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Related papers: Primordial Spikes from Wrapped Brane Inflation

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We investigate a new way of realizing a period of cosmological inflation in the context of brane gas cosmology. It is argued that a gas of co-dimension one branes, out of thermal equilibrium with the rest of the matter, has an equation of…

High Energy Physics - Theory · Physics 2007-05-23 Robert Brandenberger , Damien A. Easson , Anupam Mazumdar

The scalar mode describing the fluctuation of the 3-brane (the observable universe) in a five-dimensional bulk spacetime compactified on a circle is absorbed by the Kaluza-Klein U(1) gauge field, leading to a massive brane-vector living on…

High Energy Physics - Phenomenology · Physics 2024-08-01 Cao H. Nam , Tran N. Hung

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

We present a novel inflationary scenario in theories with low scale (TeV) quantum gravity, in which the standard model particles are localized on the branes whereas gravity propagates in the bulk of large extra dimensions. This inflationary…

High Energy Physics - Phenomenology · Physics 2009-10-31 Gia Dvali , S. -H. Henry Tye

We study the quantum-mechanical generation of gravitational waves during inflation on a brane embedded in a five-dimensional anti-de Sitter bulk. To make the problem well-posed, we consider the setup in which both initial and final phases…

High Energy Physics - Theory · Physics 2009-11-11 Tsutomu Kobayashi , Takahiro Tanaka

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

We discuss the evolution of gravitational waves in a brane-world cosmology embedded in five-dimensional anti-de Sitter spacetime. We show that during slow-roll inflation, modelled as a period of quasi-de Sitter expansion on the brane, there…

High Energy Physics - Theory · Physics 2009-10-31 David Langlois , Roy Maartens , David Wands

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

We describe type $II_A$ cosmological brane inflation scenarios based on the holographic MQCD model of Aharony et al \cite{Aharony:2010mi}. The scenarios can be related via T-duality to the type $II_B$ KKLMMT model \cite{Kachru:2003sx}. They…

High Energy Physics - Theory · Physics 2015-05-30 Horatiu Nastase , Jacob Sonnenschein

D-branes are fundamental in all scenarios where there are large extra dimensions and the string scale is much smaller than the four-dimensional Planck mass. We show that this current picture leads to a new approach to string cosmology where…

High Energy Physics - Phenomenology · Physics 2009-10-31 Antonio Riotto

In cascade inflation and some other string inflation models, collisions of mobile branes with other branes or orbifold planes occur and lead to interesting cosmological signatures. The fundamental M/string-theory description of these…

High Energy Physics - Theory · Physics 2009-02-16 Amjad Ashoorioon , Axel Krause , Krzysztof Turzynski

In this paper we quantise scalar perturbations in a Randall-Sundrum-type model of inflation where the inflaton field is confined to a single brane embedded in five-dimensional anti-de Sitter space-time. In the high energy regime,…

High Energy Physics - Theory · Physics 2010-10-27 Kazuya Koyama , Andrew Mennim , V. A. Rubakov , David Wands , Takashi Hiramatsu

We describe a D--brane inflation model which consists of two fractional D3 branes separated on a transverse $T^2 \times K3$. Inflation arises due to the resolved orbifold singularity of $K3$ which corresponds to an anomalous D--term on the…

High Energy Physics - Theory · Physics 2009-11-10 Edi Halyo

In the inflationary universe, there can be light fields other than the inflaton. We explore a possibility that such light fields source the primordial perturbations, while minimally affecting the inflaton dynamics. We show that during…

Cosmology and Nongalactic Astrophysics · Physics 2010-05-19 Takeshi Kobayashi , Shinji Mukohyama

We show that the use of higher dimensional wrapped branes can significantly extend the inflaton field range compared to brane inflation models which use D3-branes. We construct a simple inflationary model in terms of 5-branes wrapping a…

High Energy Physics - Theory · Physics 2008-11-26 Melanie Becker , Louis Leblond , Sarah Shandera

We study possible effects of Lorentz-violation on the generation of cosmological perturbations at inflation by introducing a simple inflating five-dimensional brane-world setup with violation of four-dimensional Lorentz-invariance at an…

Astrophysics · Physics 2016-08-30 M. V. Libanov , V. A. Rubakov

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 discuss the effect of Kaluza-Klein (KK) modes of bulk metric perturbations on the second Randall-Sundrum (RS II) type brane cosmology, taking the possible backreaction in the bulk and on the brane into account. KK gravitons may be…

General Relativity and Quantum Cosmology · Physics 2009-10-09 Masato Minamitsuji , Misao Sasaki , David Langlois

Cosmological perturbations, originating in the quantum fluctuations of the fields that drive inflation, are observed to be nearly scale invariant at the largest scales. At smaller scales, however, perturbations are not severely constrained…

Cosmology and Nongalactic Astrophysics · Physics 2024-07-09 Ioannis Dalianis

String theory gives rise to various mechanisms to generate primordial inflation, of which ``brane inflation'' is one of the most widely considered. In this scenario, inflation takes place while two branes are approaching each other, and the…

High Energy Physics - Theory · Physics 2009-11-10 R. Brandenberger , G. Geshnizjani , S. Watson