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It is pointed out that hybrid inflation can be implemented with the inflaton field rolling away from the origin instead of towards it. This `inverted' hybrid inflation has a spectral index $ n < 1 $, in contrast with ordinary hybrid…

High Energy Physics - Phenomenology · Physics 2008-11-26 David H. Lyth , Ewan D. Stewart

We construct a hybrid inflationary model associated with the superheavy scale of the minimal supersymmetric standard model which is based on the simplest superpotential for symmetry breaking and in which the inflaton potential along the…

High Energy Physics - Phenomenology · Physics 2009-06-19 C. Panagiotakopoulos

We propose a simple high-scale inflationary scenario based on a phenomenologically viable model with direct gauge mediation of low-scale supersymmetry breaking. Hybrid inflation is occurred in a hidden supersymmetry breaking sector. Two…

High Energy Physics - Phenomenology · Physics 2011-03-31 Yuichiro Nakai , Manabu Sakai

Moduli fields, which parameterize perturbative flat directions of the potential in supersymmetric theories, are natural candidates to act as inflatons. An inflationary potential on moduli space can result if the scale of dynamical SUSY…

High Energy Physics - Theory · Physics 2009-10-28 Scott Thomas

The abundance of the QCD axion is known to be suppressed if the Hubble parameter during inflation, $H_{\rm inf}$, is lower than the QCD scale, and if the inflation lasts sufficiently long. We show that the tight upper bound on the inflation…

High Energy Physics - Phenomenology · Physics 2020-06-24 Hiroki Matsui , Fuminobu Takahashi , Wen Yin

We consider the model of ``Chain Inflation,'' in which the period of inflation in our universe took the form of a long sequence of quantum tunneling events. We find that in the simplest such scenario, in which the tunneling processes are…

High Energy Physics - Phenomenology · Physics 2014-11-18 Brian Feldstein , Brock Tweedie

The QCD axion in the pre-inflation scenario faces a stringent isocurvature constraint, which requires a relatively low Hubble scale during inflation. If the axion was heavier than the Hubble scale during inflation, its isocurvature is…

High Energy Physics - Phenomenology · Physics 2026-01-19 Priyesh Chakraborty , Junyi Cheng , Matthew Reece , Zekai Wang

We investigate the possibility that inflation originates from a composite field theory, in terms of an effective chiral Lagrangian involving a dilaton and pions. The walking dynamics of the theory constrain the potential in a specific way,…

High Energy Physics - Phenomenology · Physics 2024-11-11 Giacomo Cacciapaglia , Dhong Yeon Cheong , Aldo Deandrea , Wanda Isnard , Seong Chan Park

Scalar field models of inflation based on a large nonminimal coupling to gravity xi, in particular, Higgs inflation, may violate unitarity at an energy scale ~ M_p / xi << M_p. In this case the model is incomplete at energy scales relevant…

High Energy Physics - Phenomenology · Physics 2010-12-01 Rose N. Lerner , John McDonald

Generically, the gravitational-wave or tensor-mode contribution to the primordial curvature spectrum of inflation is tiny if the field-range of the inflaton is much smaller than the Planck scale. We show that this pessimistic conclusion is…

High Energy Physics - Theory · Physics 2014-01-15 Arthur Hebecker , Sebastian C. Kraus , Alexander Westphal

A new shifted hybrid inflationary scenario is introduced which, in contrast to the older one, relies only on renormalizable superpotential terms. This scenario is automatically realized in a concrete extension of the "minimal"…

High Energy Physics - Phenomenology · Physics 2009-11-07 R. Jeannerot , S. Khalil , G. Lazarides

The slow roll inflation requires an extremely flat inflaton potential. The supersymmetry (SUSY) is not only motivated from the gauge hierarchy problem, but also from stabilizing that flatness of the inflaton potential against radiative…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Watari , T. Yanagida

We propose a hybrid inflation model where a pseudo-Nambu-Goldstone boson inflaton couples to $N$ waterfall scalar fields respecting a $Z_N$ symmetry. We identify the phases for the inflation and the consequent waterfall transition,…

High Energy Physics - Phenomenology · Physics 2026-05-22 Hyun Min Lee , Adriana G. Menkara

In this paper, we revisit the idea of locked inflation, which does not require a potential satisfying the normal slow-roll condition, but suffers from the problems associated with "saddle inflation". We propose a scenario based on locked…

High Energy Physics - Theory · Physics 2010-01-15 Yang Liu , Yun-Song Piao , Zong-Guo Si

We show that in supersymmetry one can obtain inflationary potentials in the observable sector that are sufficiently flat at sub-Planckian field values. Structure of the supersymmetric scalar potential along a flat direction combined with…

High Energy Physics - Theory · Physics 2012-10-16 Rouzbeh Allahverdi , Sean Downes , Bhaskar Dutta

Hybrid inflation is a two field model where inflation ends due to an instability. In the neighborhood of the instability point, the potential is very flat and the quantum fluctuations dominate over the classical motion of the inflaton and…

Cosmology and Nongalactic Astrophysics · Physics 2015-11-25 Jerome Martin , Vincent Vennin

We consider F-term hybrid inflation and supersymmetry breaking in the context of a model which largely respects a global U(1) R symmetry. The Kaehler potential parameterizes the Kaehler manifold with an enhanced U(1)_Rx(SU(1,1)/U(1))…

High Energy Physics - Phenomenology · Physics 2025-04-04 C. Pallis

A scheme of hybrid inflation is considered in the framework of the minimal supersymmetric SU(5) model with an extra singlet. The relevant role of the cubic term in the adjoint representation in the renormalizable superpotential is pointed…

High Energy Physics - Phenomenology · Physics 2009-10-30 L. Covi , G. Mangano , A. Masiero , G. Miele

We consider D-term inflation for small couplings of the inflaton to matter fields. Standard hybrid inflation then ends at a critical value of the inflaton field that exceeds the Planck mass. During the subsequent waterfall transition the…

High Energy Physics - Phenomenology · Physics 2015-06-22 W. Buchmuller , V. Domcke , K. Schmitz

Due to intra-field gravitational interactions, field configurations have a strong negative component to their energy density at the planckian and transplanckian scales, conceivably resulting in a sequestration of the transplanckian field…

General Relativity and Quantum Cosmology · Physics 2010-03-30 Robert Brout
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