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相关论文: Sneutrino Inflation with $\alpha$-attractors

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The model of RH neutrino fields coupled to the MSSM is shown to yield a large parameter regime of warm inflation. In the strong dissipative regime, it is shown that inflation, driven by a single sneutrino field, occurs with {\it all field…

高能物理 - 唯象学 · 物理学 2011-08-17 Mar Bastero-Gil , Arjun Berera

In sneutrino hybrid inflation the superpartner of one of the right-handed neutrinos involved in the seesaw mechanism plays the role of the inflaton field. It obtains its large mass after the "waterfall" phase transition which ends hybrid…

高能物理 - 唯象学 · 物理学 2010-10-27 Stefan Antusch , Jochen P. Baumann , Valerie F. Domcke , Philipp M. Kostka

Motivated by the coincidence between the Hubble scale during inflation and the typical see-saw neutrino mass scale, we present a supergravity model where the inflaton is identified with a linear combination of right-handed sneutrino fields.…

高能物理 - 唯象学 · 物理学 2015-07-29 Jason L. Evans , Tony Gherghetta , Marco Peloso

We review the scenario of sneutrino hybrid inflation, where one of the singlet sneutrinos, the superpartners of the right-handed neutrinos, plays the role of the inflaton. In a minimal model of sneutrino hybrid inflation, the spectral index…

高能物理 - 唯象学 · 物理学 2009-11-11 Stefan Antusch

We reconsider the possibility that inflation was driven by a sneutrino - the scalar supersymmetric partner of a heavy singlet neutrino - in the minimal seesaw model of neutrino masses. We show that this model is consistent with data on the…

高能物理 - 唯象学 · 物理学 2009-09-11 J. Ellis , M. Raidal , T. Yanagida

The onset of inflation in hybrid models require fine tuning in the initial conditions. The inflaton field should have an initial value close to the Planck scale $M_{P}$, whereas the auxiliary "orthogonal" field must be close to zero with an…

高能物理 - 唯象学 · 物理学 2009-11-07 Zurab Berezhiani , Anupam Mazumdar , Abdel Pérez-Lorenzana

We propose a cosmological framework in which neutrino masses evolve dynamically through coupling with a scalar field that simultaneously drives inflation. The neutrino mass is modeled as a power-law, exponential, or hybrid function of the…

宇宙学与河外天体物理 · 物理学 2025-12-01 Hemanshi Bundeliya , Gaurav Bhandari , S. D. Pathak , V. K. Sharma

We present a successful realization of sneutrino tribrid inflation model based on a gauged $U(1)_{B-L}$ extension of Minimal Supersymmetric Standard Model (MSSM). A single interaction term involving the $B-L$ Higgs field and the…

高能物理 - 唯象学 · 物理学 2021-11-18 Muhammad Atif Masoud , Mansoor Ur Rehman , Qaisar Shafi

The seesaw model of neutrinos might explain the size, age, flatness and near-homogeneity of the Universe via sneutrino inflation, as well as explaining the origin of matter via leptogenesis. The sneutrino inflation hypothesis makes…

高能物理 - 唯象学 · 物理学 2008-11-26 John Ellis

We show that the scalar field that drives inflation can have a dynamical origin, being a strongly coupled right handed neutrino condensate. The resulting model is phenomenologically tightly constrained, and can be experimentally (dis)probed…

高能物理 - 唯象学 · 物理学 2009-03-31 Gabriela Barenboim

We consider sneutrino inflation and post-inflation cosmology in the singlet extension of the MSSM with approximate Peccei-Quinn(PQ) symmetry, assuming that supersymmetry breaking is mediated by gauge interaction. The PQ symmetry is broken…

高能物理 - 唯象学 · 物理学 2011-09-09 Yeong Gyun Kim , Hyun Min Lee , Wan-Il Park

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…

高能物理 - 唯象学 · 物理学 2017-02-15 Rehan Deen , Burt A. Ovrut , Austin Purves

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 propose a chaotic inflation model in which the lightest right-handed sneutrino serves as the inflaton and the predicted values of the spectral index and tensor-to-scalar ratio are consistent with the Planck data. Interestingly, the…

高能物理 - 唯象学 · 物理学 2014-01-28 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We propose a hybrid inflation scenario in which the singlet sneutrino, the superpartner of the right-handed neutrino, plays the role of the inflaton. We study a minimal model of sneutrino hybrid inflation in supergravity, where we find a…

高能物理 - 唯象学 · 物理学 2008-11-26 Stefan Antusch , Mar Bastero-Gil , Steve F. King , Qaisar Shafi

Inflationary models based on a single scalar field $\phi$ with a quadratic potential $V = \frac{1}{2} m^2 \phi^2$ are disfavoured by the recent Planck constraints on the scalar index, $n_s$, and the tensor-to-scalar ratio for cosmological…

宇宙学与河外天体物理 · 物理学 2014-03-05 John Ellis , Malcolm Fairbairn , Maria Sueiro

We consider an extension of nuMSSM with an extra U(1) that realizes D-term inflation driven by the right-handed sneutrino. Non-renormalizable terms in the Kahler potential and the superpotential are considered, the latter controlled by a…

高能物理 - 唯象学 · 物理学 2014-11-20 O. Efthimiou , K. Tamvakis

The smallness of the neutrino masses may be related to inflation. The minimal supersymmetric Standard Model (MSSM) with small Dirac neutrino masses already has all the necessary ingredients for a successful inflation. In this model the…

高能物理 - 唯象学 · 物理学 2010-10-27 Rouzbeh Allahverdi , Alexander Kusenko , Anupam Mazumdar

We propose a scenario for realizing inflation in the framework of supersymmetric B-L extension of the Standard Model. We find that one of the associated right-handed sneutrinos (the superpartner of the Standard Model singlet fermion) can…

高能物理 - 唯象学 · 物理学 2013-05-29 Shaaban Khalil , Arunansu Sil

We investigate a scenario where the supersymmetric partners of two right-handed neutrinos (sneutrinos) work as mixed inflaton and curvaton, motivated by the fact that the curvaton contribution to scalar perturbations can reduce the…

高能物理 - 唯象学 · 物理学 2018-06-13 Naoyuki Haba , Tomo Takahashi , Toshifumi Yamada
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