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Related papers: Heating in Brane Inflation and Hidden Dark Matter

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An inflating brane-world can be created from ``nothing'' together with its Anti-de Sitter (AdS) bulk. The resulting space-time has compact spatial sections bounded by the brane. During inflation, the continuum of KK modes is separated from…

High Energy Physics - Theory · Physics 2009-10-09 Jaume Garriga , Misao Sasaki

We propose an alternative inflationary universe scenario in the context of Randall-Sundrum braneworld cosmology. In this new scenario the existence of extra-dimension(s) plays an essential role. First, the brane universe is initially in the…

High Energy Physics - Theory · Physics 2009-11-07 Uchida Gen , Akihiro Ishibashi , Takahiro Tanaka

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

The presence of Kaluza-Klein particles in the universe is a potential manifestation of string theory cosmology. In general, they can be present in the high temperature bath of the early universe. In particular examples, string theory…

High Energy Physics - Theory · Physics 2008-12-18 J. F. Dufaux , L. Kofman , M. Peloso

Our understanding of the state of the universe between the end of inflation and big bang nucleosynthesis (BBN) is incomplete. The dynamics at the end of inflation are rich and a potential source of observational signatures. Reheating, the…

High Energy Physics - Phenomenology · Physics 2015-01-16 Mustafa A. Amin , Mark P. Hertzberg , David I. Kaiser , Johanna Karouby

Generic heterotic M-theory compactifications contain five-branes wrapping non-isolated genus zero or higher genus curves in a Calabi-Yau threefold. Non-perturbative superpotentials do not depend on moduli of such five-branes.We show that…

High Energy Physics - Theory · Physics 2010-12-03 Evgeny I. Buchbinder

We propose a warm inflationary model in the context of relativistic D-brane inflation in a warped throat, which has Dirac-Born-Infeld (DBI) kinetic term and is coupled to radiation through a dissipation term. The perturbation freezes at the…

High Energy Physics - Theory · Physics 2011-05-23 Yi-Fu Cai , James B. Dent , Damien A. Easson

We construct a new brane-world model composed of a bulk -with a dilatonic field-, plus a brane -with brane tension coupled to the dilaton-, cold dark matter and an induced gravity term. It is possible to show that depending on the nature of…

High Energy Physics - Theory · Physics 2011-02-07 Mariam Bouhmadi-Lopez , Antonio Ferrera

We consider field-theoretic models of a warped extra dimension with multiple throats, in which fermions that are singlets of the Standard Model gauge group propagate in a separate throat from the Standard Model fields, which we call the…

High Energy Physics - Phenomenology · Physics 2009-12-16 Ben Gripaios

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 supersymmetry breaking" occurs in String Theory when the only available combinations of D-branes and orientifolds are not mutually BPS and yet do not introduce tree-level tachyon instabilities. It is characterized by the emergence of…

High Energy Physics - Theory · Physics 2015-06-18 N. Kitazawa , A. Sagnotti

We find a description of hybrid inflation in (3+1)-dimensions using brane dynamics of Hanany-Witten type. P-term inflation/acceleration of the universe with the hybrid potential has a slow-roll de Sitter stage and a waterfall stage which…

High Energy Physics - Theory · Physics 2010-02-03 Carlos Herdeiro , Shinji Hirano , Renata Kallosh

Following a previous work [Gen. Relativ. Gravit. 43 (2011)], we further study the behavior of a real scalar field in a hidden brane in a configuration of two branes embedded in a five dimensional bulk. We find an expression for the equation…

General Relativity and Quantum Cosmology · Physics 2012-09-18 Miguel A. García-Aspeitia , Juan Magaña , Tonatiuh Matos

We show that brane inflation is very sensitive to tiny sharp features in extra dimensions, including those in the potential and in the warp factor. This can show up as observational signatures in the power spectrum and/or non-Gaussianities…

High Energy Physics - Theory · Physics 2011-03-04 Rachel Bean , Xingang Chen , Girma Hailu , S. -H. Henry Tye , Jiajun Xu

We study in detail the recently proposed mechanism of generating superheavy Dark Matter with the mass larger than the Hubble rate at the end of inflation. A real scalar field constituting Dark Matter linearly couples to the inflaton. As a…

High Energy Physics - Phenomenology · Physics 2019-06-04 Eugeny Babichev , Dmitry Gorbunov , Sabir Ramazanov

We review recent progress in string model building in both early and late time cosmology. We describe the main theoretical and phenomenological features of an entire class of inflationary models where inflation is driven by a type IIB…

High Energy Physics - Theory · Physics 2026-04-20 Michele Cicoli

The brane cosmology has invoked new challenges to the usual Big Bang cosmology. In this paper we present a brief account on thermal history of the post-inflationary brane cosmology. We have realized that it is not obvious that the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Anupam Mazumdar

Reheating in string compactifications is generically driven by the decay of the lightest modulus which produces Standard Model particles, dark matter and light hidden sector degrees of freedom that behave as dark radiation. This common…

High Energy Physics - Phenomenology · Physics 2015-06-18 Rouzbeh Allahverdi , Michele Cicoli , Bhaskar Dutta , Kuver Sinha

It was recently pointed out that the fundamental Planck mass could be close to the TeV scale with the observed weakness of gravity at long distances being due the existence of new sub-millimeter spatial dimensions. In this picture the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Nima Arkani-Hamed , Savas Dimopoulos , Nemanja Kaloper , John March-Russell

If cosmic inflation was driven by an electrically neutral scalar field stable on cosmological time scales, the field necessarily constitutes all or part of dark matter (DM). We study this possibility in a scenario where the inflaton field…

High Energy Physics - Phenomenology · Physics 2019-03-13 Juan P. Beltrán Almeida , Nicolás Bernal , Javier Rubio , Tommi Tenkanen