ID: hep-th/0204074

Cosmic String Production Towards the End of Brane Inflation

April 8, 2002

View on ArXiv

Similar papers 3

Observational constraints on cosmological superstrings

March 13, 2016

88% Match
Olga S. Sazhina, Alfiia I. Mukhaeva
Cosmology and Nongalactic As...

From theoretical point of view and not being in contradiction with current observational data, the cosmic strings should have fundamentally different origin and are characterized by wide range of energies. The paper is devoted to search for possible cosmological observational tests on superstring theory, among them to identification of observational characteristics to distinguish between cosmological superstring of different types. In the brane-world scenario with an assumpti...

Find SimilarView on arXiv

Formation & evolution of cosmic superstrings: a short review

January 11, 2010

88% Match
M. Sakellariadou
Cosmology and Nongalactic As...

I will briefly review the formation and evolution of cosmic superstrings, in the context of brane-world cosmological models within M-theory. These objects can play the role of cosmic strings, offering a variety of astrophysical consequences, which I will briefly discuss.

Find SimilarView on arXiv

Theoretical constraints on brane inflation and cosmic superstring radiation

May 9, 2011

88% Match
Rhiannon Gwyn, Mairi Sakellariadou, Spyros Sypsas
Cosmology and Nongalactic As...

We analyze theoretical constraints on the consistency of brane inflation leading to cosmic superstring formation and on the subsequent radiation of these cosmic superstrings. We first investigate the implications of recently elucidated supergravity constraints on models of brane inflation. We show that both D3/D7 and D3/anti-D3 brane inflation are subject to non-trivial constraints. Both models can be shown to satisfy those constraints, but for the case of D3/D7 there may be ...

Find SimilarView on arXiv

Inflationary Scenarios from Branes at Angles

December 17, 2001

88% Match
J. CERN Garcia-Bellido, R. CERN Rabadan, F. CERN Zamora
High Energy Physics - Theory
High Energy Physics - Phenom...

We describe a simple mechanism that can lead to inflation within string-based brane-world scenarios. The idea is to start from a supersymmetric configuration with two parallel static Dp-branes, and slightly break the supersymmetry conditions to produce a very flat potential for the field that parametrises the distance between the branes, i.e. the inflaton field. This breaking can be achieved in various ways: by slight relative rotations of the branes with small angles, by con...

Find SimilarView on arXiv

Brane Inflation and Cosmic String Tension in Superstring Theory

January 13, 2005

88% Match
Hassan Firouzjahi, S. -H. Henry Tye
High Energy Physics - Theory
Astrophysics
General Relativity and Quant...
High Energy Physics - Phenom...

In a simple reanalysis of the KKLMMT scenario, we argue that the slow roll condition in the D3-anti-D3-brane inflationary scenario in superstring theory requires no more than a moderate tuning. The cosmic string tension is very sensitive to the conformal coupling: with less fine-tuning, the cosmic string tension (as well as the ratio of tensor to scalar perturbation mode) increases rapidly and can easily saturate the present observational bound. In a multi-throat brane inflat...

Find SimilarView on arXiv

Production of topological defects at the end of inflation

January 31, 2007

88% Match
Mairi KCL London Sakellariadou
High Energy Physics - Theory

Hybrid inflation within supersymmetric grand unified theories, as well as inflation through brane collisions within braneworld cosmological models, lead to the formation of one-dimensional defects. Observational data, mainly from the cosmic microwave background temperature anisotropies but also from the gravitational wave background, impose constraints on the free parameters of the models. I review these inflationary models and discuss the constraints from the currently avail...

Find SimilarView on arXiv

Energy Radiation by Cosmic Superstrings in Brane Inflation

October 25, 2007

88% Match
Hassan Firouzjahi
High Energy Physics - Theory
Astrophysics
General Relativity and Quant...
High Energy Physics - Phenom...

The dominant method of energy loss by a loop of cosmic D-strings in models of warped brane inflation is studied. It is shown that the energy loss via Ramond-Ramond field radiation can dominate by many orders of magnitude over the energy radiation via gravitational wave emission. The ratio of these two energy loss mechanisms depends on the energy scale of inflation, the mass scale of string theory and whether it is a single-throat or a multi-throat inflationary scenario. This ...

Find SimilarView on arXiv

Seeing through the String Landscape - a String Hunter's Companion in Particle Physics and Cosmology

April 29, 2009

88% Match
Dieter Lust
High Energy Physics - Theory

In this article we will overview several aspects of the string landscape, namely intersecting D-brane models and their statistics, possible model independent LHC signatures of intersecting brane models, flux compactification, moduli stabilization in type II compactifications, domain wall solutions and brane inflation.

Find SimilarView on arXiv

Strings, Branes and Cosmology: What can we hope to learn?

June 2, 2006

88% Match
C. P. Burgess
High Energy Physics - Theory

This article briefly summarizes the motivations for -- and recent progress in -- searching for cosmological configurations within string theory, with a focus on how much we might reasonably hope to learn about fundamental physics from precision cosmological measurements.

Find SimilarView on arXiv

Formation and evolution of cosmic D-strings

November 30, 2003

88% Match
Gia Dvali, Alexander Vilenkin
High Energy Physics - Theory

We study the formation of D and F-cosmic strings in D-brane annihilation after brane inflation. We show that D-string formation by quantum de Sitter fluctuations is severely suppressed, due to suppression of RR field fluctuations in compact dimensions. We discuss the resonant mechanism of production of D and F-strings, which are formed as magnetic and electric flux tubes of the two orthogonal gauge fields living on the world-volume of the unstable brane. We outline the subseq...

Find SimilarView on arXiv