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We explore a new class of supersymmetric models of inflation where the inflaton is realised as a combination of a Higgs field and (gauge non-singlet) matter fields, using a "tribrid" structure of the superpotential. Inflation is associated…

高能物理 - 唯象学 · 物理学 2015-03-20 Stefan Antusch , David Nolde , Mansoor Ur Rehman

We propose an entirely new class of particle physics models of inflation based on the phase transition associated with the spontaneous breaking of family symmetry responsible for the generation of the effective quark and lepton Yukawa…

高能物理 - 唯象学 · 物理学 2008-11-26 S. Antusch , S. F. King , M. Malinsky , L. Velasco-Sevilla , I. Zavala

Tribrid inflation is a variant of supersymmetric hybrid inflation in which the inflaton is a matter field (which can be charged under gauge symmetries) and inflation ends by a GUT-scale phase transition of a waterfall field. These features…

高能物理 - 唯象学 · 物理学 2015-09-30 Stefan Antusch , David Nolde

Tribrid inflation is a class of supersymmetric inflation models where the scalar component of a matter superfield, or a $D$-flat direction of matter fields, drives inflation. Similar to Hybrid inflation, the end of inflation is reached when…

高能物理 - 唯象学 · 物理学 2024-11-06 Stefan Antusch , Katarina Trailović

Recently, a class of inflation models in supergravity with gauge non-singlet matter fields as the inflaton has been proposed. It is based on a `tribrid' structure in the superpotential and on a Heisenberg symmetry for solving the…

高能物理 - 理论 · 物理学 2011-04-20 Stefan Antusch , Koushik Dutta , Johanna Erdmenger , Sebastian Halter

A new class of particle physics models of inflation based on the phase transition associated with the spontaneous breaking of family symmetry is proposed. The Higgs fields responsible for the breaking of family symmetry, the flavons, are…

高能物理 - 唯象学 · 物理学 2009-02-02 I. Zavala

We realize and study a model of hybrid inflation in the context of softly broken supersymmetry. The inflaton is taken to be a flat direction in the superfield space and, due to unsuppressed couplings, its soft supersymmetry breaking mass…

高能物理 - 唯象学 · 物理学 2016-08-25 Laura Covi

We use modular symmetry as an organizing principle that attempts to simultaneously address the lepton flavor puzzle, inflation, and post-inflationary reheating. We demonstrate this approach using the finite modular group $A_4$ in the lepton…

高能物理 - 唯象学 · 物理学 2025-11-05 Gui-Jun Ding , Si-Yi Jiang , Yong Xu , Wenbin Zhao

Supersymmetric hybrid inflation is an exquisite framework to connect inflationary cosmology to particle physics at the scale of grand unification. Ending in a phase transition associated with spontaneous symmetry breaking, it can naturally…

高能物理 - 唯象学 · 物理学 2014-07-31 Wilfried Buchmuller , Valerie Domcke , Kohei Kamada , Kai Schmitz

We present the supersymmetric extension of the unified model for inflation and Dark Matter studied in Ref. arXiv:1811.02302. The scenario is based on the incomplete decay of the inflaton field into right-handed (s)neutrino pairs. By…

高能物理 - 唯象学 · 物理学 2025-02-14 Mar Bastero-Gil , António Torres Manso

We discuss a new class of tribrid inflation models in supergravity, where the shape of the inflaton potential is dominated by effects from the K\"ahler potential. Tribrid inflation is a variant of hybrid inflation which is particularly…

高能物理 - 唯象学 · 物理学 2015-06-05 Stefan Antusch , David Nolde

In this talk, I shall focus on theories beyond the Standard Model which predict massive neutrinos. Hybrid inflation emerges naturally in these theories: the slow-rolling inflaton field is a gauge singlet which couples with a GUT Higgs field…

高能物理 - 唯象学 · 物理学 2007-05-23 Rachel Jeannerot

We propose a class of models of supersymmetric hilltop inflation (also called "new inflation") where the initial conditions of the inflaton close to the hilltop are generated through "matter field preinflation". This is achieved via a…

高能物理 - 唯象学 · 物理学 2014-05-29 Stefan Antusch , David Nolde , Stefano Orani

We present the first quantum field theory model of inflation that is renormalizable in the matter sector, with a super-Hubble inflaton mass and sub-Planckian field excursions, which is thus technically natural and consistent with a…

高能物理 - 唯象学 · 物理学 2021-01-11 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , João G. Rosa

We embed the supersymmetric standard model of hybrid inflation based on the next-to-minimal superpotential term $\lambda NH_uH_d$ supplemented by an inflaton term $\kappa \phi N^2$, into an extra-dimensional framework, in which all the…

高能物理 - 唯象学 · 物理学 2009-11-07 M. Bastero-Gil , V. Di Clemente , S. F. King

We present a unified model where the same scalar field can drive inflation and account for the present dark matter abundance. This scenario is based on the incomplete decay of the inflaton field into right-handed neutrino pairs, which is…

高能物理 - 唯象学 · 物理学 2025-02-14 Antonio Torres Manso , Joao G. Rosa

We present a see-saw $A_4$ model for Tri-Bimaximal mixing which is based on a very economical flavour symmetry and field content and still possesses all the good features of $A_4$ models. In particular the charged lepton mass hierarchies…

高能物理 - 唯象学 · 物理学 2009-08-20 Guido Altarelli , Davide Meloni

A simple realization of inflation consists of adding the following operators to the Einstein-Hilbert action: (partial phi)^2, lambda phi^4, and xi phi^2 R, with xi a large non-minimal coupling. Recently there has been much discussion as to…

高能物理 - 唯象学 · 物理学 2010-12-01 Mark P. Hertzberg

We show that inflation can naturally occur at a finite temperature T>H that is sustained by dissipative effects, when the inflaton field corresponds to a pseudo Nambu-Goldstone boson of a broken gauge symmetry. Similarly to "Little Higgs"…

高能物理 - 唯象学 · 物理学 2016-10-12 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , Joao G. Rosa

We clarify inflaton models by considering them as effective field theories in the Ginzburg-Landau spirit.In this new approach, the precise form of the inflationary potential is constructed from the present WMAP data, and a useful scheme is…

天体物理学 · 物理学 2009-11-10 D. Cirigliano , H. J. de Vega , N. G. Sanchez
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