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It has been argued that a Universe governed by Eddington-Born-Infeld gravity can be compatible with current cosmological constraints. The extra fields introduced in this theory can behave both as dark matter and dark energy, unifying the…

天体物理学 · 物理学 2009-04-02 Máximo Bañados , Pedro G. Ferreira , Constantinos Skordis

We explain the effect of dark matter (flat rotation curve) using modified gravitational dynamics. We investigate in this context a low energy limit of generalized general relativity with a nonlinear Lagrangian ${\cal L}\propto R^n$, where…

天体物理学 · 物理学 2008-11-26 Andrzej Borowiec , Wlodzimierz Godlowski , Marek Szydlowski

We investigate the correspondence between modified gravity theories and general entropic cosmology theory. Such a theory is proposed by an analogy with Jacobson's work, where the Einstein equation was derived from the Bekenstein-Hawking…

广义相对论与量子宇宙学 · 物理学 2025-03-24 Shin'ichi Nojiri , Sergei D. Odintsov

It is shown that quantum vacuum fluctuations give rise to a curvature of space-time of the order appropriate to explain the observed accelerated expansion of the universe. The fact that the fluctuations produce curvature, even if the…

广义相对论与量子宇宙学 · 物理学 2011-03-21 Emilio Santos

The quantization of Einstein-Maxwell theory with a cosmological constant is considered. We obtain all logarithmically divergent terms in the one-loop effective action that involve only the background electromagnetic field. This includes…

高能物理 - 理论 · 物理学 2009-11-06 David J. Toms

A global scale-invariant Dark Energy model based on Induced Gravity with the addition of a small $R^2$ contribution is examined. The scalar field (quintessence), playing the role of Dark Energy, has a quartic potential and generates…

广义相对论与量子宇宙学 · 物理学 2025-02-14 Alessandro Tronconi , Giovanni Venturi

We present evidence that a special class of gravitationally-coupled hidden sectors, in which conformal invariance is dynamically broken in a controlled way, exhibit the properties of dark energy. Such quantum field theories may appear while…

宇宙学与河外天体物理 · 物理学 2015-06-05 I. Mocioiu , R. Roiban

We prove the existence of a spectral resolution of the Wheeler-DeWitt equation when the underlying spacetime is a Friedman universe with flat spatial slices and where the matter fields are comprised of the strong interaction, with $\SU(3)$…

广义相对论与量子宇宙学 · 物理学 2010-07-27 Claus Gerhardt

It is shown that a weak modification of general relativity, in the linearized approach, renders a spherically symmetric and stationary model of the universe. This is due to the presence of a third mode of polarization in the linearized…

广义相对论与量子宇宙学 · 物理学 2009-08-03 Christian Corda , Herman J. Mosquera Cuesta

Gravitational waves (GWs) provide a new tool to probe the nature of dark energy (DE) and the fundamental properties of gravity. We review the different ways in which GWs can be used to test gravity and models for late-time cosmic…

宇宙学与河外天体物理 · 物理学 2018-12-24 Jose María Ezquiaga , Miguel Zumalacárregui

The empty space (with no matter fields) is not really empty because of natural metric fluctuations, quantum and classical. We show that gravitons as well as classical gravitational waves of super-horizon wavelengths are able to form the de…

综合物理 · 物理学 2017-05-08 Leonid Marochnik

Dark Energy is the dominant component of the energy density of the Universe. However, it is also very elusive since its interaction with the rest of the Universe is primarily gravitational.Since Dark Energy is a low energy phenomenon from…

综合物理 · 物理学 2020-02-18 Anupam Singh

In this report, we discuss a candidate mechanism through which one might address the various cosmological constant problems. We first observe that the renormalization of gravitational couplings (induced by integrating out various matter…

高能物理 - 理论 · 物理学 2010-03-17 Subodh P. Patil

This review presents a comprehensive overview of Myrzakulov gravity, highlighting key developments and significant results shaping the theory. It examines the foundational principles, field equations, and the role of non-metricity and…

广义相对论与量子宇宙学 · 物理学 2025-04-04 Davood Momeni , Ratbay Myrzakulov

As previously observed the massless limit of massive gravity leads to a modification of general relativity. Here we study spherically symmetric solutions of the modified field equations which contain normal matter together with a dark…

广义相对论与量子宇宙学 · 物理学 2009-02-18 G. Scharf

We point out that dark-energy perturbations may become unstable in the presence of a gravitational wave of sufficiently large amplitude. We study this effect for the cubic Horndeski operator (braiding), proportional to $\alpha_{\rm B}$. The…

广义相对论与量子宇宙学 · 物理学 2020-05-05 Paolo Creminelli , Giovanni Tambalo , Filippo Vernizzi , Vicharit Yingcharoenrat

We consider quantum general relativity in three dimensions with a positive cosmological constant. The Hartle-Hawking wave function is computed as a function of metric data at asymptotic future infinity. The analytic continuation from…

高能物理 - 理论 · 物理学 2015-06-11 Alejandra Castro , Alexander Maloney

General Relativity (GR) is a phenomenologically successful theory that rests on firm foundations, but has not been tested on cosmological scales. The advent of dark energy (and possibly even the requirement of cold dark matter), has…

广义相对论与量子宇宙学 · 物理学 2010-05-12 Constantinos Skordis

The Wheeler-DeWitt equation for a Kantowski-Sachs metric in Ho\v{r}ava-Lifshitz gravity with a set of coordinates in minisuperspace that obey a generalized uncertainty principle is studied. We first study the equation coming from a set of…

广义相对论与量子宇宙学 · 物理学 2022-04-14 H. Garcia-Compean , D. Mata-Pacheco

The Friedmann equation, augmented with an additional term that effectively takes on the role of dark energy, is demonstrated to be an exact solution to the recently proposed gravitational theory named "conformal Killing gravity." This…

广义相对论与量子宇宙学 · 物理学 2023-11-20 Junpei Harada