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Related papers: D3/D7 Inflation in a Type-0B String Background

200 papers

In this thesis, consisting of two main parts, we study observational signatures of cosmic (super)strings in the context of D-brane inflation and properties of scalar perturbations on generic homogeneous inflating backgrounds. In the first…

High Energy Physics - Theory · Physics 2014-06-05 Spyros Sypsas

In this lecture I will review the present status of 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…

Astrophysics · Physics 2007-05-23 Juan Garcia-Bellido

Fluxbrane inflation is a stringy version of D-term inflation in which two fluxed D7-branes move towards each other until their (relative) gauge flux annihilates. Compared to brane-antibrane inflation, the leading-order inflationary…

High Energy Physics - Theory · Physics 2013-01-25 Arthur Hebecker , Sebastian C. Kraus , Moritz Kuntzler , Dieter Lust , Timo Weigand

We find a general model of {\em single-field} inflation within the context of type IIB string theory compactified on large volume Calabi-Yau orientifolds with $h^{2,1} > h^{1,1} = 2$. The inflaton is the axion part of the complexified…

High Energy Physics - Theory · Physics 2007-05-23 R. Holman , Jimmy A. Hutasoit

We show how the motion through the extra dimensions of a gas of branes and antibranes can, under certain circumstances, produce an era of inflation as seen by observers trapped on a 3-brane, with the inflaton being the inter-brane…

High Energy Physics - Theory · Physics 2010-02-03 C. P. Burgess , M. Majumdar , D. Nolte , F. Quevedo , G. Rajesh , R. -J. Zhang

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

We investigate whether explicit models of warped D-brane inflation are possible in string compactifications. To this end, we study the potential for D3-brane motion in a warped conifold that includes holomorphically-embedded D7-branes…

High Energy Physics - Theory · Physics 2008-11-26 Daniel Baumann , Anatoly Dymarsky , Igor R. Klebanov , Liam McAllister , Paul J. Steinhardt

We consider non-BPS D8 (and D7) branes in type 0 open string theory and describe under which circumstances these branes are stable. We find stable non-BPS D7 and D8 in type 0 with and without D9-branes in the background. By extending the…

High Energy Physics - Theory · Physics 2009-10-31 Eduardo Eyras

We find successful models of D-brane/anti-brane inflation within a string context. We work within the GKP-KKLT class of type IIB string vacua for which many moduli are stabilized through fluxes, as recently modified to include `realistic'…

High Energy Physics - Theory · Physics 2008-11-26 C. P. Burgess , J. M. Cline , H. Stoica , F. Quevedo

Inflationary models driven by a large number of axion fields are discussed in the context of type IIB compactifications with N=1 supersymmetry. The inflatons arise as the scalar modes of the R-R two-forms evaluated on vanishing two-cycles…

High Energy Physics - Theory · Physics 2008-06-13 Thomas W. Grimm

We present a general set-up for inflation in string theory where the inflaton field corresponds to Wilson lines in compact space in the presence of magnetic fluxes. T-dualities and limits on the value of the magnetic fluxes relate this…

High Energy Physics - Theory · Physics 2008-11-26 A. Avgoustidis , D. Cremades , F. Quevedo

We investigate the possibility of embedding the vector curvaton paradigm in D-brane models of inflation in Type IIB string theory in a simple toy model. The vector curvaton is identified with the U(1) gauge field that lives on the world…

High Energy Physics - Theory · Physics 2015-05-30 Konstantinos Dimopoulos , Danielle Wills , Ivonne Zavala

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

Closed string tachyon condensation in spacetime generates potentials on the worldsheet that model two-dimensional inflationary cosmology. These models illustrate and elucidate a variety of aspects of inflation, in particular the generation…

High Energy Physics - Theory · Physics 2009-11-10 Bruno Carneiro da Cunha , Emil J. Martinec

We consider a three-dimensional brane-universe moving in a Type 0 String background. The motion induces on the brane a cosmological evolution which, for some range of the parameters, exhibits an inflationary phase.

High Energy Physics - Theory · Physics 2009-10-31 E. Papantonopoulos , I. Pappa

We discuss various realizations of the four dimensional braneworld inflation in warped geometries of string theory. In all models the inflaton field is represented by a Dp probe brane scalar specifying its position in the warped throat of…

High Energy Physics - Theory · Physics 2009-11-10 Alex Buchel , Ahmad Ghodsi

We study possible string theory compactifications which, in the low-energy limit, describe chaotic inflation with a stabilizer field. We first analyze type IIA setups where the inflationary potential arises from a D6-brane wrapping an…

High Energy Physics - Theory · Physics 2016-10-12 Aitor Landete , Fernando Marchesano , Clemens Wieck

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

We consider the motion of the brane universe moving in a background bulk space of tachyonic and non-tachyonic type 0B string theory. The effective densities are calculated for both cases and they show different power law behavior. Brane…

High Energy Physics - Theory · Physics 2009-10-31 Jin Young Kim