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相关论文: On the Viability of the Intermediate Inflation Sce…

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We investigate warm intermediate scenario of the cosmological inflation in $F(T)$ gravity in the limit of high dissipation. The inflationary expansion is driven by the scalar inflaton while the gravitational dynamics follow from the $F(T)$…

广义相对论与量子宇宙学 · 物理学 2015-06-09 Mubasher Jamil , Davood Momeni , Ratbay Myrzakulov

We study inflation in the framework of $f(T)$-gravity in the presence of a canonical scalar field. After reviewing the basic equations governing the background cosmology in $f(T)$-gravity, we turn to study the cosmological perturbations and…

广义相对论与量子宇宙学 · 物理学 2016-02-02 K. Rezazadeh , A. Abdolmaleki , K. Karami

We demonstrate that the intermediate inflation scenario, is a singular inflation cosmology, with the singularity at the origin $t=0$ being a pressure and energy density singularity and particularly a Type III singularity. Also, we show that…

广义相对论与量子宇宙学 · 物理学 2017-03-21 V. K. Oikonomou

An intermediate inflationary universe model within the context of non-minimally coupled to the scalar curvature is analyzed. We will conduct our analysis under the slow roll approximation of the inflationary dynamics and the cosmological…

广义相对论与量子宇宙学 · 物理学 2017-09-12 Carlos Gonzalez , Ramon Herrera

We investigate inflation within $f(R,\phi)$-theories, where a dynamical scalar field is coupled to gravity. A class of models which can support early-time acceleration with the emerging of an effective cosmological constant at high…

广义相对论与量子宇宙学 · 物理学 2018-12-13 R. Myrzakulov , L. Sebastiani , S. Vagnozzi

In this paper, we demonstrate that a unified description of early and late-time acceleration is possible in the context of mimetic $F(R)$ gravity. We study the inflationary era in detail and demonstrate that it can be realized even in…

广义相对论与量子宇宙学 · 物理学 2016-12-21 S. Nojiri , S. D. Odintsov , V. K. Oikonomou

We study slow-roll inflation and the generation of primordial fluctuations in $F(T)$ gravity's rainbow. We obtain the second order action for scalar and tensor perturbations and then calculate the primordial power spectrum for them. Thus,…

广义相对论与量子宇宙学 · 物理学 2022-02-18 Yoelsy Leyva , Carlos Leiva , Giovanni Otalora , Joel Saavedra

We study warm inflation in the framework of $f(\phi)T$ gravity, where $\phi$ is the inflaton and $T$ is the trace of the energy-momentum tensor. The inflaton field is assumed to roll on the natural potential and the result is analyzed in…

广义相对论与量子宇宙学 · 物理学 2024-08-02 Sabina Yeasmin , Atri Deshamukhya

In this work we address the possibility of having a positive running of the spectral index in inflationary theories. The recent ACT data indicate mildly that the running of the spectral index might be positive, and several other physical…

广义相对论与量子宇宙学 · 物理学 2026-05-19 S. D. Odintsov , V. K. Oikonomou

We investigate the inflationary realization in the context of unimodular $F(T)$ gravity, which is based on the $F(T)$ modification of teleparallel gravity, in which one imposes the unimodular condition through the use of Lagrange…

广义相对论与量子宇宙学 · 物理学 2017-06-29 Kazuharu Bamba , Sergei D. Odintsov , Emmanuel N. Saridakis

By applying a particular kind of modified gravity, we study the inflation. Precisely, we extend our investigations beyond the Einstein's gravity to explore the Natural inflation model via the term $F(\phi)T$. We compute the inflation…

广义相对论与量子宇宙学 · 物理学 2025-07-30 Feyzollah Younesizadeh , Davoud Kamani

We describe in this paper the observables of inflationary models, in particular the spectrum index of torsion scalar perturbations, the tensor-to-scalar ratio, and the running of the spectral index, in the framework of perfect fluid models…

广义相对论与量子宇宙学 · 物理学 2016-06-22 M. G. Ganiou , M. J. S. Houndjo , I. G. Salako , M. E. Rodrigues , J. Tossa

In this paper we shall consider an exponential inflationary model in the context of vacuum $F(R)$ gravity. By using well-known reconstruction techniques, we shall investigate which $F(R)$ gravity can realize the exponential inflation…

广义相对论与量子宇宙学 · 物理学 2018-03-14 V. K. Oikonomou

We investigate the warm inflationary scenario within the context of the linear version of f (Q, T ) gravity, coupled with both the inflaton scalar field and the radiation field, under the conditions of the strong dissipation regime. First,…

广义相对论与量子宇宙学 · 物理学 2024-08-14 Maryam Shiravand , Mehrdad Farhoudi , Parviz Goodarzi

In this work we study certain classes of $F(R,{\cal G})$ gravity which have appealing phenomenological features, with respect to the successful realization of the dark energy and of the inflationary era. Particularly, we discuss the general…

广义相对论与量子宇宙学 · 物理学 2019-02-20 S. D. Odintsov , V. K. Oikonomou , S. Banerjee

We propose a new version of the hybrid inflation scenario that produces a significantly tilted n>1 spectrum of curvature perturbations. This may happen in supersymmetric models where the inflaton field acquires a mass proportional to the…

天体物理学 · 物理学 2009-09-29 Juan Garcia-Bellido , Andrei Linde

We study inflation and the generation of primordial fluctuations in $f(R)$ gravity's rainbow. We calculate the cosmological perturbations and then the scalar and tensor primordial power spectrum. We contrast the predictions of the model…

广义相对论与量子宇宙学 · 物理学 2023-04-13 Yoelsy Leyva , Giovanni Otalora

We investigate intermediate inflation in the framework of a Galileon scalar field. To this aim, we first obtain the inflationary observables, including the scalar spectral index, the tensor-to-scalar ratio, the running of the scalar…

广义相对论与量子宇宙学 · 物理学 2018-09-03 Zeinab Teimoori , Kayoomars Karami

We study the inflationary scenario in the Tsallis entropy-based cosmology. The Friedmann equations in this setup can be derived by using the first law of thermodynamics. To derive the relations of the power spectra of the scalar and tensor…

广义相对论与量子宇宙学 · 物理学 2024-01-26 Zeinab Teimoori , Kazem Rezazadeh , Abasat Rostami

We study early universe with a particular form of F(T) Telleparallel gravity theory, in which inflation is driven by a scalar field. To ensure slow rollover, two different potentials are chosen in a manner, such that they remain almost flat…

宇宙学与河外天体物理 · 物理学 2021-12-20 Manas Chakrabortty , Nayem Sk , Susmita Sanyal , Abhik Kumar Sanyal
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