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Related papers: Acceleration of the Universe, String Theory and a …

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Recent astronomical observations indicate that the universe is accelerating. We argue that generic quintessence models that accommodate the present day acceleration tend to accelerate eternally. As a consequence the resulting spacetimes…

High Energy Physics - Theory · Physics 2010-02-03 W. Fischler , A. Kashani-Poor , R. McNees , S. Paban

It has been argued in the literature that if a universe is expanding with an accelerating rate indefinitely, it presents a challenge to string theories due to the existence of event horizons. We study the fate of a currently accelerating…

Astrophysics · Physics 2007-05-23 Xiao-Gang He

We discuss the obstacles for defining a set of observable quantities analogous to an S-matrix which are needed to formulate string theory in an accelerating universe. We show that the quintessence models with the equations of state $-1 < w…

High Energy Physics - Theory · Physics 2009-11-07 Simeon Hellerman , Nemanja Kaloper , Leonard Susskind

We propose that the existence of the string landscape suggests the universe can be in a quantum glass state, where an extremely large viscosity is generated, and long distance dynamics slows down. At the same time, the short distance…

High Energy Physics - Theory · Physics 2010-10-27 Jian-Huang She

Increasing astronomical evidence indicates that the expansion of the universe is accelerating. By simply solving Einstein equations we show in this letter that a wide class of generic quintessence models leading to eternal acceleration is…

Astrophysics · Physics 2009-11-07 Pedro F. González-Díaz

It is shown that if a small negative cosmological constant is added to quintessence models with equation of state $p=\omega\rho$ on the range $-1 <\omega < -1/3$, the resulting scenarios could not contain any future event horizons.…

Astrophysics · Physics 2007-05-23 Pedro F. Gonzalez-Diaz

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

Recently it was observed that the hyperbolic compactification of M/string theory related to S-branes may lead to a transient period of acceleration of the universe. We study time evolution of the corresponding effective 4d cosmological…

High Energy Physics - Theory · Physics 2009-09-29 Michael Gutperle , Renata Kallosh , Andrei Linde

The presently accelerating universe may keep accelerating forever, eventually run into the event horizon problem, and thus be in conflict with the superstring idea. In the other way around, the current accelerating phase as well as the fate…

Astrophysics · Physics 2009-11-06 Je-An Gu , W-Y. P. Hwang

A new speculative model for the expansion of our universe has been under development by the author for the last two decades, which correctly predicts astronomical measurements with no dark matter or dark energy. This new closed model (no…

General Physics · Physics 2010-02-16 Charles B. Leffert

The accelerating expansion of the universe presents an exciting, fundamental challenge to the standard models of particle physics and cosmology. I highlight some of the outstanding challenges in both developing theoretical models and…

Astrophysics · Physics 2008-11-26 Eric V. Linder

We critically assess the twin prospects of describing the observed universe in string theory, and using cosmological experiments to probe string theory. For the purposes of this short review, we focus on the limitations imposed by our…

High Energy Physics - Theory · Physics 2015-05-30 C. P. Burgess , Liam McAllister

It is shown that varying speed of light cosmology follows from a string-inspired minimal length uncertainty relation. Due to the reduction of the available phase space volume per quantum mode at short wavelengths, the equation of state of…

Astrophysics · Physics 2009-11-07 J. C. Niemeyer

In string gas cosmology, the extra dimensions of the underlying theory are kept at a microscopic scale by a gas of strings. In the matter-dominated era, however, dust pressure can lead to oscillations of the extra dimensions and to…

High Energy Physics - Theory · Physics 2009-11-05 Francesc Ferrer

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)…

High Energy Physics - Theory · Physics 2009-11-07 L. Cornalba , Miguel S. Costa

We review the existence, formation and properties of cosmic strings in string theory, the wide variety of observational techniques that are being employed to detect them, and the constraints that current observations impose on string theory…

High Energy Physics - Theory · Physics 2015-05-28 Edmund J. Copeland , Levon Pogosian , Tanmay Vachaspati

Observations provide increasingly strong evidence that the universe is accelerating. This revolutionary advance in cosmological observations confronts theoretical cosmology with a tremendous challenge, which it has so far failed to meet.…

Astrophysics · Physics 2008-11-26 Ruth Durrer , Roy Maartens

Accelerating universe or the existence of a small and positive cosmological constant is probably the most pressing obstacle as well as opportunity to significantly improving the models of four-dimensional cosmology from fundamental theories…

High Energy Physics - Theory · Physics 2009-10-23 Ishwaree P Neupane

It was recently shown that velocity-dependent forces between parallel fundamental strings moving apart in a $D-$dimensional spacetime implied an accelerating expanding universe in $D-1$-dimensional space-time. Exact solutions were obtained…

High Energy Physics - Theory · Physics 2009-11-07 Ramzi R. Khuri , Andriy Pokotilov

The problem of explaining the acceleration of the expansion of the universe and the observational and theoretical difficulties associated with dark matter and dark energy are discussed. The possibility that GR does not correctly describe…

Astrophysics · Physics 2007-05-23 J. W. Moffat
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