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相关论文: Effective Field Theory of non-Attractor Inflation

200 篇论文

Primordial magnetic fields are generated during inflation by considering actions that break the conformal invariance of the electromagnetic field. To break the conformal invariance, the electromagnetic fields are coupled either to the…

宇宙学与河外天体物理 · 物理学 2022-06-22 Sagarika Tripathy , Debika Chowdhury , Rajeev Kumar Jain , L. Sriramkumar

We present a study of the Effective Field Theory (EFT) generalization of stochastic inflation in a model-independent single-field framework and its impact on primordial black hole (PBH) formation. We show how the Langevin equations for the…

宇宙学与河外天体物理 · 物理学 2025-02-24 Sayantan Choudhury , Ahaskar Karde , Pankaj Padiyar , M. Sami

It has recently been suggested that a strongly coupled phase of inflation may be described holographically in terms of a weakly coupled quantum field theory (QFT). Here, we explore the possibility that the wave function of an inflationary…

高能物理 - 理论 · 物理学 2015-06-15 Jaume Garriga , Yuko Urakawa

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

We formulate the Effective Field Theory (EFT) of perturbations within scalar-tensor theories on an inhomogeneous background. The EFT is constructed while keeping a background of a scalar field to be $\textit{timelike}$, which spontaneously…

高能物理 - 理论 · 物理学 2024-01-11 Shinji Mukohyama , Vicharit Yingcharoenrat

We investigate the phenomenon of second sound in various states of matter from the perspective of non-equilibrium effective field theory (EFT). In particular, for each state of matter considered, we find that at least two (though sometimes…

高能物理 - 理论 · 物理学 2021-05-04 Michael J. Landry

We present a detailed study of the trispectrum of the curvature perturbation generated within a stable, well defined and predictive theory which comprises an inflationary phase. In this model the usual shift symmetry is enhanced up to the…

宇宙学与河外天体物理 · 物理学 2016-04-18 Frederico Arroja , Nicola Bartolo , Emanuela Dimastrogiovanni , Matteo Fasiello

We study the problem of obtaining de Sitter and inflationary vacua from dimensional reduction of double field theory (DFT) on nongeometric string backgrounds. In this context, we consider a new class of effective potentials that admit…

高能物理 - 理论 · 物理学 2016-05-05 Falk Hassler , Dieter Lust , Stefano Massai

We study the production of observable primordial local non-Gaussianity in two opposite regimes of canonical single field inflation: attractor (standard single field slow-roll inflation) and non attractor (ultra slow-roll inflation). In the…

宇宙学与河外天体物理 · 物理学 2018-05-15 Rafael Bravo , Sander Mooij , Gonzalo A. Palma , Bastián Pradenas

Non-trivial inflaton self-interactions can yield calculable signatures of primordial non-Gaussianity that are measurable in cosmic surveys. Surprisingly, we find that the phase transition to slow-roll eternal inflation is often incalculable…

高能物理 - 理论 · 物理学 2023-05-10 Timothy Cohen , Daniel Green , Akhil Premkumar

We study the slow-roll single field inflation in the context of the consistent $D\to4$ Einstein-Gauss-Bonnet gravity that was recently proposed in \cite{Aoki:2020lig}. In addition to the standard attractor regime, we find a new attractor…

广义相对论与量子宇宙学 · 物理学 2021-05-03 Katsuki Aoki , Mohammad Ali Gorji , Shuntaro Mizuno , Shinji Mukohyama

Slow-roll inflation is studied as an effective field theory.We find as consistent form of the inflaton potential V(phi)=N M^4 w(phi/[sqrt{N}M_P]) where phi is the inflaton field, M the inflation energy scale, M_P the Planck mass, and N~50…

天体物理学 · 物理学 2009-11-13 D. Boyanovsky , H. J. de Vega , N. G. Sanchez

In this work we present the effective field theory of primordial statistical anisotropies generated during anisotropic inflation involving a background $U(1)$ gauge field. Besides the usual Goldstone boson associated with the breaking of…

宇宙学与河外天体物理 · 物理学 2016-03-23 Ali Akbar Abolhasani , Mohammad Akhshik , Razieh Emami , Hassan Firouzjahi

We study the two-field warm inflation models with a double quadratic potential and a linear temperature dependent dissipative coefficient. We derived the evolution equation of all kinds of perturbations without assuming slow-roll…

广义相对论与量子宇宙学 · 物理学 2019-05-23 Yang-yang Wang , Xiao-Min Zhang , Jian-Yang Zhu

We revisit inflation coupled with vector fields employing kinetic coupling in the comoving gauge. It is known that there is a cumulative effect $IN^2$ on the curvature power spectrum. For a large number of e-foldings $N$, this contribution…

宇宙学与河外天体物理 · 物理学 2024-12-02 Chong-Bin Chen

We study the power spectra and entropy of two-field warm inflationary scenario with canonical condition which is described by many-dimensional stochastic differential equations. The field perturbations are analytically calculated via a…

广义相对论与量子宇宙学 · 物理学 2019-03-12 Xi-Bin Li , Xiao-Gang Zheng , Jian-Yang Zhu

We analyse field fluctuations during an Ultra Slow-Roll phase in the stochastic picture of inflation and the resulting non-Gaussian curvature perturbation, fully including the gravitational backreaction of the field's velocity. By working…

广义相对论与量子宇宙学 · 物理学 2021-10-04 Tomislav Prokopec , Gerasimos Rigopoulos

We study the slow-roll inflation models, where the inflaton slow-rolls along a trajectory whose orthogonal directions are lifted by potentials with masses of order the Hubble parameter. In these models large non-Gaussianities can be…

宇宙学与河外天体物理 · 物理学 2010-04-06 Xingang Chen , Yi Wang

Recently, we introduced an ekpyrotic model based on a single, canonical scalar field that generates nearly scale invariant curvature fluctuations through a purely "adiabatic mechanism" in which the background evolution is a dynamical…

高能物理 - 理论 · 物理学 2011-06-13 Justin Khoury , Paul J. Steinhardt

Effective Field Theory (EFT) provides a powerful framework that exploits a separation of scales in physical systems to perform systematically improvable, model-independent calculations. Particularly interesting are few-body systems with…

其他凝聚态物理 · 物理学 2009-11-10 H. -W. Hammer