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相关论文: Primordial fluctuations from nonlinear couplings

200 篇论文

In this letter we complete a previously introduced formalism to study the gauge-invariant metric fluctuations from a noncompact Kaluza-Klein theory of gravity, to study the evolution of the early universe. The evolution of both, metric and…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Agustin Membiela , Mauricio Bellini

In this paper, we suppose that the universe begins in a holographic thermal equilibrium phase with the diverged correlation length, and the phase transition to the radiation phase of standard cosmology goes with the abrupt reducing of…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Yun-Song Piao

We study the implications of deformed quantum algebras for the generation of primordial perturbations from slow-roll inflation. Specifically, we assume that the quantum commutator of the inflaton's amplitude and momentum in Fourier space…

宇宙学与河外天体物理 · 物理学 2015-06-17 Andrew C. Day , Iain A. Brown , Sanjeev S. Seahra

We present a gauge invariant formalism to study the evolution of curvature perturbations during decay of the inflaton or some other field that dominates the energy density. We specialize to the case where the total curvature perturbation…

天体物理学 · 物理学 2015-06-24 Anupam Mazumdar , Marieke Postma

It is conjectured that inflation, taking account of quantum gravity, leads to a discrete spectrum of cosmological perturbations, instead of the continuous Gaussian spectrum predicted by standard field theory in an unquantized background.…

天体物理学 · 物理学 2009-11-10 Craig J. Hogan

In many theories of reheating starting from the classical spatially homogeneous inflaton field, its accompanying inhomogeneous part (which arises from primordial quantum fluctuations) is treated as a first order perturbation. We examine…

高能物理 - 唯象学 · 物理学 2009-10-31 A. B. Henriques , R. G. Moorhouse

Cosmological perturbations, originating in the quantum fluctuations of the fields that drive inflation, are observed to be nearly scale invariant at the largest scales. At smaller scales, however, perturbations are not severely constrained…

宇宙学与河外天体物理 · 物理学 2024-07-09 Ioannis Dalianis

We investigate the origin and evolution of primordial electric and magnetic fields in the early universe, when the expansion is governed by a cosmological constant $\Lambda_0$. Using the gravitoelectromagnetic inflationary formalism with…

广义相对论与量子宇宙学 · 物理学 2009-04-06 Federico Agustin Membiela , Mauricio Bellini

We examine cosmological perturbations in a dynamical theory of inflation in which an Abelian gauge field couples directly to the inflaton, breaking conformal invariance. When the coupling between the gauge field and the inflaton takes a…

宇宙学与河外天体物理 · 物理学 2010-10-13 Timothy R. Dulaney , Moira I. Gresham

We study the evolution of quantum fluctuations of gravity around an inflationary solution in renormalizable quantum gravity, in which the initial scalar-fluctuation dominance is shown by the background-free nature expressed by a special…

高能物理 - 理论 · 物理学 2024-01-19 Ken-ji Hamada

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

Effects of heavy fields on primordial spectra of curvature perturbations are discussed in inflationary models with a sudden turning trajectory. When heavy fields are excited after the sudden turn and oscillate around the bottom of the…

高能物理 - 理论 · 物理学 2014-03-26 Toshifumi Noumi , Masahide Yamaguchi

We present a comprehensive study of primordial fluctuations generated from G-inflation, in which the inflaton Lagrangian is of the form $K(\phi, X)-G(\phi, X)\Box\phi$ with $X=-(\partial\phi)^2/2$. The Lagrangian still gives rise to…

高能物理 - 理论 · 物理学 2011-06-07 Tsutomu Kobayashi , Masahide Yamaguchi , Jun'ichi Yokoyama

In this paper we study the generation of primordial perturbation with a modified dispersion relation in various cosmological evolutions. We stress that the formation of the power spectrum is strongly dependent on the background. Working in…

宇宙学与河外天体物理 · 物理学 2009-09-01 Yi-Fu Cai , Xinmin Zhang

One essence in capturing the history of primordial fluctuations that arise during inflation and eventually lead to formation of large scale structures in the universe, relies on quantizing general relativity coupled to a scalar field. This…

高能物理 - 理论 · 物理学 2018-07-24 Gizem Sengor

Inflation may provide unique insight into the physics at the highest available energy scales that cannot be replicated in any realistic terrestrial experiment. Features in the primordial power spectrum are generically predicted in a wide…

宇宙学与河外天体物理 · 物理学 2019-03-26 Anže Slosar , Xingang Chen , Cora Dvorkin , Daniel Green , P. Daniel Meerburg , Eva Silverstein , Benjamin Wallisch

We study the spectrum of cosmological fluctuations in scenarios such as Galilean Genesis in which a spectator scalar field acquires a scale-invariant spectrum of perturbations during an early phase which asymptotes in the far past to…

高能物理 - 理论 · 物理学 2015-06-05 Yi Wang , Robert Brandenberger

We study the effects of a general type of features of the inflaton potential on the spectrum and bispectrum of primordial curvature perturbations. These features correspond to a discontinuity in the $n$-th order derivative of the potential…

宇宙学与河外天体物理 · 物理学 2015-08-25 Alexander Gallego Cadavid

It was pointed out recently that in some inflationary models quantum loops containing a scalar of mass $m$ that couples to the inflaton can be the dominant source of primordial non-Gaussianities. We explore this phenomenon in the simplest…

高能物理 - 唯象学 · 物理学 2019-03-27 Haipeng An , Mark B. Wise , Zipei Zhang

We study the effects of a class of features of the inflaton potential, corresponding to discontinuties in its derivatives. We perform fully numerical calculations and derive analytical approximations for the curvature pertubations spectrum…

宇宙学与河外天体物理 · 物理学 2016-07-29 Alexander Gallego Cadavid , Antonio Enea Romano