中文
相关论文

相关论文: Moduli and multi-field inflation

200 篇论文

The calculation of scalar gravitational and matter perturbations during multiple-field inflation valid to first order in slow roll is discussed. These fields may be the coordinates of a non-trivial field manifold and hence have non-minimal…

高能物理 - 唯象学 · 物理学 2007-05-23 B. J. W. van Tent , S. Groot Nibbelink

High-scale string inflationary models are in well-known tension with low-energy supersymmetry. A promising solution involves models where the inflaton is the volume of the extra dimensions so that the gravitino mass relaxes from large…

高能物理 - 理论 · 物理学 2016-01-20 Michele Cicoli , Francesco Muia , Francisco Gil Pedro

Inflation offers a simple model for very early evolution of our Universe and the origin of primordial perturbations on large scales. Over the last 25 years we have become familiar with the predictions of single-field models, but inflation…

天体物理学 · 物理学 2008-11-26 David Wands

We propose a simple but effective mechanism to realize an inflationary early universe consistent with the observed WMAP, Planck and/or BICEP2 data, which would be incorporated in various supersymmetric models of elementary particles…

高能物理 - 理论 · 物理学 2015-06-19 Hiroyuki Abe , Hajime Otsuka

Inflation universally produces classical almost scale free Gaussian inhomogeneities of any light scalars. Assuming the coupling constants at the time of inflation depend on some light moduli fields, we encounter the generation of modulated…

天体物理学 · 物理学 2009-11-10 Francis Bernardeau , Lev Kofman , Jean-Philippe Uzan

Multifield models of inflation with nonminimal couplings are in excellent agreement with the recent results from {\it Planck}. Across a broad range of couplings and initial conditions, such models evolve along an effectively single-field…

宇宙学与河外天体物理 · 物理学 2014-01-08 David I. Kaiser , Evangelos I. Sfakianakis

We consider the spectrum of primordial fluctuations produced by inflationary models where the inflaton potential is the sum of two exponential terms. A wide range of spectra result, with the only constraint being that the scalar spectrum…

天体物理学 · 物理学 2009-09-25 Richard Easther

Dynamical models of inflation are given with composite inflatons by means of massive supersymmetric gauge theory. Nearly flat directions and stable massive ones in the potential are identified and slow-roll during inflation is examined.…

高能物理 - 唯象学 · 物理学 2008-11-26 K. Hamaguchi , K. -I. Izawa , H. Nakajima

Models of cosmic inflation suggest that our universe underwent an early phase of accelerated expansion, driven by the dynamics of one or more scalar fields. Inflationary models make specific, quantitative predictions for several observable…

宇宙学与河外天体物理 · 物理学 2016-05-10 David I. Kaiser

We study slow-roll inflation model controlled by the modular flavor symmetry. In the model, the modulus field plays a role of inflaton and the introduction of the stabilizer field coupled to a modular form in the superpotential produces the…

高能物理 - 唯象学 · 物理学 2023-07-26 Yoshihiko Abe , Tetsutaro Higaki , Fumiya Kaneko , Tatsuo Kobayashi , Hajime Otsuka

Most models of inflation have small parameters, either to guarantee sufficient inflation or the correct magnitude of the density perturbations. In this paper we show that, in supersymmetric theories with weak scale supersymmetry breaking,…

高能物理 - 唯象学 · 物理学 2007-05-23 Lisa Randall , Marin Soljacic , Alan Guth

Most models of inflation have small parameters, either to guarantee sufficient inflation or the correct magnitude of the density perturbations. In this paper we show that, in supersymmetric theories with weak scale supersymmetry breaking,…

高能物理 - 唯象学 · 物理学 2009-09-15 Lisa Randall , Marin Soljacic , Alan Guth

We develop a new class of chaotic inflation models with spontaneously broken conformal invariance. Observational consequences of a broad class of such models are stable with respect to strong deformations of the scalar potential. This…

高能物理 - 理论 · 物理学 2015-06-16 Renata Kallosh , Andrei Linde

Curvature perturbations generated after the end of inflation are estimated for a generic multi-field inflationary potential. The curvature perturbations are generated by conversion of inflationary isocurvature perturbations, similar to…

天体物理学 · 物理学 2007-05-23 Andrei Gruzinov

We study multifield contributions to the scalar power spectrum in an ensemble of six-field inflationary models obtained in string theory. We identify examples in which inflation occurs by chance, near an approximate inflection point, and we…

宇宙学与河外天体物理 · 物理学 2015-06-05 Liam McAllister , Sébastien Renaux-Petel , Gang Xu

We describe a broad class of multi-field inflationary models with spontaneously broken conformal invariance. It generalizes the recently discovered class of cosmological attractors with a single inflaton field. In the new multi-field…

高能物理 - 理论 · 物理学 2015-06-17 Renata Kallosh , Andrei Linde

Non-abelian discrete gauge symmetries can provide the inflaton with a flat potential even when one takes into account gravitational strength effects. The discreteness of the symmetries also provide special field values where inflation can…

高能物理 - 唯象学 · 物理学 2009-10-31 E. D. Stewart , J. D. Cohn

We study the generation of the primordial curvature perturbation in multi-field inflation. Considering both the evolution of the perturbation during inflation and the effects generated at the end of inflation, we present a general formula…

宇宙学与河外天体物理 · 物理学 2015-06-04 Ki-Young Choi , Soo A Kim , Bumseok Kyae

We propose new classes of inflation models based on the modular symmetry, where the modulus field $\tau$ serves as the inflaton. We establish a connection between modular inflation and modular stabilization, wherein the modulus field rolls…

高能物理 - 唯象学 · 物理学 2024-10-21 Gui-Jun Ding , Si-Yi Jiang , Wenbin Zhao

In effective supergravity theories following from the superstring, a modulus field can quite naturally set the neccessary initial conditions for successful cosmological inflation to be driven by a hidden sector scalar field. The leading…

高能物理 - 唯象学 · 物理学 2007-05-23 Subir Sarkar