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相关论文: Lorentzian Vacuum Transitions in $f(R)$ gravity

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We compute curvature-dependent graviton correlation functions and couplings as well as the full curvature potential $f(R)$ in asymptotically safe quantum gravity coupled to scalars. The setup is based on a systematic vertex expansion about…

高能物理 - 理论 · 物理学 2019-12-05 Benjamin Bürger , Jan M. Pawlowski , Manuel Reichert , Bernd-Jochen Schaefer

We analyze some relevant features of the primordial Universe as viewed in the Jordan frame formulation of the f(R)-gravity, especially when the potential term of the non-minimally coupled scalar field is negligible. We start formulating the…

广义相对论与量子宇宙学 · 物理学 2023-04-13 Nicola Bamonti , Andrea Costantini , Giovanni Montani

We derive Friedman-Lemaitre-Robertson-Walker (FLRW) models as non-trivial solutions of "Cotton Gravity" (CG), a recently proposed gravity theory alternative to General Relativity (GR) based on the Cotton tensor. Using an equivalent…

广义相对论与量子宇宙学 · 物理学 2023-12-05 Roberto A Sussman , Sebastian Najera

In this paper we study the flat (k=0) cosmological FRW model with holonomy corrections of Loop Quantum Gravity. The considered universe contains a massless scalar field and the cosmological constant Lambda. We find analytical solutions for…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Jakub Mielczarek , Tomasz Stachowiak , Marek Szydlowski

Among relativistic theories of gravitation the closest ones to general relativity are the scalar-tensor ones and these with Lagrangians being any function f(R) of the curvature scalar. A complete chart of relationships between these…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Leszek M. Sokolowski

A free scalar field minimally coupled to gravity model is quantized and the Wheeler-DeWitt equation in minisuperspace is solved analytically, exhibiting positive and negative frequency modes. The analysis is performed for positive, negative…

广义相对论与量子宇宙学 · 物理学 2009-10-31 R. Colistete , J. C. Fabris , N. Pinto-Neto

In this work, a flat Friedmann-Robertson-Walker (FRW) universe with dust and a cosmological constant is quantized. By means of a canonical transformation, the classical Hamiltonian is reduced to that of either a harmonic oscillator or…

广义相对论与量子宇宙学 · 物理学 2010-05-12 Edésio M. Barboza , Nivaldo A. Lemos

The Higher Order Theories of Gravity - $f(R, R_{\alpha\beta}R^{\alpha\beta})$ - theory, where $R$ is the Ricci scalar, $R_{\alpha\beta}$ is the Ricci tensor and $f$ is any analytic function - have recently attracted a lot of interest as…

广义相对论与量子宇宙学 · 物理学 2010-02-07 Arturo Stabile

In this paper, the exact vacuum solution of a general plane symmetric spacetime is investigated in metric f(R) gravity with the assumption of constant Ricci scalar. For this solution, we have studied the generalized Landau-Lifshitz…

广义相对论与量子宇宙学 · 物理学 2014-06-17 Morteza Yavari

Using Ashtekar variables, we analyze Lorentzian and Euclidean gravity in vacuum up to a constant conformal transformation. We prove that the reality conditions are invariant under a Wick rotation of the time, and show that the compatibility…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Guillermo A. Mena Marugan

We investigate a lattice model for Euclidean quantum gravity based on discretization of the Palatini formulation of General Relativity. Using Monte Carlo simulation we show that while a naive approach fails to lead to a vacuum state…

高能物理 - 格点 · 物理学 2013-03-05 Simon Catterall , Daniel Ferrante , A. Nicholson

In this paper, we report the existence of transitioning scenario of Bianchi type I universe in the context of $f\left(R,T\right)$ gravity with special case $f\left(R,T\right) = f_{1}(R) + f_{2}(R)f_{3}(T)$ and it's functional forms…

综合物理 · 物理学 2019-04-24 Anil Kumar Yadav

We present a systematic approach to embed $n$-dimensional vacuum general relativity in an $(n + 1)$-dimensional pseudo-Riemannian spacetime whose source is either a (non)zero cosmological constant or a scalar field minimally-coupled to…

广义相对论与量子宇宙学 · 物理学 2015-09-30 J. Ponce de Leon

We consider a novel class of $f(\R)$ gravity theories where the connection is related to the conformally scaled metric $\hat g_{\mu\nu}=C(\R)g_{\mu\nu}$ with a scaling that depends on the scalar curvature $\R$ only. We call them C-theories…

广义相对论与量子宇宙学 · 物理学 2011-02-18 Luca Amendola , Kari Enqvist , Tomi Koivisto

We investigate the problem of metric fluctuations in the presence of the vacuum fluctuations of matter fields and critically assess the usual assertion that vacuum energy implies a Planckian cosmological constant. A new stochastic classical…

广义相对论与量子宇宙学 · 物理学 2008-06-19 Charles H. -T. Wang , Paolo M. Bonifacio , Robert Bingham , J. Tito Mendonca

In this work we present cosmological solutions from the simplest non-trivial $T$-dependence in $f(R,T)$ theory of gravity, with $R$ and $T$ standing for the Ricci scalar and trace of the energy-momentum tensor, respectively. Although such…

高能物理 - 理论 · 物理学 2016-06-29 P. H. R. S. Moraes , G. Ribeiro , R. A. C. Correa

Here we analysed a particular type of $F(R)$ gravity, the so-called exponential gravity which includes an exponential function of the Ricci scalar in the action. Such term represents a correction to the usual Hilbert-Einstein action. By…

广义相对论与量子宇宙学 · 物理学 2018-01-17 Sergei D. Odintsov , Diego Saez-Chillon Gomez , German S. Sharov

Here in this work we propose a modified gravity with the action of $f(R) = \sqrt{R^2 - R_0^2}$ instead of Einstein-Hilbert action to describe the late time acceleration of the universe. We obtain the equation of the modified gravity both in…

天体物理学 · 物理学 2008-11-26 Shant Baghram , Marzieh Farhang , Sohrab Rahvar

In Cuzinatto et al. [Phys. Rev. D 93, 124034 (2016)], it has been demonstrated that theories of gravity in which the Lagrangian includes terms depending on the scalar curvature $R$ and its derivatives up to order $n$, i.e.…

广义相对论与量子宇宙学 · 物理学 2019-05-07 R. R. Cuzinatto , C. A. M. de Melo , L. G. Medeiros , P. J. Pompeia

The Wheeler-DeWitt equation is solved for some scalar-tensor theories of gravitation in the case of homogeneous and isotropic cosmological models.We present general solutions corresponding to cosmological term: (i)\lambda(\phi)=0$ and $(ii)…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Luis O. Pimentel , César Mora
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