中文
相关论文

相关论文: Hypernatural inflation

200 篇论文

Cosmological $\alpha$-attractors stand out as particularly compelling models to describe inflation in the very early universe, naturally meeting tight observational bounds from cosmic microwave background (CMB) experiments. We investigate…

宇宙学与河外天体物理 · 物理学 2022-06-22 Laura Iacconi , Hooshyar Assadullahi , Matteo Fasiello , David Wands

We study stochastic inflation in the presence of a dynamical gravitational constant. We describe the Arnowitt--Deser--Misner formalism for Jordan--Brans--Dicke theory of gravity with an inflaton field. The inflaton and dilaton scalar fields…

天体物理学 · 物理学 2009-10-22 Juan Garcia-Bellido

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 2009-11-07 Ralf Hofmann , Mathias Th. Keil

It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing during inflation, can be responsible for the generation of the curvature perturbation in the Universe. Particle production is studied and it…

高能物理 - 唯象学 · 物理学 2008-11-26 Konstantinos Dimopoulos

We suggest a new type of hill-top inflation originating from the initial conditions in the form of the microcanonical density matrix for the cosmological model with a large number of quantum fields conformally coupled to gravity. Initial…

高能物理 - 理论 · 物理学 2016-01-27 A. O. Barvinsky , A. Yu. Kamenshchik , D. V. Nesterov

The model of Natural Inflation is examined in light of recent 3-year data from the Wilkinson Microwave Anisotropy Probe and shown to provide a good fit. The inflaton potential is naturally flat due to shift symmetries, and in the simplest…

高能物理 - 唯象学 · 物理学 2008-11-26 Christopher Savage , Katherine Freese , William H. Kinney

String scenarios generically predict that we live in a so called axiverse: the Universe with about a hundred of light axion species which are decoupled from the Standard Model particles. However, the axions can couple to the inflaton which…

高能物理 - 唯象学 · 物理学 2017-06-28 Dmitry Gorbunov , Anna Tokareva

We show how successful supersymmetric hybrid inflation is realized in realistic models where the resolution of the minimal supersymmetric standard model mu problem is intimately linked with axion physics. The scalar fields that accompany…

高能物理 - 唯象学 · 物理学 2017-04-05 G. Lazarides , C. Panagiotakopoulos , Q. Shafi

Natural inflation relies on the existence of an axion decay constant which is super-Planckian. In string theory only sub-Planckian axion decay constants have been found in any controlled regime. However in field theory it is possible to…

高能物理 - 理论 · 物理学 2015-08-10 Eran Palti

We investigate inflation models in Jordan frame supergravity, in which an inflaton non-minimally couples to the scalar curvature. By imposing the condition that an inflaton would have the canonical kinetic term in the Jordan frame, we…

高能物理 - 理论 · 物理学 2018-01-30 Ken'ichi Saikawa , Masahide Yamaguchi , Yasuho Yamashita , Daisuke Yoshida

Light scalar and pseudoscalar particles are compelling dark matter candidates, with a vast running experimental program to discover them. Previous studies have shown that these light fields can generate sizable isocurvature perturbations in…

高能物理 - 唯象学 · 物理学 2023-06-02 Andrea Caputo , Michael Geller , Giuseppe Rossi

The inflationary paradigm has enjoyed phenomenological success, however, a compelling particle physics realization is still lacking. The key obstruction is that the requirement of a suitably flat scalar potential is sensitive to…

高能物理 - 唯象学 · 物理学 2011-05-12 Neil Barnaby , Marco Peloso

Warm natural inflation is studied for the case of the original cosine potential. The radiation bath during inflation induces a dissipation (friction) rate in the equation of motion for the inflaton field, which can potentially reduce the…

广义相对论与量子宇宙学 · 物理学 2023-03-08 Gabriele Montefalcone , Vikas Aragam , Luca Visinelli , Katherine Freese

We analyse the dynamics of spinodal decomposition in inflationary cosmology using the closed time path formalism of out of equilibrium quantum field theory combined with the non-perturbative Hartree approximation. In addition to a general…

高能物理 - 唯象学 · 物理学 2009-10-31 D. Cormier , R. Holman

We investigate a constraint on reheating followed by alpha-attractor-type inflation (the E-model and T-model) from an observation of the spectral index n_s. When the energy density of the universe is dominated by an energy component with…

宇宙学与河外天体物理 · 物理学 2016-05-04 Yoshiki Ueno , Kazuhiro Yamamoto

We propose a minimal extension of the Standard Model with the Peccei-Quinn (PQ) scalar field and explain the relic density of the QCD axion through the kinetic misalignment with a relatively small axion decay constant. To this purpose, we…

高能物理 - 唯象学 · 物理学 2024-05-02 Hyun Min Lee , Adriana G. Menkara , Myeong-Jung Seong , Jun-Ho Song

A direct coupling between the inflaton and Standard Model gluons can dynamically raise the QCD confinement scale during inflation, making the axion temporarily heavy and suppressing axion isocurvature perturbations. As inflation proceeds,…

宇宙学与河外天体物理 · 物理学 2026-05-21 Katherine Freese , Evangelos I. Sfakianakis , Barmak Shams Es Haghi

Fibre inflation is a specific string theory construction based on the Large Volume Scenario that produces an inflationary plateau. We outline its relation to $\alpha$-attractor models for inflation, with the cosmological sector originating…

高能物理 - 理论 · 物理学 2018-04-04 Renata Kallosh , Andrei Linde , Diederik Roest , Alexander Westphal , Yusuke Yamada

In this work, we study constant-roll inflation driven by a scalar field with non-minimal derivative coupling to gravity, via the Einstein tensor. This model contains a free parameter, $\eta$, which quantifies the non-minimal derivative…

广义相对论与量子宇宙学 · 物理学 2019-10-23 A. Oliveros , Hernán E. Noriega

We show that the hybrid inflation is naturally realized in the framework of a supersymmetric axion model, which is consistent with the WMAP observation if the Peccei-Quinn symmetry breaking scale is around 10^{15}GeV. By solving the post…

高能物理 - 唯象学 · 物理学 2015-03-19 Masahiro Kawasaki , Naoya Kitajima , Kazunori Nakayama