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We consider hybrid inflation for small couplings of the inflaton to matter such that the critical value of the inflaton field exceeds the Planck mass. It has recently been shown that inflation then continues at subcritical inflaton field…

High Energy Physics - Phenomenology · Physics 2015-04-16 Wilfried Buchmuller , Koji Ishiwata

Minimal hybrid inflation in supergravity has been ruled out by the 2015 Planck observations because the spectral index of the produced curvature perturbation falls outside observational bounds. To resurrect the model, a number of…

High Energy Physics - Phenomenology · Physics 2016-10-25 Konstantinos Dimopoulos , Charlotte Owen

We study inflation driven by a slow-rolling inflaton field, characterised by a quadratic potential, and incorporating radiative corrections within the context of supergravity. In this model the energy scale of inflation is not overly…

High Energy Physics - Phenomenology · Physics 2011-02-16 Gabriel German , Graham Ross , Subir Sarkar

For hybrid inflationary potentials, we derive the tunneling rate from field configurations along the flat direction towards the waterfall regime. This process competes with the classically rolling evolution of the scalar fields and needs to…

High Energy Physics - Phenomenology · Physics 2010-10-27 Bjorn Garbrecht , Thomas Konstandin

We consider the construction of inverted hybrid inflation models in which the vacuum energy during inflation is at the TeV scale, and the inflaton couples to the Higgs field. Such models are of interest in the context of some recently…

High Energy Physics - Phenomenology · Physics 2009-11-07 Edmund J. Copeland , David Lyth , Arttu Rajantie , Mark Trodden

We discuss the hybrid inflation model where the inflaton field is nonminimally coupled to gravity. In the Jordan frame, the potential contains $\phi^4$ term as well as terms in the original hybrid inflation model. In our model, inflation…

High Energy Physics - Theory · Physics 2011-02-22 Seoktae Koh , Masato Minamitsuji

We consider supersymmetric inflation with the hybrid-type potential. In the absence of the symmetry that forbids Hubble-induced mass terms, the inflaton mass will be as large as the Hubble scale during inflation. We consider gravitational…

High Energy Physics - Phenomenology · Physics 2010-02-15 Tomohiro Matsuda

We investigate a topological inflation model in supergravity. By means of numerical simulations, it is confirmed that topological inflation can take place in supergravity. We also show that the condition for successful inflation depends not…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Kawasaki , Nobuyuki Sakai , Masahide Yamaguchi , T. Yanagida

A new scenario of hybrid-like inflation is considered without using hybrid-type potential. Radiation raised continuously by a dissipating inflaton field keeps symmetry restoration in a remote sector, and the false-vacuum energy of the…

Cosmology and Nongalactic Astrophysics · Physics 2009-07-22 Tomohiro Matsuda

Inverted hybrid inflation (in which the inflaton field slowly rolls away from the origin, giving a spectral index $n\lsim 1$) is an appealing variant of the more usually studied hybrid model. Analysing the model alongside the ordinary…

High Energy Physics - Phenomenology · Physics 2009-10-30 S. F. King , J. Sanderson

We propose a new version of the hybrid inflation scenario that produces a significantly tilted n>1 spectrum of curvature perturbations. This may happen in supersymmetric models where the inflaton field acquires a mass proportional to the…

Astrophysics · Physics 2009-09-29 Juan Garcia-Bellido , Andrei Linde

In low scale quantum gravity scenarios the fundamental scale of nature can be as low as TeV, in order to address the naturalness of the electroweak scale. A number of difficulties arise in constructing specific models; stabilisation of the…

High Energy Physics - Phenomenology · Physics 2009-11-07 Anne M Green , Anupam Mazumdar

The general structure of Hybrid Inflation remains a very well-motivated mechanism for lower-scale cosmic inflation in the face of improving constraints on the tensor-to-scalar ratio. However, as originally modeled, the "waterfall" field in…

High Energy Physics - Phenomenology · Physics 2021-07-23 Kaustubh Deshpande , Soubhik Kumar , Raman Sundrum

We study the supergravity hybrid inflation model of Ref.[1] in the presence of a modulus field. The eta-problem is solved by a shift symmetry for the inflaton, which protects the inflaton mass even in the presence of the modulus field.…

High Energy Physics - Phenomenology · Physics 2010-11-09 Sander Mooij , Marieke Postma

We discuss inflation in models with large extra dimensions, driven by a bulk scalar field. The brane inflaton is then a single effective field, obtained from the bulk scalar field by scaling. The self interaction terms of the effective…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. N. Mohapatra , A. Pérez-Lorenzana , C. A. de S. Pires

It is shown that, when the inflaton field modulates the gauge kinetic function of the gauge fields in supergravity realisations of inflation, the dynamic backreaction leads to a new inflationary attractor solution, in which the inflaton's…

Cosmology and Nongalactic Astrophysics · Physics 2016-01-15 Konstantinos Dimopoulos , George Lazarides , Jacques M. Wagstaff

In conventional scenario of thermal inflation, the requirement that the reheating temperature must be larger than the temperature of the nucleosynthesis puts a lower bound on the mass of the inflaton field. At the same time, the mass of the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Tomohiro Matsuda

In hybrid inflation, the inflaton generically has a tadpole due to gravitational effects in supergravity, which significantly changes the inflaton dynamics in high-scale supersymmetry. We point out that the tadpole can be cancelled if there…

High Energy Physics - Phenomenology · Physics 2015-06-12 Tetsutaro Higaki , Kwang Sik Jeong , Fuminobu Takahashi

Allowing for the possibility of large extra dimensions, the fundamental Planck scale $M$ could be anywhere in the range $\TeV\lsim M\lsim \mpl$, where $\mpl=2.4\times 10^{18}\GeV$ is the four-dimensional Planck scale. If $M\sim\TeV$,…

High Energy Physics - Phenomenology · Physics 2009-10-31 David H Lyth

We investigate chaotic inflation models with two scalar fields, such that one field (the inflaton) rolls while the other is trapped in a false vacuum state. The false vacuum becomes unstable when the inflaton field falls below some critical…

Astrophysics · Physics 2009-10-22 Edmund J Copeland , Andrew R Liddle , David H Lyth , Ewan D Stewart , David Wands
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