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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

Following the holographic description of linear dilaton null Cosmologies with a Big Bang in terms of Matrix String Theory put forward by Craps, Sethi and Verlinde, we propose an extended background describing a Universe including both Big…

高能物理 - 理论 · 物理学 2008-11-26 J. Bedford , C. Papageorgakis , D. Rodriguez-Gomez , J. Ward

We present cosmological solutions for (1+3+n)-dimensional steady state universe in dilaton gravity with an arbitrary dilaton coupling constant w and exponential dilaton self-interaction potentials in the string frame. We focus particularly…

广义相对论与量子宇宙学 · 物理学 2013-03-01 Ozgur Akarsu , Tekin Dereli

The BFSS matrix model is a suggested non-perturbative definition of string theory. Starting from a thermal state of this matrix model, we show how space and time can emerge dynamically. Results from the IKKT matrix model indicate that the…

高能物理 - 理论 · 物理学 2022-12-07 Suddhasattwa Brahma , Robert Brandenberger , Samuel Laliberte

In the standard picture of cosmological structure formation, the Universe we see today is evolved under the gravitational instability from tiny random fluctuations. In this talk I discuss the onset of non-linearity in the large scale…

天体物理学 · 物理学 2007-05-23 Lung-Yih Chiang

The aim of this talk is to provide non-experts with a brief and elementary introduction on the field of extra dimensions. The main motivation for extra dimensions relies on the more fundamental string theories that predict ten (or eleven)…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Quiros

In models of spacetime that are the product of a four-dimensional spacetime with an ``extra'' dimension, there is the possibility that the extra dimension will collapse to zero size, forming a singularity. We ask whether this collapse is…

广义相对论与量子宇宙学 · 物理学 2009-11-07 James Geddes

String theory, as a theory containing quantum gravity, is usually thought to require more dimensions of spacetime than the usual 3+1. Here I argue on physical grounds that needing extra dimensions for strings may well be an artefact of…

广义相对论与量子宇宙学 · 物理学 2011-10-25 John Swain

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

In this contribution we identify two scenarios for the evolutionary branch cut universe. In the first scenario, the universe evolves continuously from the negative complex cosmological time sector, prior to a primordial singularity, to the…

广义相对论与量子宇宙学 · 物理学 2021-05-19 C. A. Z. Vasconcellos , P. O. Hess , D. Hadjimichef , B. Bodmann , M. Razeira , G. L. Volkmer

An interpretation of spacelike singularities in string theory uses target space duality to relate the collapsing Schwarzschild geometry near the singularity to an inflationary cosmology in dual variables. An appealing picture thus results…

高能物理 - 理论 · 物理学 2010-04-06 Emil Martinec

Scenario of a bouncing universe is one of the most active area of research to arrive at singularity free cosmological models. Different proposals have been suggested to avoid the so called 'big bang' singularity through the quantum aspect…

广义相对论与量子宇宙学 · 物理学 2022-10-26 Indrani Banerjee , Tanmoy Paul , Soumitra SenGupta

Bucher [Bucher2001] has recently proposed an interesting brane-world cosmological scenario where the ``Big Bang'' hypersurface is the locus of collision of two vacuum bubbles which nucleate in a five dimensional flat space. This gives rise…

高能物理 - 理论 · 物理学 2008-11-26 Jaume Garriga , Takahiro Tanaka

Despite impressive phenomenological successes, cosmological models are incomplete without an understanding of what happened at the big bang singularity. Depending on the model, one would like to understand how appropriate initial conditions…

高能物理 - 理论 · 物理学 2010-01-26 Ben Craps

We suggest that the "Big Bang" may be a result of the first-order phase transition driven by changing scalar curvature of the 4D space-time in expanding cold Universe, filled with nonlinear scalar field $\phi $ and neutral matter with…

广义相对论与量子宇宙学 · 物理学 2016-05-04 E. A. Pashitskii , V. I. Pentegov

We consider branching of baby universes off parent one in (1+1)-dimensional dilaton gravity with 24 types of conformal matter fields. This theory is equivalent to string theory in a certain background in D=26-dimensional target space, so…

高能物理 - 理论 · 物理学 2011-09-09 V. A. Rubakov

Changing the dimensionality of the space-time at the smallest and largest distances has manifold theoretical advantages. If the space is lower dimensional in the high energy regime, then there are no ultraviolet divergencies in field…

高能物理 - 理论 · 物理学 2015-06-19 Niayesh Afshordi , Dejan Stojkovic

Big bang/crunch curvature singularities in exact CFT string backgrounds can be removed by turning on gauge fields. This is described within a family of {SL(2)xSU(2)xU(1)_x}/{U(1)xU(1)} quotient CFTs. Uncharged incoming wavefunctions from…

高能物理 - 理论 · 物理学 2009-11-07 Shmuel Elitzur , Amit Giveon , Eliezer Rabinovici

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 ekpyrotic and cyclic universe scenarios have revived the idea that the density perturbations apparent in today's universe could have been generated in a `pre-singularity' epoch before the big bang. These scenarios provide explicit…

高能物理 - 理论 · 物理学 2009-11-07 Christopher Gordon , Neil Turok