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相关论文: Palatini-Born-Infeld Gravity, Bouncing Universe, a…

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In this study, we consider a flat Friedmann-Robertson-Walker (FRW) universe in the context of Palatini $f(R)$ theory of gravity. Using the dynamical equivalence between $f(R)$ gravity and scalar-tensor theories, we construct a point…

广义相对论与量子宇宙学 · 物理学 2012-02-02 Y. Kucukakca , U. Camci

The non-equivalence between the metric and Palatini formalisms of $f(R)$ gravity is an intriguing feature of these theories. However, in the recently proposed hybrid metric-Palatini gravity, consisting of the superposition of the metric…

广义相对论与量子宇宙学 · 物理学 2013-08-23 Salvatore Capozziello , Tiberiu Harko , Francisco S. N. Lobo , Gonzalo J. Olmo

The recent direct detection of gravitational waves has highlighted the huge importance of the tensorial modes in any extended gravitational theory. One of the most appealing approaches to extend gravity beyond general relativity is the…

广义相对论与量子宇宙学 · 物理学 2020-01-16 Imanol Albarran , Mariam Bouhmadi-López , Che-Yu Chen , Pisin Chen

We investigate the dynamics of a family of functional extensions of the (Eddington-inspired) Born-Infeld gravity theory, constructed with the inverse of the metric and the Ricci tensor. We provide a generic formal solution for the…

高能物理 - 理论 · 物理学 2014-08-06 Sergei D. Odintsov , Gonzalo J. Olmo , D. Rubiera-Garcia

We construct Born-Infeld (BI) type gravity theories which describe tree-level unitary (non-ghost and non-tachyonic) massless spin-2 modes around their maximally symmetric vacua in four dimensions. Building unitary BI actions around flat…

高能物理 - 理论 · 物理学 2015-03-05 Ibrahim Gullu , Tahsin Cagri Sisman , Bayram Tekin

In this paper we present the techniques for computing cosmological bounces in polynomial $f(R)$ theories, whose order is more than two, for spatially flat FLRW spacetime. In these cases the conformally connected Einstein frame shows up…

广义相对论与量子宇宙学 · 物理学 2016-02-17 Kaushik Bhattacharya , Saikat Chakrabarty

The occurrence of a bounce in FRW cosmology requires modifications of general relativity. An example of such a modification is the recently proposed Horava-Lifshitz theory of gravity, which includes a ``dark radiation'' term with a negative…

高能物理 - 理论 · 物理学 2011-03-31 Ewa Czuchry

In the framework of classical scale invariance, we consider quadratic gravity in the Palatini formalism and investigate the inflationary predictions of the theory. Our model corresponds to a two-field scalar-tensor theory, that involves the…

宇宙学与河外天体物理 · 物理学 2021-07-28 Ioannis D. Gialamas , Alexandros Karam , Thomas D. Pappas , Vassilis C. Spanos

We study a model of quintessential inflation constructed in $R^2$ modified gravity with a non-minimally coupled scalar field, in the Palatini formalism. Our non-minimal inflaton field is characterised by a simple exponential potential. We…

广义相对论与量子宇宙学 · 物理学 2022-04-21 Konstantinos Dimopoulos , Alexandros Karam , Samuel Sánchez López , Eemeli Tomberg

General Relativity has shown an outstanding observational success in the scales where it has been directly tested. However, modifications have been intensively explored in the regimes where it seems either incomplete or signals its own…

广义相对论与量子宇宙学 · 物理学 2018-02-14 Jose Beltran Jimenez , Lavinia Heisenberg , Gonzalo J. Olmo , Diego Rubiera-Garcia

We use the Bogoliubov formalism to study both, particles and gravitons creation at the reheating epoch, after a phase transition from inflation to a radiation dominated universe. The modes of the inflaton field fluctuations and the scalar…

广义相对论与量子宇宙学 · 物理学 2011-10-07 Mariano Anabitarte , Mauricio Bellini

A novel theory of Quantum Gravity is presented in which the real gravitons manifest themselves as holes in space. In general, these holes propagate at the speed of light through an expanding universe with boundary denoted by U, which is…

综合物理 · 物理学 2015-08-26 Gregory W. Horndeski

In this paper we follow a new approach for particle creation by a localized strong gravitational field. The approach is based on a definition of the physical vacuum drawn from Heisenberg uncertainty principle. Using the fact that the…

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

In a Palatini $f(\mathcal{R})$-model, we define chonodynamical effects due to the choice of atomic clocks as standard reference clocks and we develop a formalism able to quantitatively separate them from the usual effective dark sources one…

广义相对论与量子宇宙学 · 物理学 2019-01-08 L. Del Vecchio , L. Fatibene , S. Capozziello , M. Ferraris , P. Pinto , S. Camera

We study the conditions for 2-dimensional dilaton gravity models to have dynamical formation of black holes and construct all such models. Furthermore we present a parametric representation of the general solutions of the black holes.

广义相对论与量子宇宙学 · 物理学 2014-11-17 T. Futamase , M. Hotta , Y. Itoh

In this paper by deriving the Modified Friedmann equation in the Palatini formulation of $R^2$ gravity, first we discuss the problem of whether in Palatini formulation an additional $R^2$ term in Einstein's General Relativity action can…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Xin He Meng , Peng Wang

We investigate the viability of f(R) theories in the framework of the Palatini approach as solutions to the problem of the observed accelerated expansion of the universe. Two physically motivated popular choices for f(R) are considered:…

天体物理学 · 物理学 2009-11-10 S. Capozziello , V. F. Cardone , M. Francaviglia

Previous work involving Born-regulated gravity theories in two dimensions is extended to four dimensions. The action we consider has two dimensionful parameters. Black hole solutions are studied for typical values of these parameters. For…

高能物理 - 理论 · 物理学 2016-08-25 James A. Feigenbaum

Gravitational collapse into a black hole has been extensively studied with classical sources. We develop a new formalism to simulate quantum fields forming a black hole. This formalism utilizes well-established techniques used for classical…

广义相对论与量子宇宙学 · 物理学 2021-08-18 Benjamin Berczi , Paul M. Saffin , Shuang-Yong Zhou

We study single-field slow-roll inflation embedded in Palatini $F(R)$ gravity where $F(R)$ grows faster than $R^2$. Surprisingly, the consistency of the theory requires the Jordan frame inflaton potential to be unbounded from below. Even…

广义相对论与量子宇宙学 · 物理学 2024-03-21 Christian Dioguardi , Antonio Racioppi , Eemeli Tomberg