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相关论文: Curvaton reheating in a Scale Invariant Two Measur…

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The instant preheating mechanism in the framework of a scale invariant two measures theory is studied. We introduce this mechanism into a non oscillating inflationary model as another possible solution to the reheating of the universe in…

广义相对论与量子宇宙学 · 物理学 2021-06-16 Eduardo I. Guendelman , Ramon Herrera , Pedro Labrana

The dilaton-gravity sector of a linear in the scalar curvature, scale invariant Two Measures Field Theory (TMT), is explored in detail in the context of closed FRW cosmology and shown to allow stable emerging universe solutions. The model…

宇宙学与河外天体物理 · 物理学 2015-05-28 Sergio del Campo , Eduardo I. Guendelman , Alexander B. Kaganovich , Ramon Herrera , Pedro Labrana

A unified multi scalar field model with three flat regions is discussed. The three flat regions are the inflation, early and late dark energy epochs. The potential is obtained by a spontaneous breaking of scale invariance generated by Non…

广义相对论与量子宇宙学 · 物理学 2022-06-22 Eduardo Guendelman , Ramon Herrera , David Benisty

There might be a light scalar field during inflation which is not responsible for the accelerating inflationary expansion. Then, its quantum fluctuation is stretched during inflation. This scalar field could be a curvaton, if it decays at a…

宇宙学与河外天体物理 · 物理学 2015-06-04 Ki-Young Choi , Osamu Seto

A new class of gravity-matter model defined with an independent non-Riemannian volume form is studied, in the second order formalism. The action has a global scale invariance symmetry, which can be broken by the equation of motion of the…

广义相对论与量子宇宙学 · 物理学 2019-05-22 David Benisty , Eduardo I. Guendelman

The curvaton reheating in a tachyonic inflationary universe model with an exponential potential is studied. We have found that the energy density in the kinetic epoch, has a complicated dependencies of the scale factor. For different…

广义相对论与量子宇宙学 · 物理学 2009-11-11 C. Campuzano , S. del Campo , R. Herrera

A new class of gravity-matter models defined in terms of two independent non-Riemannian volume forms (alternative generally covariant integration measure densities) on the space-time manifold are studied in some detail. These models involve…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Eduardo Guendelman , Ramón Herrera , Pedro Labraña , Emil Nissimov , Svetlana Pacheva

Scale invariance is considered in the context of a gravitational theory where the action, in the first order formalism, is of the form S = \int L_{1} \Phi d^4x + \int L_{2}\sqrt{-g}d^4x where \Phi is a density built out of degrees of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 E. I. Guendelman , A. B. Kaganovich

The curvaton reheating mechanism in a non-minimal derivative coupling to gravity for any non-oscillating (NO) model is studied. In this framework, we analyze the energy density during the kinetic epoch and we find that this energy has a…

广义相对论与量子宇宙学 · 物理学 2016-10-05 Ramon Herrera , Joel Saavedra , Cuauhtemoc Campuzano

The quantum evolution of a model of the universe with account of two scalar fields ({\it dilaton} and {\it inflaton}) is considered. For this case, the closed and flat models has been examined. It is shown that in both cases the realization…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. N. Folomeev

The curvaton and the inhomogeneous reheating scenarios for the generation of the cosmological curvature perturbation on large scales represent an alternative to the standard slow-roll scenario where the observed density perturbations are…

天体物理学 · 物理学 2009-11-10 L. Pilo , A. Riotto , A. Zaffaroni

We present a gauge-invariant formalism to study the evolution of the curvature and entropy perturbations in the case in which spatial and time variations of the inflaton decay rate into ordinary matter are present. During the reheating…

天体物理学 · 物理学 2009-11-10 Sabino Matarrese , Antonio Riotto

In a logamediate inflationary universe model we introduce the curvaton field in order to bring this inflationary model to an end. In this approach we determine the reheating temperature. We also outline some interesting constraints on the…

宇宙学与河外天体物理 · 物理学 2010-04-23 Cuauhtemoc Campuzano , Sergio del Campo , Ramon Herrera , Efrain Rojas , Joel Saavedra

The curvaton reheating in a non-oscillatory inflationary universe model is studied in a Jordan-Brans-Dicke theory. For different scenarios, the temperature of reheating is computed. The result tells us that the reheating temperature becomes…

天体物理学 · 物理学 2009-11-11 Cuauhtemoc Campuzano , Sergio del Campo , Ramon Herrera

We present a new general mechanism for generating curvature perturbations after inflation. Our model is based on the simple assumption that a field that starts to oscillate after inflation has a potential characterized by an underlying…

高能物理 - 唯象学 · 物理学 2008-11-26 Tomohiro Matsuda

Inspired by \cite{Jiang:2018uce}, we propose a similar curvaton mechanism whose realization occurs in preheating process, in which the effective mass is running (its potential consists of coupling part and exponential part whose…

宇宙学与河外天体物理 · 物理学 2020-08-04 Lei-Hua Liu , Wu-Long Xu

In this paper we study a novel realization of inflation, based on Weyl invariant gravity with torsion. We show that requiring the classical action for the scalar field to be Weyl invariant introduces a dilaton which induces a non trivial…

广义相对论与量子宇宙学 · 物理学 2019-01-16 A. Barnaveli , S. Lucat , T. Prokopec

The curvaton was introduced recently as a distinct inflationary mechanism for generating adiabatic density perturbations. Implicit in that scenario is that the curvaton offers a new mechanism for reheating after inflation, as it is a form…

天体物理学 · 物理学 2009-11-07 Andrew R. Liddle , L. Arturo Urena-Lopez

We study an inflationary scenario where thermal inflation is followed by fast-roll inflation. This is a rather generic possibility based on the effective potentials of spontaneous symmetry breaking in the context of particle physics models.…

高能物理 - 唯象学 · 物理学 2008-11-26 Jinn-Ouk Gong

We consider the possible decay of the inflaton into curvaton particles during reheating and analyse its effect on curvaton scenarios. Typical decay curvatons are initially relativistic then become non-relativistic, changing the background…

宇宙学与河外天体物理 · 物理学 2016-12-05 Christian T Byrnes , Marina Cortês , Andrew R Liddle
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