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相关论文: Large Field Inflation in Supergravity

200 篇论文

We have constructed a large field N-flation model in the supergravity framework. In this simple set-up, N fields collectively drive inflation where each field traverses sub-Planckian field values. This has been realised with a…

高能物理 - 唯象学 · 物理学 2015-12-30 Kumar Das , Koushik Dutta

We study the possibility that inflation is driven by a scalar field together with a vector field minimally coupled to gravity. By assuming an effective potential that incorporates both fields into the action, we explore two distinct…

广义相对论与量子宇宙学 · 物理学 2024-12-09 Manuel Gonzalez-Espinoza , Ramon Herrera

We consider D-term hybrid inflation in the framework of superconformal supergravity. In part of the parameter space, inflation continues for subcritical inflaton field value. Consequently, a new type of inflation emerges, which gives…

宇宙学与河外天体物理 · 物理学 2018-06-04 Koji Ishiwata

We introduce a simple string model of inflation, in which the inflaton field can take trans-Planckian values while driving a period of slow-roll inflation. This leads naturally to a realisation of large field inflation, inasmuch as the…

高能物理 - 理论 · 物理学 2015-03-13 M. Cicoli , C. P. Burgess , F. Quevedo

We point out that the prediction of the minimal chaotic inflation model is altered if a scalar field takes a large field value close to the Planck scale during inflation due to a negative Hubble induced mass. In particular, we show that the…

高能物理 - 唯象学 · 物理学 2016-03-09 Keisuke Harigaya , Masahiro Ibe , Masahiro Kawasaki , Tsutomu T. Yanagida

We describe the coupling of matter fields to an inflationary sector of supergravity, the inflaton $\Phi$ and a stabilizer $S$, in models where the Kahler potential has a flat inflaton direction. Such models include, in particular, advanced…

高能物理 - 理论 · 物理学 2016-04-11 Renata Kallosh , Andrei Linde , Timm Wrase

The evolution of the quintessence field during a phase of chaotic inflation is studied. The inflaton and the quintesssence field are described in a supergravity framework where the coupling between the inflaton and quintessence is induced…

天体物理学 · 物理学 2008-11-26 Philippe Brax , Jerome Martin

We identify a new mechanism in supergravity theories which leads to successful inflation without any need for fine tuning. The simplest model yields a spectrum of density fluctuations tilted away from scale-invariance and negligible…

高能物理 - 唯象学 · 物理学 2014-11-17 Jennifer A. Adams , Graham G. Ross , Subir Sarkar

A new family of inflation models is introduced and studied. The models are characterised by a scalar potential which, far from the origin, approaches an inflationary plateau in a power-law manner, while near the origin becomes monomial, as…

高能物理 - 唯象学 · 物理学 2015-11-20 Konstantinos Dimopoulos

We describe a way to construct supergravity models with an arbitrary inflaton potential V ({\phi}) and show that all other scalar fields in this class of models can be stabilized at the inflationary trajectory by a proper choice of the…

高能物理 - 理论 · 物理学 2011-02-18 Renata Kallosh , Andrei Linde , Tomas Rube

We construct a class of single small field models of inflation that can predict, contrary to popular wisdom, an observable gravitational wave signal in the cosmic microwave background anisotropies. The spectral index, its running, the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Ido Ben-Dayan , Ram Brustein

We initiate the analysis of the inflationary dynamics in Weyl-invariant Einstein-Cartan gravity nonminimally coupled to the Standard Model of particle physics. We take the axion-like particle of gravitational origin to be heavy and show…

高能物理 - 唯象学 · 物理学 2025-07-23 Georgios K. Karananas , Mikhail Shaposhnikov , Sebastian Zell

We propose a new broad class of multi-field non-canonical inflationary models as an extension of multi-field conformal cosmological attractors. This also generalizes the recently discovered class of non-canonical conformal attractors for…

高能物理 - 理论 · 物理学 2020-03-17 Tony Pinhero , Supratik Pal

We propose a single field inflationary model by generalizing the inverse power law potential from the intermediate model. We study the implication of our model on the primordial anisotropy of cosmological microwave background radiation.…

高能物理 - 理论 · 物理学 2015-06-17 Zhun Lu

The Higgs field is an attractive candidate for the inflaton because it is an observationally confirmed fundamental scalar field. Importantly, it can be modeled by the most general renormalizable scalar potential. However, if the classical…

宇宙学与河外天体物理 · 物理学 2021-03-29 Martin Bojowald , Suddhasattwa Brahma , Sean Crowe , Ding Ding , Joseph McCracken

Large-field inflation in supergravity requires the approximate global symmetry needed to protect flatness of the scalar potential. In helical-phase inflation, the U(1) symmetry of the Kahler potential is assumed, the phase part of the…

高能物理 - 理论 · 物理学 2015-11-24 Sergei V. Ketov , Takahiro Terada

Models of inflation in which the Higgs field is non-minimally coupled to gravity lead, after a recaling of the metric, to a complicated expression for the potential of the inflaton field. Nevertheless, this potential produces the desired…

高能物理 - 理论 · 物理学 2022-06-08 Noureddine Mohammedi

We present viable F-term realizations of the hybrid inflationary scenario in the context of supergravity addressing at the same time the well-known problems of the initial conditions and of the adequate suppression of the inflaton mass. An…

高能物理 - 唯象学 · 物理学 2009-11-10 C. Panagiotakopoulos

Large-field inflation is an interesting and predictive scenario. Its non-trivial embedding in supergravity was intensively studied in the recent literature, whereas its interplay with supersymmetry breaking has been less thoroughly…

高能物理 - 理论 · 物理学 2015-06-22 Wilfried Buchmuller , Emilian Dudas , Lucien Heurtier , Clemens Wieck

We discuss inflation in models with large extra dimensions, driven by a bulk scalar field. The brane inflaton is then a single effective field, obtained from the bulk scalar field by scaling. The self interaction terms of the effective…

高能物理 - 唯象学 · 物理学 2008-11-26 R. N. Mohapatra , A. Pérez-Lorenzana , C. A. de S. Pires