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Related papers: Curvature perturbation and waterfall dynamics in h…

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In this paper the possibility of generating large scale curvature perturbations induced from the entropic perturbations during the waterfall phase transition of standard hybrid inflation model is studied. We show that whether or not…

High Energy Physics - Theory · Physics 2011-03-22 Ali Akbar Abolhasani , Hassan Firouzjahi

We estimate large-scale curvature perturbations from isocurvature fluctuations in the waterfall field during hybrid inflation, in addition to the usual inflaton field perturbations. The tachyonic instability at the end of inflation leads to…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 José Fonseca , Misao Sasaki , David Wands

We consider a variant of hybrid inflation where the waterfall phase transition happens during inflation. By adjusting the parameters associated with the mass of the waterfall field we arrange that the phase transition is not sharp so…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Ali Akbar Abolhasani , Hassan Firouzjahi , Mohammad Hossein Namjoo

We discuss the waterfall that ends hybrid inflation. Making some simplifying assumptions, that may be satisfied by GUT inflation models, two issues are addressed. First, the procedure of keeping the quantum fluctuation of the waterfall…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 David H. Lyth

We study carefully the contribution of the waterfall field to the curvature perturbation at the end of hybrid inflation. In particular we clarify the parameter dependence analytically under reasonable assumptions on the model parameters.…

Cosmology and Nongalactic Astrophysics · Physics 2011-03-28 Jinn-Ouk Gong , Misao Sasaki

We carried out numerical calculations of a contribution of the waterfall field to the primordial curvature perturbation (on uniform density hypersurfaces) $\zeta$, which is produced during waterfall transition in hybrid inflation scenario.…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-17 Edgar Bugaev , Peter Klimai

We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly generated at the end of inflation. By finely tuning the coupling of the fields to the waterfall we find that we can get a measurable amount…

Astrophysics · Physics 2009-11-11 Laila Alabidi , David Lyth

We identify a new inflationary regime for which more than 60 e-folds are generated classically during the waterfall phase occuring after the usual hybrid inflation. By performing a bayesian Monte-Carlo-Markov-Chain analysis, this scenario…

General Relativity and Quantum Cosmology · Physics 2011-03-22 Sebastien Clesse

For the original hybrid inflation as well as the supersymmetric F-term and D-term hybrid models, we calculate the level of non-gaussianities and the power spectrum of curvature perturbations generated during the waterfall, taking into…

Cosmology and Nongalactic Astrophysics · Physics 2014-03-26 Sébastien Clesse , Björn Garbrecht , Yi Zhu

We introduce a new method for calculating density perturbations in hybrid inflation which avoids treating the fluctuations of the "waterfall" field as if they were small perturbations about a classical trajectory. We quantize only the…

Cosmology and Nongalactic Astrophysics · Physics 2012-11-01 Alan H. Guth , Evangelos I. Sfakianakis

A recent variant of the inflationary paradigm is that the ``primordial'' curvature perturbations come from quantum fluctuations of a scalar field, subdominant and effectively massless during inflation, called the ``curvaton'', instead of…

Astrophysics · Physics 2009-11-10 David Langlois , Filippo Vernizzi

We construct a model of hybrid inflation within a controlled five-dimensional effective field theory framework. The inflaton and waterfall fields are realized as naturally light moduli of the 5D compactification. At the quantum level,…

High Energy Physics - Phenomenology · Physics 2014-11-20 Raman Sundrum , Christopher M. Wells

We discuss the possible role of isocurvature perturbations for the quantum decoherence of the curvature perturbation during inflation. We point out that if the inflaton trajectory in field space is curved, the adiabatic mode is generically…

Astrophysics · Physics 2011-08-04 Tomislav Prokopec , Gerasimos I. Rigopoulos

We provide an analytical study of the coupling of short and long wavelength fluctuation modes during the initial phase of reheating in two field models like hybrid inflation. In these models, there is - at linear order in perturbation…

High Energy Physics - Theory · Physics 2011-01-20 Laurence Perreault Levasseur , Guillaume Laporte , Robert Brandenberger

Inflation models can have an early phase of inflation where the evolution of the inflaton is driven by quantum fluctuations before entering the phase driven by the slope of the scalar field potential. For a Coleman-Weinberg potential this…

Cosmology and Nongalactic Astrophysics · Physics 2013-03-06 Arjun Berera , Raghavan Rangarajan

We study adiabatic (curvature) and entropy (isocurvature) perturbations produced during a period of cosmological inflation that is driven by multiple scalar fields with an arbitrary interaction potential. A local rotation in field space is…

Astrophysics · Physics 2009-10-31 Christopher Gordon , David Wands , Bruce A. Bassett , Roy Maartens

We present a new general mechanism for generating curvature perturbations after inflation. Our model is based on the simple assumption that a field that starts to oscillate after inflation has a potential characterized by an underlying…

High Energy Physics - Phenomenology · Physics 2008-11-26 Tomohiro Matsuda

We propose a hybrid inflation model with a complex waterfall field which contains an interaction term that breaks the U(1) global symmetry associated to the waterfall field charge. We show that the asymmetric evolution of the real and…

High Energy Physics - Phenomenology · Physics 2008-11-26 David Delepine , Carlos Martinez , L. Arturo Urena-Lopez

The dynamics of hybrid models is usually approximated by the evolution of a scalar field slowly rolling along a nearly flat valley. Inflation ends with a waterfall phase, due to a tachyonic instability. This final phase is usually assumed…

Cosmology and Nongalactic Astrophysics · Physics 2011-09-27 Sébastien Clesse

We study the emergence of quantum entanglement in multi-field inflation. In this scenario, the perturbations of one field contribute to the observable curvature perturbation, while multi-field dynamics with the other fields affect the…

Cosmology and Nongalactic Astrophysics · Physics 2018-09-19 Nadia Bolis , Tomohiro Fujita , Shuntaro Mizuno , Shinji Mukohyama
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