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The motion of a pseudo-scalar field $X$ during inflation naturally induces a significant amplification of the gauge fields to which it is coupled. The amplified gauge fields can source characteristic scalar and tensor primordial…

宇宙学与河外天体物理 · 物理学 2016-09-21 Marco Peloso , Lorenzo Sorbo , Caner Unal

Processes of particle production during inflation can increase the amplitude of the scalar metric perturbations. We show that such a mechanism can naturally arise in supergravity models where an axion-like field, whose potential is…

高能物理 - 唯象学 · 物理学 2021-07-07 Michael A. Roberts , Lorenzo Sorbo

We investigate classical and quantum correlations of a quantum field in the inflationary universe using a particle detector model. By considering the entanglement and correlations between two comoving detectors interacting with a scalar…

广义相对论与量子宇宙学 · 物理学 2011-09-08 Yasusada Nambu , Yuji Ohsumi

Simple monomial inflationary scenarios have been ruled out by recent observations. In this work we revisit the next simplest scenario, a single--field model where the scalar potential is a polynomial of degree four which features a concave…

宇宙学与河外天体物理 · 物理学 2022-12-14 Manuel Drees , Yong Xu

We analyze a massive vector field with a non-canonical kinetic term in the action, minimally coupled to gravity, where the mass and kinetic function of the vector field vary as functions of time during inflation. The vector field is…

宇宙学与河外天体物理 · 物理学 2013-07-25 Andres A. Navarro , Yeinzon Rodriguez

Light vector fields during inflation obtain a superhorizon perturbation spectrum when their conformal invariance is appropriately broken. Such perturbations, by means of some suitable mechanism (e.g. the vector curvaton mechanism), can…

高能物理 - 唯象学 · 物理学 2015-06-16 Juan C. Bueno Sanchez , Konstantinos Dimopoulos

Attention has focussed recently on models of inflation that involve a second or more fields with a mass near the inflationary Hubble parameter $H$, as may occur in supersymmetric theories if the supersymmetry-breaking scale is not far from…

宇宙学与河外天体物理 · 物理学 2016-02-17 Emanuela Dimastrogiovanni , Matteo Fasiello , Marc Kamionkowski

We compute the large scalar four-point correlation functions in general single field inflation models, where the inflaton Lagrangian is an arbitrary function of the inflaton and its first derivative. We find that the leading order…

宇宙学与河外天体物理 · 物理学 2010-05-28 Xingang Chen , Bin Hu , Min-xin Huang , Gary Shiu , Yi Wang

We construct the global phase portraits of inflationary dynamics in teleparallel gravity models with a scalar field nonminimally coupled to torsion scalar. The adopted set of variables can clearly distinguish between different asymptotic…

广义相对论与量子宇宙学 · 物理学 2022-03-03 Laur Järv , Joosep Lember

We present a minimal axion inflation model which can generate a large tensor-to-scalar ratio while remaining sub-Planckian. The modulus of a complex scalar field $\Phi$ with a $\lambda |\Phi|^4$ potential couples directly to the gauge field…

高能物理 - 唯象学 · 物理学 2015-06-22 John McDonald

Inflation in cosmology is a specific stage preceding the Big Bang, aimed at solving both old background problems and new perturbation issues. Single-field inflation is a candidate to illustrate the picture of the initial universe, and…

宇宙学与河外天体物理 · 物理学 2025-05-21 Guanqiao Liu

We explore the possibility of obtaining inflation in weakly coupled heterotic string theory, where the model dependent axions are responsible for driving inflation. This model can be considered as a certain extrapolation of…

高能物理 - 理论 · 物理学 2010-10-27 Martin E. Olsson

We study the multifield dynamics of axion models nonminimally coupled to gravity. As usual, we consider a canonical $U(1)$ symmetry-breaking model in which the axion is the phase of a complex scalar field. If the complex scalar field has a…

高能物理 - 理论 · 物理学 2024-06-07 Evan McDonough , Alan H. Guth , David I. Kaiser

In inflationary scenarios with more than one scalar field, inflation may proceed even if each of the individual fields has a potential too steep for that field to sustain inflation on its own. We show that scalar fields with exponential…

天体物理学 · 物理学 2010-01-06 Andrew R Liddle , Anupam Mazumdar , Franz E Schunck

The representation theory of de Sitter space allows for a category of partially massless particles which have no flat space analog, but could have existed during inflation. We study the couplings of these exotic particles to inflationary…

高能物理 - 理论 · 物理学 2018-05-23 Daniel Baumann , Garrett Goon , Hayden Lee , Guilherme L. Pimentel

The parity-odd four-point function provides a unique probe of fundamental symmetries and potential new physics in the large-scale structure of the Universe. We present measurements of the parity-odd four-point function using the DESI DR1…

We propose a method that provides an observational signature of the quantum origin of primordial fluctuations generated during inflation. The method gives a prescription for testing a Bell inequality constructed exclusively from the…

宇宙学与河外天体物理 · 物理学 2026-03-30 Pablo Tejerina-Pérez , Leonid Sarieddine , Daniele Bertacca , Raul Jimenez

The effective field theory (EFT) of inflation provides an essential picture to explore the effects of the unknown high energy physics in the single scalar field inflation models. For a generic EFT of inflation, possible high energy…

广义相对论与量子宇宙学 · 物理学 2019-12-03 Guang-Hua Ding , Jin Qiao , Qiang Wu , Tao Zhu , Anzhong Wang

In models of inflation driven by an axion-like pseudoscalar field, the inflaton, a, may couple to the standard model hypercharge via a Chern-Simons-type interaction, $L \subset a/(4\Lambda) F\tilde{F}$. This coupling results in explosive…

高能物理 - 唯象学 · 物理学 2017-12-20 Daniel Jimenez , Kohei Kamada , Kai Schmitz , Xun-Jie Xu

We study the linear perturbation of the recently proposed model of inflation where a uniform gauge-kinetic coupling of the inflaton to multiple vector fields breaks the cosmic no-hair conjecture while maintaining the isotropy. We derive the…

宇宙学与河外天体物理 · 物理学 2012-10-09 Kei Yamamoto