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Related papers: Multi-Throat Brane Inflation

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Non-supersymmetric brane world scenarios in string theory display perturbative instabilities that usually involve run-away potentials for scalar moduli fields. We investigate in the framework of intersecting brane worlds whether the leading…

High Energy Physics - Theory · Physics 2009-10-07 Ralph Blumenhagen , Boris Kors , Dieter Lust , Tassilo Ott

The brane inflationary model inspired by a polytropic inflationary idea is studied. In the slow-roll approximation and high energy limit, for a chaotic potential, the model is developed, and its characteristics are discussed. We obtain…

General Relativity and Quantum Cosmology · Physics 2018-04-18 Mohammad Reza Setare , Arvin Ravanpak , Hossein Farajollahi

D3-branes feel no force in no-scale flux compactifications of type IIB string theory, but the nonperturbative effects required to stabilize the Kahler moduli break the no-scale structure and generate a potential for D3-brane motion,…

High Energy Physics - Theory · Physics 2008-11-26 Oliver DeWolfe , Liam McAllister , Gary Shiu , Bret Underwood

We investigate in the context of brane inflation the possibility of additional light scalar fields generating significant power spectrum and non-Gaussianities at the end of inflation affecting the CMB scale observations. We consider the…

High Energy Physics - Theory · Physics 2008-11-26 Heng-Yu Chen , Jinn-Ouk Gong , Gary Shiu

We describe type $II_A$ cosmological brane inflation scenarios based on the holographic MQCD model of Aharony et al \cite{Aharony:2010mi}. The scenarios can be related via T-duality to the type $II_B$ KKLMMT model \cite{Kachru:2003sx}. They…

High Energy Physics - Theory · Physics 2015-05-30 Horatiu Nastase , Jacob Sonnenschein

In brane world scenarios inflationary vacuum energy may escape into the higher dimensional bulk leaving behind a dark radiation effect on the brane. The paper analyses the damping of an inflaton by massless bulk scalar radiation and the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Cheng-Ji Chang , I. G. Moss

In this paper we obtain a model of Natural Inflation from string theory with a Planckian decay constant. We investigate D-brane dynamics in the background of the warped resolved conifold (WRC) throat approximation of Type IIB string…

High Energy Physics - Theory · Physics 2015-03-02 Zachary Kenton , Steven Thomas

A characteristic of D-brane inflation is that fluctuations in the inflaton field can propagate at a speed significantly less than the speed of light. This yields observable effects that are distinct from those of single-field slow roll…

Astrophysics · Physics 2008-11-26 Hiranya V. Peiris , Daniel Baumann , Brett Friedman , Asantha Cooray

In this paper, warm inflationary models on a brane scenario are studied. Here we consider slow-roll inflation and high-dissipation regime in a high-energy scenario. General conditions required for these models to be realizable are derived.…

Astrophysics · Physics 2008-11-26 M. Antonella Cid , Sergio del Campo , Ramon Herrera

We study multifield aspects of Dirac-Born-Infeld (DBI) inflation. More specifically, we consider an inflationary phase driven by the radial motion of a D-brane in a conical throat and determine how the D-brane fluctuations in the angular…

High Energy Physics - Theory · Physics 2014-11-20 Sébastien Renaux-Petel

The inflationary models developed in presence of a background radiation can be a solution to the reheating problem faced by common cold (isentropic) inflationary scenario. A D-brane system comprising of k Neuvo-Schwarz(NS) 5-branes with a…

Cosmology and Nongalactic Astrophysics · Physics 2014-02-28 Anindita Bhattacharjee , Atri Deshamukhya

Generic heterotic M-theory compactifications contain five-branes wrapping non-isolated genus zero or higher genus curves in a Calabi-Yau threefold. Non-perturbative superpotentials do not depend on moduli of such five-branes.We show that…

High Energy Physics - Theory · Physics 2010-12-03 Evgeny I. Buchbinder

We consider a probe codimension-2 brane inflation scenario in a warped six-dimensional flux compactification. Our background model is Salam-Sezgin gauged supergravity with codimension-2 brane sources, which preserve N=1 supersymmetry. The…

High Energy Physics - Theory · Physics 2009-09-02 Hyun Min Lee , Antonios Papazoglou

We analyze observational constraints on the parameter space of tachyonic inflation with a Gaussian potential and discuss some predictions of this scenario. As was shown by Kofman and Linde, it is extremely problematic to achieve the…

High Energy Physics - Theory · Physics 2008-11-26 Joris Raeymaekers

We reconsider a string theoretic inflationary model, where inflation is driven by $n$ multiple coincident $D3$-branes in the finite $n$ limit. We show that the finite $n$ action can be continued to the limit of large $n$, where it converges…

High Energy Physics - Theory · Physics 2010-01-22 Aaron Berndsen , James. E. Lidsey , John Ward

Inflationary models in string theory which identify the inflaton with an open string modulus lead to effective field theories with non-canonical kinetic terms: Dirac-Born-Infeld scalar field theories. In the case of a $D$-brane moving in an…

High Energy Physics - Theory · Physics 2009-11-13 Michal Spalinski

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 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

We discuss a brane based inflationary scenario in which an initially non-supersymmetric configuration involving a D4 brane is dynamically transformed into a supersymmteric one in a background space-time geometry determined by a stack of D6…

High Energy Physics - Phenomenology · Physics 2011-05-12 Bumseok Kyae , Qaisar Shafi

We study the cosmological evolution of a D3-brane universe in a type 0 string background. We follow the brane-universe along the radial coordinate of the background and we calculate the energy density which is induced on the brane because…

High Energy Physics - Theory · Physics 2007-05-23 E. Papantonopoulos
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