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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

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

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

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

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 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

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

A variation of sneutrino inflation based on chi^2 potential is considered where the inflaton and the late-decaying field are sneutrinos of different generations. The lighter, late-decaying sneutrino dilutes the gravitinos over-produced…

高能物理 - 唯象学 · 物理学 2019-10-11 Vedat Nefer Şenoğuz

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

We propose an extension of the standard model (SM) by two SU(2) triplet scalars and an inert SU(2) doublet. We demonstrate that this setup can simultaneously produce an inflaton and baryon asymmetry in the early universe, provide a dark…

高能物理 - 唯象学 · 物理学 2025-10-09 Sin Kyu Kang , Raymundo Ramos

We study non-Gaussianity, the spectral index of primordial scalar fluctuations and tensor modes in models where fluctuations from the inflaton and the curvaton can both contribute to the present cosmic density fluctuations. Even though…

天体物理学 · 物理学 2008-11-26 Kazuhide Ichikawa , Teruaki Suyama , Tomo Takahashi , Masahide Yamaguchi

We bring together some known ingredients beyond the Standard Model physics which can explain the hot Big Bang model with the observed baryon asymmetry and also the fluctuations in the cosmic microwave background radiation with a minimal set…

高能物理 - 唯象学 · 物理学 2008-11-26 Anupam Mazumdar , A. Pérez-Lorenzana

We propose that the observed baryon asymmetry of the Universe can naturally arise from a net asymmetry generated in the sleptonic sector at fairly low reheat temperatures. The best candidate is indeed the right-handed sneutrino. The initial…

高能物理 - 唯象学 · 物理学 2009-11-10 Rouzbeh Allahverdi , Bhaskar Dutta , Anupam mazumdar

We consider a right-handed scalar neutrino as the inflaton which carries a gravitational coupling with a supersymmetric QCD sector responsible for breaking supersymmetry dynamically. The framework suggests an inflaton potential which is a…

高能物理 - 唯象学 · 物理学 2016-01-20 Abhijit Kumar Saha , Arunansu Sil

We discuss resonant leptogenesis arising from the decays of two nearly-degenerate right-handed neutrinos, identified as the inflaton and stabiliser superfields in a model of chaotic sneutrino inflation. We compare an analytical estimate of…

高能物理 - 唯象学 · 物理学 2017-02-28 Fredrik Björkeroth , Stephen F. King , Kai Schmitz , Tsutomu T. Yanagida

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 propose a simple framework to split neutrinos with a slight departure from tribimaximal mixing - where two of the neutrinos are Majorana type which provide thermal leptogenesis. The Dirac neutrino with a tiny Yukawa coupling explains…

高能物理 - 唯象学 · 物理学 2013-05-30 Anupam Mazumdar , Stefano Morisi

Modifications to the Friedmann equation in brane cosmology can have important implications for early universe phenomena such as inflation and the generation of the baryon asymmetry. In the framework of braneworld cosmology, we discuss a…

高能物理 - 唯象学 · 物理学 2017-08-23 N. M. C. Santos , M. C. Bento , R. González Felipe

We consider the scotogenic model, where the standard model (SM) is extended by a scalar doublet and three $Z_2$ odd SM-singlet fermions ($N_i$, $i=1,2,3$), all odd under an additional $Z_2$ symmetry, as a unifying framework for simultaneous…

高能物理 - 唯象学 · 物理学 2019-03-13 Debasish Borah , P. S. Bhupal Dev , Abhass Kumar

We consider a new physics model, where the Standard Model (SM) is extended by hyperchargeless $Y=0$ triplet fermions and Higgs triplet with hypercharge $Y=2$. The first two generation fermion triplets are even under the $Z_2$…

高能物理 - 唯象学 · 物理学 2023-04-21 Pritam Das , Najimuddin Khan
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