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Related papers: Inflaton mass in the nuMSM inflation

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In many models of inflation, reheating is realized through a coupling between the inflaton and the Higgs boson. Often, the mass of the inflaton is of order $10^{13}~$GeV determined by the amplitude of the scalar fluctuation spectrum.…

High Energy Physics - Phenomenology · Physics 2025-08-19 Yann Cado , Mathieu Gross , Yann Mambrini , Keith Olive

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 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

We analyse the process of reheating the Universe in the electroweak theory where the Higgs field plays a role of the inflaton. We estimate the maximal temperature of the Universe and fix the initial conditions for radiation-dominated phase…

High Energy Physics - Phenomenology · Physics 2010-04-14 F. Bezrukov , D. Gorbunov , M. Shaposhnikov

Renormalisation group analysis with the present measurements of the top quark mass $m_t = 172.69\pm 0.30$ GeV indicates that the Standard Model (SM) Higgs potential becomes unstable at energy scales $\sim 10^{10}$ GeV. This may be…

High Energy Physics - Phenomenology · Physics 2024-02-26 Shinsuke Kawai , Nobuchika Okada , Qaisar Shafi

We show that warm inflation can be realized within a minimal extension of the Standard Model with three right-handed neutrinos, three complex scalars and a gauged lepton/B-L U(1) symmetry. This simple model can address all the shortcomings…

High Energy Physics - Phenomenology · Physics 2022-01-05 Miguel Levy , João G. Rosa , Luis B. Ventura

We show how to enlarge the $\nu$MSM (the minimal extension of the standard model by three right-handed neutrinos) to incorporate inflation and provide a common source for electroweak symmetry breaking and for right-handed neutrino masses.…

High Energy Physics - Phenomenology · Physics 2011-05-05 Mikhail Shaposhnikov , Igor Tkachev

We examine an intriguing possibility that a single field is responsible for both inflation and dark matter, focussing on the minimal set-up where inflation is driven by a scalar coupling to curvature. We study in detail the reheating…

High Energy Physics - Phenomenology · Physics 2021-09-08 Oleg Lebedev , Jong-Hyun Yoon

We discuss inflation and dark matter in the inert doublet model coupled non-minimally to gravity where the inert doublet is the inflaton and the neutral scalar part of the doublet is the dark matter candidate. We calculate the various…

High Energy Physics - Phenomenology · Physics 2017-11-16 Sandhya Choubey , Abhass Kumar

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…

High Energy Physics - Phenomenology · Physics 2025-02-14 Mar Bastero-Gil , António Torres Manso

Considering gravitino dark matter scenarios, we study constraints on the reheating temperature of inflation. We present the gauge-invariant result for the thermally produced gravitino yield to leading order in the Standard Model gauge…

High Energy Physics - Phenomenology · Physics 2008-11-26 Josef Pradler , Frank Daniel Steffen

We study the augmentation of the Standard Model (SM) with another $SU(2)$ Higgs doublet and right-handed neutrinos. The second Higgs doublet ($\Phi_2$) is defined to be odd under the $Z_2$ symmetry, and hence, the lightest stable neutral…

High Energy Physics - Phenomenology · Physics 2026-02-03 Seong Chan Park , Shilpa Jangid

We revisit Higgs inflation in the framework of a minimal extension of the Standard Model gauge symmetry by a $U(1)_{B-L}$ factor. Various aspects are taken into account with particular focus on the role of the supersymmetry breaking (SUSY)…

High Energy Physics - Phenomenology · Physics 2021-09-29 Waqas Ahmed , Athanasios Karozas , George K. Leontaris

If cosmic inflation was driven by an electrically neutral scalar field stable on cosmological time scales, the field necessarily constitutes all or part of dark matter (DM). We study this possibility in a scenario where the inflaton field…

High Energy Physics - Phenomenology · Physics 2019-03-13 Juan P. Beltrán Almeida , Nicolás Bernal , Javier Rubio , Tommi Tenkanen

We have discussed in detail how neutrinos produced from inflaton solely through gravitational interaction can successfully reheat the universe. For this, we have introduced the well-known Type-I seesaw neutrino model. Depending on seesaw…

High Energy Physics - Phenomenology · Physics 2025-04-01 Md Riajul Haque , Debaprasad Maity , Rajesh Mondal

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

We present a minimal UV complete framework to embed inflation and dark matter by extending the standard model with a singlet real scalar field (the inflaton) and a singlet fermonic field acting as dark matter. The inflaton features the most…

High Energy Physics - Phenomenology · Physics 2022-07-27 Nicolás Bernal , Yong Xu

We investigate the possibility of Higgs inflation with an extended standard model by right-handed neutrinos and scalar dark matter. We find that the masses of the dark matter and one of the right-handed neutrinos should stand around TeV and…

High Energy Physics - Phenomenology · Physics 2015-04-29 Hiroyuki Ishida

We consider the conditions for the decay products of perturbative inflaton decay to thermalize. The importance of considering the full spectrum of inflaton decay products in the thermalization process is emphasized. It is shown that the…

High Energy Physics - Phenomenology · Physics 2009-10-31 John McDonald

We study reheating after the end of inflation in models where the inflaton is the superpartner of goldstino and is charged under a gauged $U(1)$ R-symmetry. We consider two classes of models -- one is small field characterized by an almost…

High Energy Physics - Theory · Physics 2021-12-10 Yermek Aldabergenov , Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono
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