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Connecting inflation with neutrino physics through non-thermal leptogenesis via direct inflaton-right-handed neutrino (RHN) coupling naturally incorporates neutrino reheating, leaving no ambiguity regarding the early history of the…

高能物理 - 唯象学 · 物理学 2025-07-10 Xinyi Zhang

We study the impact of a temperature-dependent curvaton decay rate on the primordial curvature perturbation generated in the curvaton scenario. Using the familiar sudden decay approximation, we obtain an analytical expression for the…

宇宙学与河外天体物理 · 物理学 2015-06-22 Naoya Kitajima , David Langlois , Tomo Takahashi , Tomohiro Takesako , Shuichiro Yokoyama

We propose a model for early universe cosmology without the need for fundamental scalar fields. Cosmic acceleration and phenomenologically viable reheating of the universe results from a series of energy transitions, where during each…

高能物理 - 理论 · 物理学 2008-11-26 Scott Watson , Malcolm J. Perry , Gordon L. Kane , Fred C. Adams

Optomechanical systems explore and exploit the coupling between light and the mechanical motion of matter. A nonlinear coupling offers access to rich new physics, in both the quantum and classical regimes. We investigate a dynamic, as…

量子物理 · 物理学 2016-10-26 P. Z. G. Fonseca , E. B. Aranas , J. Millen , T. S. Monteiro , P. F. Barker

Reheating is a transition era after the end of inflation, during which the inflaton is converted into the particles that populate the Universe at later times. No direct cosmological observables are normally traceable to this period of…

宇宙学与河外天体物理 · 物理学 2015-06-23 Jessica L. Cook , Emanuela Dimastrogiovanni , Damien A. Easson , Lawrence M. Krauss

We discuss inflation and dark matter in the inert doublet model coupled non-minimally to gravity where the inert doublet is the inflaton and the neutral scalar part of the doublet is the dark matter candidate. We calculate the various…

高能物理 - 唯象学 · 物理学 2017-11-16 Sandhya Choubey , Abhass Kumar

We study density perturbations, including their non-Gaussianity, in models in which the decay rate of the curvaton depends on another light scalar field, denoted the modulaton. Although this model shares some similarities with the standard…

宇宙学与河外天体物理 · 物理学 2015-06-12 David Langlois , Tomo Takahashi

We study both oscillating and inflating curvaton scenarios when the curvaton mechanism is caused by a hybrid potential. The source of the curvature perturbation is the inhomogeneous phase transition that causes the modulation of the onset…

高能物理 - 唯象学 · 物理学 2013-05-30 Konstantinos Dimopoulos , Kazunori Kohri , Tomohiro Matsuda

We present detailed calculations at the basis of our recent proposal for simultaneous cooling the rotational, vibrational and external molecular degrees of freedom. In this method, the molecular rovibronic states are coupled by an intense…

We consider the possibility of a gravitationally induced particle production through the mechanism of a nonminimal curvature-matter coupling. An interesting feature of this gravitational theory is that the divergence of the energy-momentum…

广义相对论与量子宇宙学 · 物理学 2015-08-31 Tiberiu Harko , Francisco S. N. Lobo , José P. Mimoso , Diego Pavón

We propose a two-phase reheating scenario where the initial preheating dynamics is described by an effective dynamics followed by the standard perturbative reheating. Some of the important universal results of lattice simulation during…

高能物理 - 理论 · 物理学 2020-11-05 Md Riajul Haque , Debaprasad Maity , Pankaj Saha

We show that a minimal scenario, utilizing only the graviton as an intermediate messenger between the inflaton, the dark sector and the Standard Model (SM), is able to generate $simultaneously$ the observed relic density of dark matter…

高能物理 - 唯象学 · 物理学 2023-01-04 Basabendu Barman , Simon Cléry , Raymond T. Co , Yann Mambrini , Keith A. Olive

We carry out a comprehensive analysis of the simplest curvaton model, which is based on two non-interacting massive fields. Our analysis encompasses cases where the inflaton and curvaton both contribute to observable perturbations, and…

宇宙学与河外天体物理 · 物理学 2014-08-13 Christian T. Byrnes , Marina Cortês , Andrew R. Liddle

We consider the non-equilibrium evolution of the inflaton field coupled to both lighter scalars and fermions. The dissipational dynamics of this field is studied and found to be quite different than that believed in inflationary models. In…

高能物理 - 唯象学 · 物理学 2009-09-25 D. Boyanovsky , M. D'Attanasio , H. J. de Vega , R. Holman , D. S. -Lee , A. Singh

We have tested some simple quintessential inflation models, imposing that they match with the recent observational data provided by the BICEP and Planck's team and leading to a reheating temperature, which is obtained via gravitational…

广义相对论与量子宇宙学 · 物理学 2017-11-28 Llibert Aresté Saló , Jaume de Haro

We analyze the dynamics of models of warm inflation with general dissipative effects. We consider phenomenological terms both for the inflaton decay rate and for viscous effects within matter. We provide a classification of the asymptotic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Jose P. Mimoso , Ana Nunes , Diego Pavon

We extend an earlier semiclassical model to describe the dissipative motion of N atoms coupled to M modes inside a coherently driven high-finesse cavity. The description includes momentum diffusion via spontaneous emission and cavity decay.…

量子物理 · 物理学 2009-11-07 Peter Horak , Helmut Ritsch

We consider a novel cosmological scenario in which a curvaton is long-lived and plays the role of cold dark matter (CDM) in the presence of a short, secondary inflation. Non-trivial evolution of the large scale cosmological perturbation in…

高能物理 - 唯象学 · 物理学 2017-04-17 Jinn-Ouk Gong , Naoya Kitajima , Takahiro Terada

A new modified string-inspired modular invariant supergravity model is proposed and is applied to realize the slow roll inflation in Einstein frame, so that the model explains WMAP observations very well. Gravitino mass and their production…

高能物理 - 唯象学 · 物理学 2010-11-23 Yuta Koshimizu , Toyokazu Fukuoka , Kenji Takagi , Hikoya Kasari , Mitsuo J. Hayashi

In higher-curvature inflation models ($R+\alpha_n R^n$), we study a parametric preheating of a scalar field $\chi$ coupled non-minimally to a spacetime curvature $R$ ($\xi R \chi^2$). In the case of $R^2$-inflation model, efficient…

高能物理 - 唯象学 · 物理学 2008-11-26 S. Tsujikawa , K. Maeda , T. Torii