string we have vacuum solutions of the generalized Einstein…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Tae Hoon Lee

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…

高能物理 - 理论 · 物理学 2009-10-22 K. Behrndt , S. Foerste

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)…

高能物理 - 理论 · 物理学 2009-11-07 L. Cornalba , Miguel S. Costa

We present exact inhomogeneous and anisotropic cosmological solutions of low-energy string theory containing dilaton and axion fields. The spacetime metric possesses cylindrical symmetry. The solutions describe ever-expanding universes with…

高能物理 - 理论 · 物理学 2009-10-30 John D. Barrow , Kerstin E. Kunze

We consider the theory obtained by adding to the usual string frame dilaton gravity action specially constructed higher derivative terms motivated by the limited curvature construction of [MukhanovET1992a] and determine the spatially…

高能物理 - 理论 · 物理学 2009-10-31 Damien A. Easson , Robert H. Brandenberger

Progress on string theory in curved spacetimes since 1992 are reviewed. After a short introduction on strings in Minkowski and curved spacetimes, we focus on strings in cosmological spacetimes. The classical behaviour of strings in FRW and…

高能物理 - 理论 · 物理学 2009-09-25 H. J. de Vega , N. Sánchez

We consider the low-energy effective string action in four dimensions including the leading order-$\alpha'$ terms. An exact homogeneous solution is obtained. It represents a non-singular expanding cosmological model in which the tensor…

广义相对论与量子宇宙学 · 物理学 2014-11-17 A. A. Al-Nowaiser , Murat Özer , M. O. Taha

We reconsider here the problem of finding the general 4D spherically symmetric, asymptotically flat and time-independent solutions to the lowest-order string equations in the $\ap$ expansion. Our construction includes earlier work, but…

高能物理 - 理论 · 物理学 2010-11-19 C. P. Burgess , R. C. Myers , F. Quevedo

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…

高能物理 - 理论 · 物理学 2007-05-23 K. Behrndt

We present a class of static, spherically symmetric, non-singular solutions of the tree-level string effective action, truncated to first order in $\alpha'$. In the string frame the solutions approach asymptotically (at $r\to 0$ and $r\to…

高能物理 - 理论 · 物理学 2009-10-30 A. Buonanno , M. Gasperini , C. Ungarelli

We argue that traditional methods of compactification of string theory make it very difficult to understand how the cosmological constant becomes zero. String inspired models can give zero cosmological constant after fine tuning but since…

高能物理 - 理论 · 物理学 2009-10-31 S. P. de Alwis , A. T. Flournoy , N. Irges

We show that a class of 3+1 dimensional Friedmann-Robertson-Walker cosmologies can be embedded within a variety of solutions of string theory. In some realizations the apparent singularities associated with the big bang or big crunch are…

高能物理 - 理论 · 物理学 2016-09-06 Finn Larsen , Frank Wilczek

In a universe whose elementary constituents are point particles there does not seem to be any obvious mechanism for avoiding the initial singularities in physical quantities in the standard model of cosmology. In contrast in string theory…

广义相对论与量子宇宙学 · 物理学 2009-10-30 Sanjay Jain

We present arguments for the existence of new black string solutions with negative cosmological constant. These higher-dimensional configurations have no dependence on the `compact' extra dimension, and their conformal infinity is the…

高能物理 - 理论 · 物理学 2009-11-11 Robert B. Mann , Eugen Radu , Cristian Stelea

There are no reasons why the singularity in the growth of the dilaton coupling should not be regularised, in a string cosmological context, by the presence of classical inhomogeneities. We discuss a class of inhomogeneous dilaton-driven…

高能物理 - 理论 · 物理学 2010-11-19 Massimo Giovannini

In the context of a cosmological string model describing the propagation of strings in a time-dependent Robertson-Walker background space-time, we show that the asymptotic acceleration of the Universe can be identified with the square of…

高能物理 - 理论 · 物理学 2009-09-11 John Ellis , N. E. Mavromatos , D. V. Nanopoulos