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Related papers: Inflation on the resolved warped deformed conifold

200 papers

The inflationary scenario for the brane world driven by the bulk inflaton is proposed. The quantum fluctuations of the inflaton is calculated and compared to those of the conventional 4-dimensional inflationary scenario. It is shown that…

High Energy Physics - Theory · Physics 2009-10-31 Shinpei Kobayashi , Kazuya Koyama , Jiro Soda

We study the motion of a (space filling) D3-brane at the tip of a warped deformed conifold, looking for inflationary trajectories. In our setup no anti D3-brane is present and the inflaton potential is induced by threshold corrections to…

High Energy Physics - Theory · Physics 2014-11-18 Enrico Pajer

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 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 2009-10-31 E. Papantonopoulos , I. Pappa

We propose a stringy version of the old inflation scenario which does not require any slow-roll inflaton potential and is based on a specific example of string compatification with warped metric. Our set-up admits the presence of…

High Energy Physics - Theory · Physics 2009-11-10 L. Pilo , A. Riotto , A. Zaffaroni

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 I. Pappa

Using DBI inflation as an example, we demonstrate that the detailed geometry of warped compactification can leave an imprint on the cosmic microwave background (CMB). We compute CMB observables for DBI inflation in a generic class of warped…

High Energy Physics - Theory · Physics 2008-11-26 Gary Shiu , Bret Underwood

In a recent paper we showed how Starobinsky-like inflation could emerge from dilaton dynamics in brane cosmology scenarios based on string theory, in which our universe is represented as a three-brane and the effective potential acquires a…

High Energy Physics - Theory · Physics 2015-06-19 John Ellis , Nick E. Mavromatos , Dimitri V. Nanopoulos

Brane inflation is a specific realization of the inflationary universe scenario in the early universe within the brane world framework in string theory. The naturalness and robustness of this realistic scenario is explained. Its predictions…

High Energy Physics - Theory · Physics 2008-11-26 S. -H. Henry Tye

We present a curvaton model from type IIB string theory compactified on a warped throat with approximate isometries. Considering an (anti-)D3-brane sitting at the throat tip as a prototype standard model brane, we show that the brane's…

High Energy Physics - Theory · Physics 2009-07-21 Takeshi Kobayashi , Shinji Mukohyama

We derive constraints on the tensor to scalar ratio and on the background charge of the warped throat for DBI inflation driven by D5- and D7-branes wrapped over cycles of the throat. It is shown that the background charge well beyond the…

High Energy Physics - Theory · Physics 2009-11-18 Takeshi Kobayashi , Shinji Mukohyama , Shunichiro Kinoshita

We construct a model of inflation in string theory after carefully taking into account moduli stabilization. The setting is a warped compactification of Type IIB string theory in the presence of D3 and anti-D3-branes. The inflaton is the…

High Energy Physics - Theory · Physics 2014-11-18 Norihiro Iizuka , Sandip P. Trivedi

In a simple reanalysis of the KKLMMT scenario, we argue that the slow roll condition in the D3-anti-D3-brane inflationary scenario in superstring theory requires no more than a moderate tuning. The cosmic string tension is very sensitive to…

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

In Randall-Sundrum type braneworld cosmologies, the dynamical equations on the three-brane differ from the general relativity equations by terms that carry the effects of embedding and of the free gravitational field in the five-dimensional…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Deon Solomons , Peter Dunsby , George Ellis

Brane and warped Dvali-Gabadadze-Porrati inflationary universe models in the context of intermediate inflation are studied. In both models we consider that the energy density is a standard scalar field and we discuss the evolution of the…

General Relativity and Quantum Cosmology · Physics 2015-06-17 Ramon Herrera , Marco Olivares , Nelson Videla

We study D-brane inflation in a warped conifold background that includes brane-position dependent corrections for the nonperturbative superpotential. Instead of stabilizing the volume modulus chi at instantaneous minima of the potential and…

High Energy Physics - Theory · Physics 2009-09-29 Sudhakar Panda , M. Sami , Shinji Tsujikawa

We review a viable alternative scenario of the inflationary universe in the context of the Randall-Sundrum (RS) braneworld. In this scenario, the dynamics of a 5-dimensional scalar field, which we call a bulk scalar field, plays the central…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Yoshiaki Himemoto , Misao Sasaki

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

We demonstrate that a gas of wrapped branes in the early Universe can help resolve the cosmological Dine-Seiberg/Brustein-Steinhardt overshoot problem in the context of moduli stabilization with steep potentials in string theory. Starting…

High Energy Physics - Theory · Physics 2009-11-11 Damien A. Easson , Mark Trodden