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Related papers: Inflation from D-\bar{D} brane annihilation

200 papers

We present a mechanism for exit from inflation and reheating using the AdS/CFT correspondence. A cosmological evolution is induced on a probe D3-brane as it moves in a black D-brane background of type-0 string theory. If the tachyon field…

High Energy Physics - Theory · Physics 2009-11-10 E. Papantonopoulos , V. Zamarias

Towards the end of brane inflation, the brane pair annihilation produces massive closed strings. The transfer of this energy to Standard Model (SM) open string modes depends on where the SM branes and the brane annihilation are located: in…

High Energy Physics - Theory · Physics 2009-11-11 Xingang Chen , S. -H. Henry Tye

Quintessential inflation--in which a single scalar field plays the role of the inflaton and quintessence--from a sum of exponentials potential V = A (exp{5 phi}+exp{sqrt{2} phi}) or V = A (exp{5 phi}+exp{phi}) or a cosh potential V = 2A…

High Energy Physics - Phenomenology · Physics 2007-05-23 Carl L. Gardner

Inspired by the Randall-Sundrum brane-world scenario, we investigate the possibility of brane-world inflation driven not by an inflaton field on the brane, but by a bulk, dilaton-like gravitational field. As a toy model for the dilaton-like…

General Relativity and Quantum Cosmology · Physics 2009-10-09 Yoshiaki Himemoto , Misao Sasaki

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 analyse the mechanism of quintessential inflation in brane world scenarios for a number of particle physics inspired scalar potentials. We constrain the parameter space of those scalar potentials and comment on the likelihood that we…

Astrophysics · Physics 2009-11-07 N. J. Nunes , E. J. Copeland

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

We examine the possibility of achieving quintessential inflation, where the same field serves as both inflaton and quintessence, in the context of a five-dimensional braneworld. Braneworld cosmology provides an appropriate environment as it…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-22 Mafalda Dias , Andrew R Liddle

We review the recent attempts of unifying inflation with quintessence. It appears natural to join the two ends in the framework of brane world cosmology. The models of quintessential inflation belong to the class of {\it non-oscillatory}…

High Energy Physics - Theory · Physics 2007-05-23 M. Sami , N. Dadhich

We analyze the quantum-corrected moduli space of D7-brane position moduli with special emphasis on inflationary model building. D7-brane deformation moduli are key players in two recently proposed inflationary scenarios: The first, D7-brane…

A quantum-mechanical technique is used within the framework of U(2) super-Yang-Mills theory to investigate processes after recombination of two D-p-branes at one angle. Two types of initial conditions are considered, one of which with $p=4$…

High Energy Physics - Theory · Physics 2007-05-23 Takeshi Sato

We demonstrate an inflationary solution to the cosmological horizon problem during the Hagedorn regime in the early universe. Here the observable universe is confined to three spatial dimensions (a three-brane) embedded in higher…

High Energy Physics - Theory · Physics 2007-05-23 Steven Abel , Katherine Freese , Ian Kogan

We demonstrate an inflationary solution to the cosmological horizon problem during the Hagedorn regime in the early universe. Here the observable universe is confined to three spatial dimensions (a three-brane) embedded in higher…

High Energy Physics - Theory · Physics 2014-11-18 Steven Abel , Katherine Freese , Ian Kogan

We discuss a five dimensional inflationary scenario based on a supersymmetric SO(10) model compactified on $S^1/(Z_2\times Z_2')$. Inflation is implemented through scalar potentials on four dimensional branes, and a brane-localized…

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

In certain implementations of the brane inflationary paradigm, the exit from inflation occurs when the branes annihilate through tachyon condensation. We investigate various cosmological effects produced by this tachyonic era. We find that…

High Energy Physics - Theory · Physics 2010-10-27 Louis Leblond , Sarah Shandera

We present an explicit string realisation of a cosmological inflationary scenario we proposed recently within the framework of type IIB flux compactifications in the presence of three magnetised D7-brane stacks. Inflation takes place around…

High Energy Physics - Theory · Physics 2022-01-19 Ignatios Antoniadis , Osmin Lacombe , George K. Leontaris

In this paper we argue that the mechanism of unwinding inflation is naturally present in warped compactifications of type IIB string theory with local throats. The unwinding of flux is caused by its annihilation against branes. The…

High Energy Physics - Theory · Physics 2016-12-05 Fridrik Freyr Gautason , Marjorie Schillo , Thomas Van Riet

We investigate a new mechanism for realizing slow roll inflation in string theory, based on the dynamics of p anti-D3 branes in a class of mildly warped flux compactifications. Attracted to the bottom of a warped conifold throat, the…

High Energy Physics - Theory · Physics 2009-11-10 Oliver DeWolfe , Shamit Kachru , Herman Verlinde

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

A long period of inflation can be triggered when the inflaton is held up on the top of a steep potential by the infrared end of a warped space. We first study the field theory description of such a model. We then embed it in the flux…

High Energy Physics - Theory · Physics 2009-11-11 Xingang Chen