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Related papers: Extended Inflation from Strings

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We propose that under certain conditions the universal open string tachyon can drive topological inflation in moduli stabilised frameworks. Namely, the presence of electric field in the world volume of the D-brane can slow down its decay…

High Energy Physics - Theory · Physics 2009-11-11 Daniel Cremades

We consider a cosmological scenario within the KKLT framework for moduli stabilization in string theory. The universal open string tachyon of decaying non-BPS D-brane configurations is proposed to drive eternal topological inflation.…

High Energy Physics - Theory · Physics 2009-11-11 Daniel Cremades , Fernando Quevedo , Aninda Sinha

We show that the naive application of the Kibble mechanism seriously underestimates the initial density of cosmic superstrings that can be formed during the annihilation of D-branes in the early universe, as in models of brane-antibrane…

High Energy Physics - Theory · Physics 2009-11-10 Neil Barnaby , Aaron Berndsen , James M. Cline , Horace Stoica

We use a new mechanism for generating a Fayet-Iliopoulos term in supergravity, which is not associated to an R symmetry, to construct a semi-realistic theory of slow-roll inflation for a theory with the same K\"ahler potential and…

High Energy Physics - Theory · Physics 2021-05-14 Hun Jang , Massimo Porrati

We propose new large field inflation scenarios built on the framework of F-term axion monodromy. Our setup is based on string compactifications where D-branes create potentials for closed string axions via F-terms. Because the source of the…

High Energy Physics - Theory · Physics 2016-04-13 Dagoberto Escobar , Aitor Landete , Fernando Marchesano , Diego Regalado

The string $\alpha^\prime$-correction to the usual Einstein action comprises a Gauss-Bonnet integrand multiplied by non-trivial functions of the modulus field $\chi$ and/or the dilaton field $\phi$. We discuss how the presence of such terms…

High Energy Physics - Theory · Physics 2007-05-23 Ishwaree P Neupane

In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the vacuum fluctuations of the inflaton field corresponding to the position of the brane. We show that a significant, and possibly dominant,…

Astrophysics · Physics 2009-11-11 D. H. Lyth , A. Riotto

We study the conditions for successful Affleck-Dine baryogenesis in generic inflation and supergravity scenarios, finding powerful restrictions on them. String-based SUGRA models are especially interesting since they are surprisingly…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. A. Casas

In this paper we consider inflation as a probe of new physics near the string or Planck scale. We discuss how new physics can be captured by the choice of vacuum, and how this leads to modifications of the primordial spectrum as well as the…

High Energy Physics - Theory · Physics 2009-11-11 Ulf H. Danielsson

The recent progress in embedding inflation in string theory has made it clear that the problem of moduli stabilization cannot be ignored in this context. In many models a special role is played by the volume modulus, which is modified in…

High Energy Physics - Theory · Physics 2009-11-10 Marcus Berg , Michael Haack , Boris Kors

A first order inflation model where a gauge coupling constant runs as the universe inflates is investigated. This model can solve the graceful-exit problem within Einstein gravity by varying the bubble formation rate. The sufficient…

High Energy Physics - Phenomenology · Physics 2008-02-03 Jae-weon Lee , In-guy Koh

Natural inflation relies on the existence of an axion decay constant which is super-Planckian. In string theory only sub-Planckian axion decay constants have been found in any controlled regime. However in field theory it is possible to…

High Energy Physics - Theory · Physics 2015-08-10 Eran Palti

A consistent theory of supersymmetry breaking must have a hidden sector, an observable sector, and must be embedded in a locally supersymmetric theory which arises from string theory. For phenomenological reasons it must also transmit…

High Energy Physics - Theory · Physics 2009-03-27 S. P. de Alwis

Motivated by the string landscape we examine scenarios for which inflation is a two-step process, with a comparatively short inflationary epoch near the string scale and a longer period at a much lower energy (like the TeV scale). We…

High Energy Physics - Theory · Physics 2009-11-11 C. P. Burgess , Richard Easther , Anupam Mazumdar , David F. Mota , Tuomas Multamaki

We embed the supersymmetric standard model of hybrid inflation based on the next-to-minimal superpotential term $\lambda NH_uH_d$ supplemented by an inflaton term $\kappa \phi N^2$, into an extra-dimensional framework, in which all the…

High Energy Physics - Phenomenology · Physics 2009-11-07 M. Bastero-Gil , V. Di Clemente , S. F. King

We analyze a distinctive mechanism for inflation in which particle production slows down a scalar field on a steep potential, and show how it descends from angular moduli in string compactifications. The analysis of density perturbations --…

High Energy Physics - Theory · Physics 2009-11-06 Daniel Green , Bart Horn , Leonardo Senatore , Eva Silverstein

A gravity-driven inflation is shown to arise from a simple higher dimensional universe. In vacuum, the shear of $n>1$ contracting dimensions is able to inflate the remaining three spatial dimensions. Said another way, the expansion of the…

General Relativity and Quantum Cosmology · Physics 2009-10-22 Janna Levin

In the context of supersymmetric models, we analyze the production of topological defects at the end of inflation driven by a conjugate pair of inflaton fields which are non-singlets under the continuous symmetry group of the theory. We…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides , Q. Shafi

We present a new model of large field inflation along a winding trajectory in the field space of two axionic fields, where the 'axions' originate from the complex structure moduli sector of a Calabi-Yau 3-fold at large complex structure.…

High Energy Physics - Theory · Physics 2015-08-05 Arthur Hebecker , Patrick Mangat , Fabrizio Rompineve , Lukas T. Witkowski

We adopt methods from statistical field theory to stochastic inflation. For the example of a free test field in de Sitter and power-law inflation, the power spectrum of long-wavelength fluctuations is computed. We study its dependence on…

General Relativity and Quantum Cosmology · Physics 2011-02-01 Florian Kuhnel , Dominik J. Schwarz