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Related papers: Trapped Brane Features in DBI Inflation

200 papers

"Brane supersymmetry breaking" occurs in String Theory when the only available combinations of D-branes and orientifolds are not mutually BPS and yet do not introduce tree-level tachyon instabilities. It is characterized by the emergence of…

High Energy Physics - Theory · Physics 2015-06-18 N. Kitazawa , A. Sagnotti

We investigate the embedding of brane inflation into stable compactifications of string theory. At first sight a warped compactification geometry seems to produce a naturally flat inflaton potential, evading one well-known difficulty of…

High Energy Physics - Theory · Physics 2009-09-29 Shamit Kachru , Renata Kallosh , Andrei Linde , Juan Maldacena , Liam McAllister , Sandip P. Trivedi

In brane inflation, the relative brane position in the bulk of a brane world is the inflaton. For branes moving in a compact manifold, the approximate translational (or shift) symmetry is necessary to suppress the inflaton mass, which then…

High Energy Physics - Theory · Physics 2010-12-03 Hassan Firouzjahi , S. -H. Henry Tye

Brane inflation and the production of topological defects at the end of the inflationary phase are discussed. After a description of the inflationary setup we discuss the properties of the cosmic strings produced at the end of inflation.…

High Energy Physics - Theory · Physics 2008-11-26 A. C. Davis , P. Brax , C. van de Bruck

We reanalyze brane inflation with brane-brane interactions at an angle, which include the special case of brane-anti-brane interaction. If nature is described by a stringy realization of the brane world scenario today (with arbitrary…

High Energy Physics - Theory · Physics 2009-11-07 Nicholas Jones , Horace Stoica , S. -H. Henry Tye

We propose a novel inflationary scenario in string theory in which the inflaton field is a 'Wilson line' degree of freedom in the worldvolume of a probe Dp-brane, in a warped flux compactification. Kinetic terms for Wilson line fields on…

High Energy Physics - Theory · Physics 2009-02-09 A. Avgoustidis , I. Zavala

We compute the tree-level connected four-point function of the primordial curvature perturbation for a fairly general minimally coupled single field inflationary model, where the inflaton's Lagrangian is a general function of the scalar…

High Energy Physics - Theory · Physics 2010-04-14 Frederico Arroja , Shuntaro Mizuno , Kazuya Koyama , Takahiro Tanaka

We show that, in constructions with additional intersecting D-branes, brane-antibrane inflation may naturally occur in a warm regime, such that strong dissipative effects damp the inflaton's motion, greatly alleviating the associated…

High Energy Physics - Theory · Physics 2015-05-27 Mar Bastero-Gil , Arjun Berera , Joao G. Rosa

We analyze the spectrum of density perturbations generated in models of the recently discovered "D-cceleration" mechanism of inflation. In this scenario, strong coupling quantum field theoretic effects sum to provide a DBI-like action for…

High Energy Physics - Theory · Physics 2009-11-10 Mohsen Alishahiha , Eva Silverstein , David Tong

An impressed feature of inflation on warped Dvali-Gabadadze-Porrati (DGP) brane is that the inflationary phase exits spontaneously for a scalar inflaton field with exponential potential, which presents a graceful exit mechanism for the…

Astrophysics · Physics 2008-11-26 Hongsheng Zhang , Zong-Hong Zhu

We study inflation and reheating in a brane world model derived from Type IIA string theory. This particular setup is based on a model of string mediated supersymmetry breaking. The inflaton is one of the transverse scalars of a D4-brane…

High Energy Physics - Theory · Physics 2007-05-23 John H. Brodie , Damien A. Easson

Cosmic inflation driven by branes wrapping the extra dimensions involves Kaluza-Klein (KK) degrees of freedom in addition to the zero-mode position of the brane which plays the role of the inflaton. As the wrapped brane passes by localized…

Cosmology and Nongalactic Astrophysics · Physics 2013-09-02 Takeshi Kobayashi , Jun'ichi Yokoyama

We show that brane inflation is very sensitive to tiny sharp features in extra dimensions, including those in the potential and in the warp factor. This can show up as observational signatures in the power spectrum and/or non-Gaussianities…

High Energy Physics - Theory · Physics 2011-03-04 Rachel Bean , Xingang Chen , Girma Hailu , S. -H. Henry Tye , Jiajun Xu

Many existing models of brane inflation suffer from a steep irreducible gravitational potential between the branes that causes inflation to end too early. Inspired by the fact that point masses in 2+1 D exert no gravitational force, we…

High Energy Physics - Theory · Physics 2010-05-12 Jason Gallicchio , Rakhi Mahbubani

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

In canonical scalar field inflation, the Starobinsky model (with a linear potential but discontinuous slope) is remarkable in that though slow-roll is violated, both the power-spectrum and bi-spectrum can be calculated exactly analytically.…

High Energy Physics - Theory · Physics 2015-06-15 Santiago Avila , Jerome Martin , Daniele Steer

We investigate brane inflation, focusing on warm inflation realizations within a warped throat geometry. While the standard scenario relies on a single mobile $D3$-brane moving radially toward an anti-$D3$-brane at the tip of the throat, we…

High Energy Physics - Theory · Physics 2026-04-01 Dibya Chakraborty , Rudnei O. Ramos

We propose a geometrical model of brane inflation where inflation is driven by the flux generated by opposing brane charges and terminated by the collision of the branes, with charge annihilation. We assume the collision process is…

High Energy Physics - Theory · Physics 2009-11-11 Sugumi Kanno , Jiro Soda , David Wands

At energies higher than the brane tension, the dynamics of a scalar field rolling down a potential are modified relative to the predictions of General Relativity. The modifications imply, among other things, that steeper potentials can be…

Astrophysics · Physics 2009-11-07 P. R. Ashcroft , C. van de Bruck , A. -C. Davis

Dirac-Born-Infeld scalar field theories which appear in the context of inflation in string theory in general have a field dependent speed of sound. It is however possible to write down DBI models which possess exact solutions characterized…

Astrophysics · Physics 2009-06-23 Michal Spalinski