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Recent work has proposed the principle of `asymptotic past triviality' to characterize the initial state in the pre-big bang scenario of string cosmology, that it is a generic perturbative solution of the low-energy effective action. Among…

高能物理 - 理论 · 物理学 2009-10-31 Richard Madden

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…

高能物理 - 理论 · 物理学 2017-06-01 M. Gasperini , G. Veneziano

Classical and quantum gravitational instabilities, can, respectively, inflate and warm up a primordial Universe satisfying a superstring-motivated principle of "Asymptotic Past Triviality". A physically viable big bang is thus generated…

高能物理 - 理论 · 物理学 2007-05-23 G. Veneziano

We calculate the density and gravitational wave spectrums generated in a version of string cosmology termed pre-big bang scenario. The large scale structures are originated from quantum fluctuations of the metric and dilaton field during a…

高能物理 - 理论 · 物理学 2011-05-23 J. Hwang

The production of a background of super-horizon curvature perturbations with the appropriate (red) spectrum needed to trigger the cosmic anisotropies observed on large scales is associated, in the context of pre-big bang inflation, with a…

广义相对论与量子宇宙学 · 物理学 2017-09-08 M. Gasperini

We analyse numerically the onset of pre-big bang inflation in an inhomogeneous, spherically symmetric Universe. Adding a small dilatonic perturbation to a trivial (Milne) background, we find that suitable regions of space undergo…

广义相对论与量子宇宙学 · 物理学 2010-02-03 J. Maharana , E. Onofri , G. Veneziano

A string cosmology scenario ("pre-big-bang") postulates that the evolution of the Universe starts from a state of very small curvature and coupling, undergoes a long phase of dilaton-driven kinetic inflation and at some later time joins…

高能物理 - 理论 · 物理学 2016-10-26 Ram Brustein

An inhomogeneous version of pre--Big Bang cosmology emerges, within string theory, from quite generic initial conditions, provided they lie deeply inside the weak-coupling, low-curvature regime. Large-scale homogeneity, flatness, and…

高能物理 - 理论 · 物理学 2009-10-30 G. Veneziano

We generalize previous work on inhomogeneous pre-big bang cosmology by including the effect of non-trivial moduli and antisymmetric-tensor/axion fields. The general quasi-homogeneous asymptotic solution---as one approaches the big bang…

高能物理 - 理论 · 物理学 2009-10-30 A. Buonanno , K. A. Meissner , C. Ungarelli , G. Veneziano

We propose a picture, within the pre-big-bang approach, in which the universe emerges from a bath of plane gravitational and dilatonic waves. The waves interact gravitationally breaking the exact plane symmetry and lead generically to…

高能物理 - 理论 · 物理学 2014-11-18 A. Feinstein , K. E. Kunze , M. A. Vazquez-Mozo

The beautiful scenario of pre-big-bang cosmology is appealling not only because it is more or less derived from string theory, but also because it separates clearly the problem of the initial conditions for the universe from that of high…

高能物理 - 理论 · 物理学 2007-05-23 M. Borunda , M. Ruiz-Altaba

I report recent studies on the evolution of perturbations in the context of the ``pre-big-bang" scenario typical of string cosmology, with emphasis on the formation of a stochastic background of relic photons and gravitons, and its possible…

高能物理 - 理论 · 物理学 2009-09-25 M. Gasperini

We study the collapse of the universe described by a scalar field spherically symmetric collapse of a system described by a massless scalar field from a 5D Riemann-flat canonical metric, on which we make a dynamical foliation on the extra…

广义相对论与量子宇宙学 · 物理学 2015-05-28 Mauricio Bellini

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

We present a short introduction to a non-standard cosmological scenario motivated by the duality symmetries of string theory, in which the big bang singularity is replaced with a "big bounce" at high but finite curvature. The bouncing epoch…

高能物理 - 理论 · 物理学 2022-08-03 M. Gasperini

The Pre-Big Bang cosmology inspired generations of cosmologists in attempts to cure the initial Big Bang singularity using a fundamental length scale as proposed by String Theory. The existence of a phase of collapse/inflation with…

广义相对论与量子宇宙学 · 物理学 2022-07-14 V. Bozza

The duality-type symmetries of string cosmology naturally lead to a pre-big-bang phase of accelerated evolution as dual counterpart of the decelerated expansion of standard cosmology. We discuss several properties of this scenario,…

高能物理 - 理论 · 物理学 2011-05-23 M. Gasperini , G. Veneziano

This paper presents a review of the basic, model-independent differences between the pre-big bang scenario, arising naturally in a string cosmology context, and the standard inflationary scenario. We use an unconventional approach in which…

高能物理 - 理论 · 物理学 2010-04-06 M. Gasperini

The pre-big-bang cosmology inspired by superstring theories has been suggested as an alternative to slow-roll inflation. We analyze, in both the Jordan and Einstein frames, the effect of spatial curvature on this scenario and show that too…

高能物理 - 理论 · 物理学 2016-08-25 Michael S. Turner , Erick J. Weinberg

General non-singular accelerating cosmological solutions for an initial cosmic period of pure vacuum birth era are derived. This vacuum era is described by a varying cosmological "constant" suggested by the Renormalisation Group flow of…

广义相对论与量子宇宙学 · 物理学 2016-11-23 Georgios Kofinas , Vasilios Zarikas
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