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Related papers: Heating in Brane Inflation and Hidden Dark Matter

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Protecting the inflationary potential from quantum corrections typically requires symmetries that constrain the form of couplings of the inflaton to other sectors. We will explore how these restrictions affect reheating in models with UV…

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

We present a model where the inflaton field behaves like quintessence at late times, generating the present phase of accelerated expansion. This is achieved within the framework of warm inflation, in particular the Warm Little Inflaton…

High Energy Physics - Phenomenology · Physics 2019-10-23 João G. Rosa , Luís B. Ventura

It has very recently been realized that coupling branes to higher dimensional quantum gravity theories and considering the consistency of what lives on the branes, one is able to understand whether such theories can belong either to the…

General Relativity and Quantum Cosmology · Physics 2020-02-05 Vahid Kamali , Meysam Motaharfar , Rudnei O. Ramos

We study brane-world preheating in massive chaotic inflationary scenario where scalar fields are confined on the 3-brane. Assuming that quadratic contribution in energy densities dominates the Hubble expansion rate during preheating, the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Shinji Tsujikawa , Kei-ichi Maeda , Shuntaro Mizuno

We propose a model of inflation in the framework of brane cosmology driven by background supergravity. Starting from bulk supergravity we construct the inflaton potential on the brane and employ it to investigate for the consequences to…

High Energy Physics - Theory · Physics 2012-12-21 Sayantan Choudhury , Supratik Pal

Recent models of axion monodromy inflation in string theory link the inflationary potential and the moduli stabilization potential. Realistic inflationary models require mechanisms to moderately suppress the inflaton mass with respect to…

High Energy Physics - Theory · Physics 2015-06-19 Sebastian Franco , Daniele Galloni , Ander Retolaza , Angel Uranga

We investigate the scalar metric perturbations about a de Sitter brane universe in a 5-dimensional anti de Sitter bulk. We compare the master-variable formalism, describing metric perturbations in a 5-dimensional longitudinal gauge, with…

High Energy Physics - Theory · Physics 2009-11-10 K. Koyama , D. Langlois , R. Maartens , D. Wands

We obtain cosmological constraints on models of inflation which exhibit rapid roll solutions. Rapid roll attractors exist for potentials with large mass terms and are thus of interest for inflationary model building within string theory. We…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-15 Takeshi Kobayashi , Shinji Mukohyama , Brian A. Powell

Despite their consequential applications, metastable states of antibranes in warped throats are not yet fully understood. In this thesis, we provide new information on various aspects of these metastable antibranes through applications of…

High Energy Physics - Theory · Physics 2021-06-29 Nam Nguyen

In this paper, warm inflationary models on a brane scenario are studied. Here we consider slow-roll inflation and high-dissipation regime in a high-energy scenario. General conditions required for these models to be realizable are derived.…

Astrophysics · Physics 2008-11-26 M. Antonella Cid , Sergio del Campo , Ramon Herrera

Heavy long-lived particles are abundant in BSM physics and will, under generic circumstances, get to dominate the energy density of the universe. The resulting matter dominated era has to end before the onset of Big Bang Nucleosynthesis…

High Energy Physics - Phenomenology · Physics 2022-05-17 Manuel Drees , Bardia Najjari

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

In this paper, $k$-inflation is analyzed in warm braneworld scenario. A general class of $k$-essence models with power-law kinetic term is investigated and weak and strong dissipation regimes are studied. Scalar perturbations and spectral…

General Relativity and Quantum Cosmology · Physics 2017-05-16 Lorenzo Sebastiani , Ratbay Myrzakulov

The primordial inflation dilutes all matter except the quantum fluctuations which we see in the cosmic microwave background (CMB) radiation. Therefore the last phases of inflation must be embedded within a beyond the Standard Model (SM)…

High Energy Physics - Phenomenology · Physics 2013-02-06 Celine Boehm , Jonathan Da Silva , Anupam Mazumdar , Ernestas Pukartas

We investigate the embedding of brane anti-brane inflation into a concrete type IIB string theory compactification with all moduli fixed. Specifically, we are considering a D3-brane, whose position represents the inflaton $\phi$, in a…

High Energy Physics - Theory · Physics 2009-04-17 Axel Krause , Enrico Pajer

Higher-form flux that extends in all 3+1 dimensions of spacetime is a source of positive vacuum energy that can drive meta-stable eternal inflation. If the flux also threads compact extra dimensions, the spontaneous nucleation of a bubble…

High Energy Physics - Theory · Physics 2015-06-12 Guido D'Amico , Roberto Gobbetti , Matthew Kleban , Marjorie Schillo

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 revisit the energy transfer necessary for the warped reheating scenario in a two-throat geometry. We study KK mode wavefunctions of the full two-throat system in the Randall--Sundrum (RS) approximation and find an interesting subtlety in…

High Energy Physics - Theory · Physics 2010-02-03 Peter Langfelder

A string theory based inflationary model is developed where the inflaton interacts with a multitude of massive string level states causing dissipation of vacuum energy. Inflation terminates in a warm Universe without the need for reheating.

High Energy Physics - Phenomenology · Physics 2009-10-31 Arjun Berera , Thomas W. Kephart

It was recently understood that if the swampland conjectures are confronted to experiment they naturally point to a solution of the cosmological hierarchy problem in which the smallness of the dark energy is ascribed to an internal (dark)…

High Energy Physics - Phenomenology · Physics 2023-05-10 Luis A. Anchordoqui , Ignatios Antoniadis , Dieter Lust