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Related papers: Can MSSM Particle be the Inflaton?

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One interpretation of proton stability is the existence of extra-flat directions of the MSSM, in particular $u^{c}u^{c}d^{c}e^{c}$ and $QQQL$, where the operators lifting the potential are suppressed by a mass scale $\Lambda$ which is much…

High Energy Physics - Phenomenology · Physics 2008-11-26 John McDonald , Osamu Seto

We study models of inflation where the inflaton corresponds to a flat direction in field space and its mass term is generated by gravity mediated soft supersymmetry breaking at high scale. Assuming the inflaton to have non negligible…

High Energy Physics - Phenomenology · Physics 2007-05-23 Laura Covi

The potential during inflation must be very flat in, at least, the direction of the inflaton. In renormalizable global supersymmetry, flat directions are ubiquitous, but they are not preserved in a generic supergravity theory. It is known…

High Energy Physics - Theory · Physics 2009-09-29 Mary K. Gaillard , David H. Lyth , Hitoshi Murayama

Flat directions in the Minimal Supersymmetric Standard Model (MSSM) can become unstable due to radiative corrections, and the global minimum of the (zero temperature) potential can lie at large values of the squark and/or slepton fields.…

High Energy Physics - Phenomenology · Physics 2009-09-15 Toby Falk , Keith A. Olive , Leszek Roszkowski , Anupam Singh , Mark Srednicki

We present a model of inflation in a supergravity framework in the Einstein frame where the Higgs field of the next to minimal supersymmetric standard model (NMSSM) plays the role of the inflaton. Previous attempts which assumed non-minimal…

High Energy Physics - Phenomenology · Physics 2010-12-09 Ido Ben-Dayan , Martin B. Einhorn

It has been recently pointed out that the polarization BICEP2 results are consistent with the identification of an inflaton mass m \simeq 10^{13} GeV with the SUSY breaking scale in an MSSM with a fine-tuned SM Higgs. This identification…

High Energy Physics - Theory · Physics 2015-06-19 Luis E. Ibanez , Irene Valenzuela

We consider instant preheating as the mechanism for generating the curvature perturbation at the end of chaotic inflation. Then we examine if inflation could be driven by a Minimal Supersymmetric Standard Model (MSSM) flat direction or a…

High Energy Physics - Phenomenology · Physics 2010-10-27 Tomohiro Matsuda

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 discuss the constraints on the inhomogeneous reheating scenario. In particular, we discuss the prospects for low scale inflation with a Hubble constant of the order of the gravitino mass, and the possibility that an MSSM flat direction…

Astrophysics · Physics 2009-11-10 Marieke Postma

We explore the possibility that inflation is driven by supersymmetry breaking with the superpartner of the goldstino (sgoldstino) playing the role of the inflaton. Moreover, we impose an R-symmetry that allows to satisfy easily the…

High Energy Physics - Theory · Physics 2017-11-22 Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono , Rob Knoops

In the framework of MSSM inflation, matter and gravitino production are here investigated through the decay of the fields which are coupled to the udd inflaton, a gauge invariant combination of squarks. After the end of inflation, the flat…

High Energy Physics - Phenomenology · Physics 2017-10-31 Andrea Ferrantelli

In the context of the Higgs model involving gauge and Yukawa interactions with the spontaneous gauge symmetry breaking, we consider $\lambda \phi^4$ inflation with non-minimal gravitational coupling, where the Higgs field is identified as…

High Energy Physics - Phenomenology · Physics 2015-09-23 Nobuchika Okada , Digesh Raut

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 show that a class of Wess--Zumino models lead to inflation in supersymmetry and supergravity. This is due to the existence of a classically flat direction generic to these models. The pseudomodulus that parametrizes this flat direction…

High Energy Physics - Phenomenology · Physics 2010-01-28 Edi Halyo

We show that MSSM with three right handed neutrinos incorporating a renormalizable Type-I seesaw superpotential and no-scale SURGA K\"{a}hler potential can lead to a Starobinsky kind of inflation potential along a flat direction associated…

High Energy Physics - Phenomenology · Physics 2018-08-15 Ila Garg , Subhendra Mohanty

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

Inflation creates perturbations for the large scale structures in the universe, but it also dilutes everything. Therefore it is pertinent that the end of inflation must explain how to excite the Standard Model {\it dof} along with the dark…

High Energy Physics - Phenomenology · Physics 2013-07-22 Lingfei Wang , Ernestas Pukartas , Anupam Mazumdar

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…

High Energy Physics - Phenomenology · Physics 2025-11-05 Gui-Jun Ding , Si-Yi Jiang , Yong Xu , Wenbin Zhao

We explore in the supergravity context the possibility that a Higgs scalar may drive inflation via a non-minimal coupling to gravity characterised by a large dimensionless coupling constant. We find that this scenario is not compatible with…

High Energy Physics - Phenomenology · Physics 2014-11-20 Martin B Einhorn , D R Timothy Jones

It is shown that in the phenomenologically realistic supersymmetric $B-L$ MSSM theory, a linear combination of the neutral, up Higgs field with the third family left-and right-handed sneutrinos can play the role of the cosmological…

High Energy Physics - Phenomenology · Physics 2017-02-15 Rehan Deen , Burt A. Ovrut , Austin Purves