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We explore the generic motion of cosmic (super)strings when the internal compact dimensions are warped, using the Klebanov-Strassler solution as a prototypical throat geometry. We find that there is no dynamical mechanism which localises…

High Energy Physics - Theory · Physics 2013-05-30 Anastasios Avgoustidis , Sarah Chadburn , Ruth Gregory

We investigate DBI inflation using $N$ multiple branes and show how the configuration is equivalent to a single wrapped $D5$-brane with flux. We then show how 1/N corrections can be implemented, and we examine the sound speed and levels of…

High Energy Physics - Theory · Physics 2009-05-20 John Ward

We argue for the existence of bounds on the tensions of $p$-branes in de Sitter space in terms of the Hubble rate and the strength of a class of Chern-Simons-like couplings. The world-volume couplings involve Abelian 1-form gauge fields in…

High Energy Physics - Theory · Physics 2025-07-28 Saquib Hassan , Georges Obied , John March-Russell

Inflationary models whose vacuum energy arises from a D-term are believed not to suffer from the supergravity eta problem of F-term inflation. That is, D-term models have the desirable property that the inflaton mass can naturally remain…

High Energy Physics - Theory · Physics 2009-11-11 Liam McAllister

We construct supersymmetric unified models which automatically lead to a period of inflation. The models all involve a U(1) symmetry which does not belong to the MSSM. We consider three different types of models depending on whether this…

High Energy Physics - Phenomenology · Physics 2009-10-30 R. Jeannerot

In this thesis we study the dynamics of higher-dimensional gravity in a universe emerging from a brane collision. We develop a set of powerful analytic methods which, we believe, render braneworld cosmological perturbation theory solvable.…

High Energy Physics - Theory · Physics 2007-05-23 Paul McFadden

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

We consider the cosmological evolution of the three-brane in the background of type IIB string theory. For two different backgrounds which give nontrivial dilaton profile we have derived the Friedman-like equations. These give the…

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

In String theory realizations of inflation, the end point of inflation is often brane-anti brane annihilation. We consider the processes of reheating of the Standard Model universe after brane inflation. We identify the channels of inflaton…

High Energy Physics - Theory · Physics 2014-11-18 Lev Kofman , Piljin Yi

An anti-D3-brane plays a crucial role in the construction of semi-realistic cosmological models in string theory. Part of its action provides an uplift term that has been used to lift AdS solutions to phenomenologically viable dS vacua in…

High Energy Physics - Theory · Physics 2019-09-11 Niccolò Cribiori , Christoph Roupec , Timm Wrase , Yusuke Yamada

By exploiting recent arguments about stable nonsupersymmetric D-brane states, we argue that D-brane charge takes values in the K-theory of spacetime, as has been suspected before. In the process, we gain a new understanding of some novel…

High Energy Physics - Theory · Physics 2010-04-07 Edward Witten

Braneworld inflation on the resolved warped deformed conifold is represented by the dynamics of a D3-brane probe with the world volume of a brane spanning the large dimensions of the observable Universe. This model was recently proposed as…

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

We describe a model of D--brane inflation on fractional D3 branes transverse to a resolved and deformed conifold. The resolution and the deformation are both necessary for inflation. The fractional branes slowly approach each other along…

High Energy Physics - Theory · Physics 2007-05-23 Edi Halyo

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

I summarize recent work on (1) constraining spike-like features in the cosmic microwave background and large scale structure; (2) nonstandard Friedmann equation in stabilized warped 6D brane cosmology, with applications to inflation; and…

Astrophysics · Physics 2008-05-15 James M. Cline

We study the effects of quantum production of open strings on the relativistic scattering of D-branes. We find strong corrections to the brane trajectory from copious production of highly-excited open strings, whose typical oscillator level…

High Energy Physics - Theory · Physics 2008-11-26 Liam McAllister , Indrajit Mitra

We study classical lump solutions in a warped throat where brane inflation takes place. Some of the solitonic or lump solutions that we study here are the (p,q) cosmic strings and their junctions, cosmic necklaces and semi-local strings and…

High Energy Physics - Theory · Physics 2009-11-13 Keshav Dasgupta , Hassan Firouzjahi , Rhiannon Gwyn

Certain inflationary models can feature periods of preheating - an era preceding reheating during which parametric resonance triggers an exponential production of bosons. This non-perturbative process can have significant impact on the…

High Energy Physics - Theory · Physics 2024-12-02 Jacob M. Leedom , Margherita Putti , Nicole Righi , Alexander Westphal

We consider a general brane-world model parametrized by the brane tension scale $f$ and the branon mass $M$. For low tension compared to the fundamental gravitational scale, we calculate the relic branon abundance and its contribution to…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. A. R. Cembranos , A. Dobado , A. L. Maroto

The slow-roll inflation is a beautiful paradigm, yet the inflaton potential can hardly be sufficiently flat when unknown gravitational effects are taken into account. However, the hybrid inflation models constructed in D = 4 N = 1…

High Energy Physics - Theory · Physics 2014-11-18 Fumikazu Koyama , Yuji Tachikawa , Taizan Watari
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