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Related papers: Inflation from Tachyon Condensation, Large N Effec…

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We study the possibility to construct an observationally viable scenario where both early Inflation and the recently detected accelerated expansion of the universe can be explained by using a single scalar field associated with the Tachyon.…

General Relativity and Quantum Cosmology · Physics 2009-11-11 Victor H. Cardenas

In this lecture I will review the present status of 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…

Astrophysics · Physics 2007-05-23 Juan Garcia-Bellido

We analyze warm tachyonic inflation, proposed in the literature, but from the viewpoint of four dimensional effective action for tachyon field on a non-BPS D3-brane. We find that consistency with observational data on density perturbation…

High Energy Physics - Theory · Physics 2010-02-17 Atri Deshamukhya , Sudhakar Panda

I review the theory of preheating after inflation, focusing on the recently found tachyonic preheating in the theories with spontaneous symmetry breaking. This occurs due to the tachyonic instability of the scalar field near the top of its…

High Energy Physics - Phenomenology · Physics 2007-05-23 Lev Kofman

Cosmological solutions of the beta function equations for the background fields of the closed bosonic string are investigated at the one-loop level. Following recent work of Kostelecky and Perry, it is assumed that the spatial sections of…

High Energy Physics - Theory · Physics 2010-11-01 Eric Raiten

Closed string tachyon condensation in spacetime generates potentials on the worldsheet that model two-dimensional inflationary cosmology. These models illustrate and elucidate a variety of aspects of inflation, in particular the generation…

High Energy Physics - Theory · Physics 2009-11-10 Bruno Carneiro da Cunha , Emil J. Martinec

It was pointed out that brane-anti-brane inflation without warped geometry is not viable due to compactification effects (in the simplified scenario where the inflaton is decoupled from the compactification moduli). We show that the…

High Energy Physics - Theory · Physics 2009-11-10 Sarah Shandera , Benjamin Shlaer , Horace Stoica , S. -H. Henry Tye

Variation of constants in the very early universe can generate inflation. We consider a scenario where the strong coupling constant was changing in time and where the gluon condensate underwent a phase transition ending the inflation.

Astrophysics · Physics 2008-11-26 N. Chamoun , S. J. Landau , H. Vucetich

Natural (axionic) inflation can accommodate sizeable primordial tensor modes but suffers from the necessity of trans-Planckian variations of the inflaton field. This problem can be solved via the mechanism of aligned axions…

High Energy Physics - Theory · Physics 2014-09-01 Rolf Kappl , Sven Krippendorf , Hans Peter Nilles

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…

High Energy Physics - Theory · Physics 2014-11-18 J. Garcia-Bellido , R. Rabadan , F. Zamora

The inflaton potential in four-dimensional theory is rather arbitrary, and fine-tuning is required generically. By contrast, inflation in the brane world scenario has the interesting feature that the inflaton potential is motivated from…

High Energy Physics - Theory · Physics 2011-05-05 Gary Shiu , S. -H. Henry Tye

We study inflation arising from the motion of a BPS D3-brane in the background of a stack of k parallel D5-branes. There are two scalar fields in this set up-- (i) the radion field R, a real scalar field, and (ii) a complex tachyonic scalar…

High Energy Physics - Theory · Physics 2008-11-26 Sudhakar Panda , M. Sami , Shinji Tsujikawa , John Ward

We investigate multi-field inflationary scenarios with fields that drop out of the model in a staggered fashion. This feature is natural in certain multi-field inflationary setups within string theory; for instance, it can manifest itself…

High Energy Physics - Theory · Physics 2009-12-10 Diana Battefeld , Thorsten Battefeld , Anne-Christine Davis

We consider the brane gas picture of the early universe. At later stages, when there are no winding modes and the background is free to expand, we show that a moving 3-brane, which we identify with our universe, can inflate even though it…

High Energy Physics - Phenomenology · Physics 2009-11-07 M. F. Parry , D. A. Steer

In this paper we study the tachyonic inflation in brane world cosmology with Gauss-Bonnet term in the bulk. We obtain the exact solution of slow roll equations in case of exponential potential. We attempt to implement the proposal of Lidsey…

High Energy Physics - Theory · Physics 2009-11-10 B. C. Paul , M. Sami

We present inflationary models of the early universe in the braneworld scenario considering both scalar field and tachyon field separately. The technique of Chervon and Zhuravlev to obtain inflationary cosmological models without…

High Energy Physics - Theory · Physics 2007-08-08 B. C. Paul , Dilip Paul

We consider the possibility that the universe, viewed as a three-brane, originated in a region of strong external field strength due to a four-form gauge field in the bulk. It is shown that in a scenario of this kind inflation is generic…

High Energy Physics - Theory · Physics 2017-09-20 Jeff Greensite

In this article, our prime objective is to study the inflationary paradigm from generalized tachyon (GTachyon) living on the world volume of a non-BPS string theory. The tachyon action is considered here is getting modified compared to the…

High Energy Physics - Theory · Physics 2016-05-23 Sayantan Choudhury , Sudhakar Panda

We investigate a new way of realizing a period of cosmological inflation in the context of brane gas cosmology. It is argued that a gas of co-dimension one branes, out of thermal equilibrium with the rest of the matter, has an equation of…

High Energy Physics - Theory · Physics 2007-05-23 Robert Brandenberger , Damien A. Easson , Anupam Mazumdar

We present a scenario where brane inflation arises more generically. We start with D3 and anti-D3-branes at the infrared ends of two different throats. This setup is a natural consequence of the assumption that in the beginning we have a…

High Energy Physics - Theory · Physics 2010-04-06 Xingang Chen