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The Higgs inflation scenario is an approach to realize the cosmic inflation, where the Higgs boson plays a role of the inflaton. In the minimal model, it would be difficult to satisfy theoretical constraints from vacuum stability and…

High Energy Physics - Phenomenology · Physics 2014-05-23 Toshinori Matsui

We study radiative plateau-like inflation \& Z$_{BL}$-portal freeze-in fermionic dark matter (DM) in a minimal B-L extended model. The U(1)$_{B-L}$ Higgs, responsible for heavy neutrino masses, also drives inflation in the early universe,…

High Energy Physics - Phenomenology · Physics 2022-11-30 Anish Ghoshal , Nobuchika Okada , Arnab Paul

We show that the seesaw mechanism as well as leptogenesis are natural outcomes of a viable chaotic inflation in supergravity. The inflation model contains two superfields, the inflaton and stabilizer fields, which, being singlets under the…

High Energy Physics - Phenomenology · Physics 2016-03-23 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We describe how non-minimal coupling term between the Higgs boson and gravity can lead to the chaotic inflation in the Standard Model without introduction of any additional degrees of freedom. Produced cosmological perturbations are…

High Energy Physics - Phenomenology · Physics 2008-05-16 F. L. Bezrukov

We investigate an inflation model with the inflaton being identified with a Higgs boson responsible for the breaking of U(1)B-L symmetry. We show that supersymmetry must remain a good symmetry at scales one order of magnitude below the…

High Energy Physics - Phenomenology · Physics 2012-03-13 Kazunori Nakayama , Fuminobu Takahashi

We investigate an inflationary model involving a gauge singlet scalar and fermionic dark matter. The mixing between the singlet scalar and the Higgs boson provides a portal to dark matter. The inflaton could either be the Higgs boson or the…

High Energy Physics - Phenomenology · Physics 2017-10-04 Aditya Aravind , Minglei Xiao , Jiang-Hao Yu

We construct a chaotic inflation model in which the Higgs fields play the role of the inflaton in the standard model as well as in the singlet extension of the supersymmetric standard model. The key idea is to allow a non-canonical kinetic…

High Energy Physics - Phenomenology · Physics 2011-02-15 Kazunori Nakayama , Fuminobu Takahashi

The Standard Model Higgs boson, which has previously been shown to develop an effective vacuum expectation value during inflation, can give rise to large particle masses during inflation and reheating, leading to temporary blocking of the…

High Energy Physics - Phenomenology · Physics 2019-09-20 Katherine Freese , Evangelos I. Sfakianakis , Patrick Stengel , Luca Visinelli

A reheating phase in the early universe is an essential part of all inflationary models during which not only the Standard Model (SM) quanta are produced but it can also shed light on the production of dark matter. In this work, we explore…

High Energy Physics - Phenomenology · Physics 2023-02-24 Aqeel Ahmed , Bohdan Grzadkowski , Anna Socha

The Higgs inflation scenario is an approach to realize the inflation, in which the Higgs boson plays a role of the inflaton without introducing a new particle. We investigate a Higgs inflation scenario in the so-called radiative seesaw…

High Energy Physics - Phenomenology · Physics 2013-05-02 Toshinori Matsui

We study the minimal extension of the SM by a scalar with quartic interaction serving as an inflaton. For the model where scale symmetry is broken only in the inflaton sector, the mass of the inflaton is constrained to be relatively low.…

High Energy Physics - Phenomenology · Physics 2021-01-04 Fedor Bezrukov , Abigail Keats

We study the decay of scalar fields, in particular the inflaton, into lighter scalars in a De Sitter spacetime background. After providing a practical definition of the rate, we focus on the case of an inflaton interacting with a massless…

High Energy Physics - Phenomenology · Physics 2011-04-15 D. Boyanovsky , R. Holman , S. Prem Kumar

We argue that the Higgs boson of the Standard Model can lead to inflation and produce cosmological perturbations in accordance with observations. An essential requirement is the non-minimal coupling of the Higgs scalar field to gravity; no…

High Energy Physics - Theory · Physics 2008-11-26 F. L. Bezrukov , M. E. Shaposhnikov

We discuss a minimal extension of the Standard Model (SM) where a single real scalar field serves as both inflaton and dark matter. The corresponding Lagrangian contains the renormalizable interactions of the inflaton field. Quantum effects…

High Energy Physics - Phenomenology · Physics 2022-05-30 Jong-Hyun Yoon

Inflation occurring at energy densities less than (10$^{14}$ GeV)$^4$ produces tensor perturbations too small to be measured by cosmological surveys. However, we show that it is possible to probe low scale inflation by measuring the mass of…

High Energy Physics - Phenomenology · Physics 2016-12-14 Joseph Bramante , Jessica Cook , Antonio Delgado , Adam Martin

Inflection-point inflation is an interesting possibility to realize a successful slow-roll inflation when inflation is driven by a single scalar field with its initial value below the Planck mass ($\phi_I \lesssim M_{Pl}$). In order for a…

High Energy Physics - Phenomenology · Physics 2017-03-08 Nobuchika Okada , Digesh Raut

It is a longstanding desire of cosmologists, and particle physicists as well, to connect inflation to low energy physics, culminating, for instance, in what is known as Higgs inflation. The condition for the standard Higgs boson playing the…

High Energy Physics - Phenomenology · Physics 2017-11-15 J. G. Ferreira , C. A. de S. Pires , J. G. Rodrigues , P. S. Rodrigues da Silva

The existing constraints from particle colliders reveal a suspicious but nonlethal metastability for our current electroweak vacuum of Higgs potential in the standard model of particle physics, which is, however, disfavored in the early…

High Energy Physics - Phenomenology · Physics 2021-01-13 Rong-Gen Cai , Shao-Jiang Wang

We consider a scenario where the inflaton decays to a hidden sector thermally decoupled from the visible Standard Model sector. A tiny portal coupling between the hidden and the visible sectors later heats the visible sector so that the…

Cosmology and Nongalactic Astrophysics · Physics 2016-10-19 Tommi Tenkanen , Ville Vaskonen

We study a recently proposed running kinetic inflation model in which the inflaton potential becomes flat due to rapid growth of the kinetic term at large inflaton field values. As concrete examples, we build a variety of chaotic inflation…

High Energy Physics - Phenomenology · Physics 2010-12-09 Kazunori Nakayama , Fuminobu Takahashi