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Related papers: Can MSSM Particle be the Inflaton?

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Current Higgs boson and top quark data favor metastability of our vacuum which raises questions as to why the Universe has chosen an energetically disfavored state and remained there during inflation. In this Letter, we point out that these…

High Energy Physics - Phenomenology · Physics 2015-12-15 Christian Gross , Oleg Lebedev , Marco Zatta

We study in detail a scenario in which the inflaton scalar field couples to both a visible sector (VS) and a hidden sector (HS). The VS is assumed to contain the Standard Model (SM), while the HS contains a dark matter (DM) candidate. We…

High Energy Physics - Phenomenology · Physics 2026-05-12 Simon Cléry , Jean Kimus , Michel H. G. Tytgat

We study preheating, i.e., non-perturbative resonant decay, of flat direction fields, concentrating on MSSM flat directions and the right handed sneutrino. The difference between inflaton preheating and flaton preheating, is that the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Marieke Postma , Anupam Mazumdar

The minimal $U(1)_{L_\mu-L_\tau}$ gauge symmetry extended Standard Model (SM) is a well motivated framework that resolves the discrepancy between the theoretical prediction and experimental observation of muon anomalous magnetic moment. We…

High Energy Physics - Phenomenology · Physics 2024-10-08 Arnab Paul , Sourov Roy , Abhijit Kumar Saha

A mirror-extended standard model (MESM) is offered, where in the left-right symmetric underlying action the sector of the standard model (SM) and its mirror copy have the same SU(2)\times U(1) gauge structure and parameters; the mirror…

High Energy Physics - Theory · Physics 2021-08-31 Alexander B. Kaganovich

The standard model Higgs boson can serve as the inflaton field of slow roll inflationary models provided it exhibits a large non-minimal coupling with the gravitational scalar curvature. The Higgs boson self interactions and its couplings…

High Energy Physics - Phenomenology · Physics 2009-11-05 T. E. Clark , Boyang Liu , S. T. Love , T. ter Veldhuis

We propose an inflationary scenario, M-flation, in which inflation is driven by three $N\times N$ hermitian matrices $\Phi_i, i=1,2,3$. The inflation potential of our model, which is strongly motivated from string theory, is constructed…

High Energy Physics - Theory · Physics 2010-10-13 Amjad Ashoorioon , Hassan Firouzjahi , M. M. Sheikh-Jabbari

Based on a previously derived superstring model possessing a cosmological sector that mimics Starobinsky inflation, we analyze several questions addressed in the recent literature: the generation of an effective $R^2$-term, the stability of…

High Energy Physics - Theory · Physics 2025-09-03 Ignatios Antoniadis , Dimitri V. Nanopoulos , Keith A. Olive

We propose a realisation of 'new inflation' in supergravity (SUGRA), where the flatness of the inflaton potential is protected by a Heisenberg symmetry. Inflation can be associated with a particle physics phase transition, with the inflaton…

High Energy Physics - Phenomenology · Physics 2013-12-04 Stefan Antusch , Francesco Cefala

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 consider a quantum corrected inflation scenario driven by a generic GUT or Standard Model type particle model whose scalar field playing the role of an inflaton has a strong non-minimal coupling to gravity. We show that currently widely…

High Energy Physics - Phenomenology · Physics 2009-01-06 A. O. Barvinsky , A. Yu. Kamenshchik , A. A. Starobinsky

We propose a cosmological inflationary scenario based on the supergravity-embedded Standard Model supplemented by the right-handed neutrinos. We show that with an appropriate Kahler potential the L-H_u direction gives rise to successful…

High Energy Physics - Phenomenology · Physics 2013-05-30 Masato Arai , Shinsuke Kawai , Nobuchika Okada

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 propose that the inflaton is coupled to ordinary matter only gravitationally and that it decays into a completely hidden sector. In this scenario both baryonic and dark matter originate from the decay of a flat direction of the minimal…

High Energy Physics - Phenomenology · Physics 2009-11-07 Kari Enqvist , Shinta Kasuya , Anupam Mazumdar

We study the effects of including one-loop radiative corrections in a non-supersymmetric hybrid inflationary model. These corrections can arise from Yukawa couplings between the inflaton and right-handed neutrinos, and induce a maximum in…

High Energy Physics - Phenomenology · Physics 2009-10-29 Mansoor Ur Rehman , Qaisar Shafi , Joshua R. Wickman

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

Models of induced-gravity inflation are formulated within Supergravity employing as inflaton the Higgs field which leads to a spontaneous breaking of a U(1)_{B-L} symmetry at Mgut=2x10^16 GeV. We use a renormalizable superpotential, fixed…

High Energy Physics - Phenomenology · Physics 2023-11-16 C. Pallis

Extensions of the Standard Model and general relativity featuring a UV fixed point can leave observable implications at accessible energies. Although mass parameters such as the Planck scale can appear through dimensional transmutation, all…

High Energy Physics - Phenomenology · Physics 2019-09-13 Alberto Salvio

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"…

High Energy Physics - Phenomenology · Physics 2016-10-12 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , Joao G. Rosa

The idea of the strongly interacting field theories constitutes one of the pillars of the standard model of particle physics. The goal of this work is to export such theories to cosmology. Here we are interested in models in which the…

High Energy Physics - Phenomenology · Physics 2012-05-07 Phongpichit Channuie