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相关论文: Genesis--Starobinsky inflation can explain the ACT…

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In this work we examine a theoretical scenario which combines two fundamental theoretical proposals for the early Universe and a possible evolution for the early post-inflationary epoch. Specifically, we assume that the early Universe…

广义相对论与量子宇宙学 · 物理学 2025-09-23 S. D. Odintsov , V. K. Oikonomou

We have found numerically initial conditions in the $(R, H)$ plane leading to a successful Starobinsky inflation in $R+R^2$ gravity for a isotropic metrics with positive spatial curvature. Trajectories can reach inflation regime either…

广义相对论与量子宇宙学 · 物理学 2023-11-03 Daniel Müller , Alexey Toporensky

Our primary objective is the formulation of a plausible cosmological inflationary model entirely in terms of a pure modified gravity without any a priori matter couplings within the formalism of non-Riemannian spacetime volume elements. The…

广义相对论与量子宇宙学 · 物理学 2019-12-24 David Benisty , Eduardo Guendelman , Emil Nissimov , Svetlana Pacheva

We examine the power-law Starobinsky model, a generalized version of the Starobinsky inflation model, characterized by a power-law correction to Einstein gravity. Employing the $f(R)$ formalism, the scalar and tensor power spectra were…

宇宙学与河外天体物理 · 物理学 2025-02-10 Saisandri Saini , Akhilesh Nautiyal

The first inflationary model conceived was the one proposed by Starobinsky which includes an additional term quadratic in the Ricci-scalar R in the Einstein-Hilbert action. The model is now considered a target for several future cosmic…

宇宙学与河外天体物理 · 物理学 2021-01-27 S. Santos da Costa , M. Benetti , R. M. P. Neves , F. A. Brito , R. Silva , J. S. Alcaniz

We investigate the cosmological inflation in a class of supergravity models that are generalizations of non-supersymmetric $R^2$ models. Although such models have been extensively studied recently, especially after the launch of the PLANCK…

高能物理 - 理论 · 物理学 2015-06-23 G. A. Diamandis , B. C. Georgalas , K. Kaskavelis , P. Kouroumalou , A. B. Lahanas , G. Pavlopoulos

We give a brief review of the basic principles of inflationary theory and discuss the present status of the simplest inflationary models that can describe Planck/BICEP/Keck observational data by choice of a single model parameter. In…

高能物理 - 理论 · 物理学 2025-10-28 Renata Kallosh , Andrei Linde

We derive a general criterion that defines all single-field models leading to Starobinsky-like inflation and to universal predictions for the spectral index and tensor-to-scalar ratio, which are in agreement with Planck data. Out of all the…

高能物理 - 唯象学 · 物理学 2015-06-18 Gian F. Giudice , Hyun Min Lee

We consider the ghost-free higher order corrections to the Starobinsky model in the old minimal supergravity. In general, higher order corrections cannot be forbidden by symmetries, which likely violate the flatness of the scalaron…

高能物理 - 理论 · 物理学 2015-01-26 Kohei Kamada , Jun'ichi Yokoyama

Starobinsky's $R+\alpha R^2$ inflation provides a compelling one-parameter inflationary model that is supported by current cosmological observations. However, at the same order in spacetime derivatives as the $R^2$ term, an effective theory…

广义相对论与量子宇宙学 · 物理学 2025-12-03 Eugenio Bianchi , Mauricio Gamonal

We present a joint Bayesian analysis to impose constraints on the generalized $\alpha$-Starobinsky inflationary model using the high-precision cosmological datasets: Planck, CMB lensing from ACT DR6, and Baryon Acoustic Oscillations (BAO)…

宇宙学与河外天体物理 · 物理学 2026-03-27 Karim Carrion , Francisco X. Linares Cedeño , Gabriel Germán , Juan Carlos Hidalgo

An extension of the Starobinsky model is proposed. Besides the usual Starobinsky Lagrangian, a term proportional to the derivative of the scalar curvature, $\nabla_{\mu}R\nabla^{\mu}R$, is considered. The analyzis is done in the Einstein…

广义相对论与量子宇宙学 · 物理学 2019-03-04 R. R. Cuzinatto , L. G. Medeiros , P. J. Pompeia

In light of the recent results from the Atacama Cosmology Telescope (ACT), which have provided a notable shift in the constraints on $(n_s, r)$ and placed several otherwise viable models of inflation in tension with the latest data, we…

宇宙学与河外天体物理 · 物理学 2026-03-03 William J. Wolf

We apply the gravity-thermodynamics conjecture, namely the first law of thermodynamics on the Universe horizon, but using the generalized Kaniadakis entropy instead of the standard Bekenstein-Hawking one. The former is a one-parameter…

广义相对论与量子宇宙学 · 物理学 2021-12-07 Andreas Lymperis , Spyros Basilakos , Emmanuel N. Saridakis

In the framework of Born-Infeld inspired gravity theories, which deviates from General Relativity (GR) in the high curvature regime, we discuss the viability of Cosmic Inflation without scalar fields. For energy densities higher than the…

广义相对论与量子宇宙学 · 物理学 2016-03-10 Jose Beltran Jimenez , Lavinia Heisenberg , Gonzalo J. Olmo , Christophe Ringeval

We have presented previously a general treatment of Starobinsky-like inflation in no-scale supergravity where the tensor-to-scalar ratio $r = 3(1 - n_s)^2$, and $n_s$ is the tilt of the scalar perturbations. In particular, we have shown how…

高能物理 - 理论 · 物理学 2019-10-02 John Ellis , Dimitri V. Nanopoulos , Keith A. Olive , Sarunas Verner

We display some simple cosmological solutions of gravity theories with quadratic Ricci curvature terms added to the Einstein-Hilbert lagrangian which exhibit anisotropic inflation. The Hubble expansion rates are constant and unequal in…

广义相对论与量子宇宙学 · 物理学 2010-04-21 J. D. Barrow , S. Hervik

Models of inflation are tightly constrained by the PLANCK satellite data. Among them, Starobinsky's model with an exponential type potential seems to be challenged by the recent BICEP2 results. The model is based on the existence of $\,~…

高能物理 - 理论 · 物理学 2015-01-28 A. B. Lahanas , K. Tamvakis

Recent measurements from the Atacama Cosmology Telescope (ACT), particularly when combined with DESI baryon acoustic oscillation data, have reported a scalar spectral index $n_s$ slightly higher than that inferred by {\it Planck}~2018,…

宇宙学与河外天体物理 · 物理学 2025-11-18 Jureeporn Yuennan , Farruh Atamurotov , Phongpichit Channuie

To explain the accelerated expansion of late universe, the 1/R correction to Einstein gravity is usually considered, where R is the Ricci scalar. This correction term is generally believed to be negligible in the early universe. However, if…

宇宙学与河外天体物理 · 物理学 2014-11-20 Shi Pi , Tower Wang