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相关论文: Light inflaton after LHC8 and WMAP9 results

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A new modified string-inspired modular invariant supergravity model is proposed and is applied to realize the slow roll inflation in Einstein frame. Because inflation deals with Planck scale physics, the dilaton can be a strong candidate…

高能物理 - 唯象学 · 物理学 2011-04-22 Mitsuo J. Hayashi , Yuta Koshimizu , Toyokazu Fukuoka , Kenji Takagi , Hikoya Kasari

We consider a minimal supersymmetric extension of the Standard Model, with right-handed neutrinos and local B-L, the difference between baryon and lepton number, a symmetry which is spontaneously broken at the scale of grand unification. To…

高能物理 - 唯象学 · 物理学 2015-04-09 Wilfried Buchmüller , Valerie Domcke , Kohei Kamada , Kai Schmitz

We study the decay of scalar fields, in particular the inflaton, into lighter scalars in a De Sitter spacetime background. After providing a practical definition of the rate, we focus on the case of an inflaton interacting with a massless…

高能物理 - 唯象学 · 物理学 2011-04-15 D. Boyanovsky , R. Holman , S. Prem Kumar

We consider a model of baryogenesis based on adding lepton number-violating quadratic mass terms to the inflaton potential of a non-minimally coupled inflation model. The $L$-violating mass terms generate a lepton asymmetry in a complex…

高能物理 - 唯象学 · 物理学 2023-07-12 Kit Lloyd-Stubbs , John McDonald

We propose a class of models in which a stable inflaton is produced as a thermal relic in the early universe and constitutes the dark matter. We show that inflaton annihilations can efficiently reheat the universe, and identify several…

高能物理 - 唯象学 · 物理学 2019-03-13 Dan Hooper , Gordan Krnjaic , Andrew J. Long , Samuel D. McDermott

We propose a minimal extension of the standard model of particle physics to accommodate cosmic inflation, dark matter and light neutrino masses. While the inflationary phase is obtained from a modified chaotic inflation scenario, consistent…

高能物理 - 唯象学 · 物理学 2020-04-15 Debasish Borah , Dibyendu Nanda , Abhijit Kumar Saha

We consider the decay of the inflaton in Starobinsky-like models arising from either an $R+R^2$ theory of gravity or $N=1$ no-scale supergravity models. If Standard Model matter is simply introduced to the $R + R^2$ theory, the inflaton…

高能物理 - 唯象学 · 物理学 2024-04-24 Yohei Ema , Marcos A. G. Garcia , Wenqi Ke , Keith A. Olive , Sarunas Verner

An extension of the Standard Model with three right-handed neutrinos and a simple invisible axion model can account for all experimentally confirmed signals of new physics (neutrino oscillations, dark matter and baryon asymmetry) in…

高能物理 - 唯象学 · 物理学 2019-02-06 Alberto Salvio

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…

高能物理 - 唯象学 · 物理学 2007-05-23 Laura Covi

The previously proposed modification of the standard (flat) inflationary $\Lambda CDM$ model in which the inflaton field(s) and ``dark energy" are replaced by the vacum in expanding Friedmann-Lema\^itre-Robertson-Walker Universe is studied.…

广义相对论与量子宇宙学 · 物理学 2026-03-24 Robert Alicki

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical abelian projection and centerization. The underlying gauge symmetry is…

高能物理 - 唯象学 · 物理学 2007-05-23 Ralf Hofmann , Mathias Th. Keil

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

The inflationary phase of the Universe is explored by proposing a toy model related to the scalar field, termed as {\it inflaton}. The potential part of the energy density in the said era is assumed to have a constant vacuum energy density…

综合物理 · 物理学 2019-05-22 Indranath Bhattacharyya , Saibal Ray , Prasenjit Paul

Within the $SP(2,R)$ symmetry, the Two-time model (2T model) has six dimensions with two dimensions of time and the dilaton field that can be identified as inflaton in a warm inflation scenario with potential of the form $\sim\phi^4$. From…

高能物理 - 唯象学 · 物理学 2022-10-07 Vo Quoc Phong , Ngo Phuc Duc Loc

We provide an update on five relatively well motivated inflationary models in which the inflaton is a Standard Model singlet scalar field. These include i) the textbook quadratic and quartic potential models but with additional couplings of…

高能物理 - 唯象学 · 物理学 2016-04-28 Nobuchika Okada , Vedat Nefer Şenoğuz , Qaisar Shafi

We propose a minimal setup that realises dynamical inflection point inflation, and, using the same field content, generates neutrino masses, a baryon asymmetry of the universe, and dark matter. A dark $SU(2)_D$ gauge sector with a dark…

高能物理 - 唯象学 · 物理学 2024-02-15 Debasish Borah , Arnab Dasgupta , Daniel Stolarski

We place functional constraints on the shape of the inflaton potential from the cosmic microwave background through a variant of the generalized slow roll approximation that allows large amplitude, rapidly changing deviations from…

宇宙学与河外天体物理 · 物理学 2010-09-01 Cora Dvorkin , Wayne Hu

We propose a mechanism by which the inflaton can generate baryogenesis, by taking the inflaton to be a complex scalar field with a weakly broken global symmetry and present a new version of the Affleck-Dine mechanism. The smallness of the…

高能物理 - 唯象学 · 物理学 2014-04-02 Mark P. Hertzberg , Johanna Karouby

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…

高能物理 - 唯象学 · 物理学 2021-09-08 Oleg Lebedev , Jong-Hyun Yoon

We show that a corpuscular description of gravity can lead to an inflationary scenario similar to Starobinsky's model without requiring the introduction of the inflaton field. All relevant properties are determined by the number of…

广义相对论与量子宇宙学 · 物理学 2018-10-30 Roberto Casadio , Andrea Giugno , Andrea Giusti