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We present a model of the gravitational field based on two symmetric tensors. Gravity is affected by the new field, but outside matter the predictions of the model coincide exactly with general relativity, so all classical tests are…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Jorge Alfaro , Pablo González

We present a model of the gravitational field based on two symmetric tensors. The equations of motion of test particles are derived: Massive particles do not follow a geodesic but massless particles trajectories are null geodesics of an…

广义相对论与量子宇宙学 · 物理学 2015-05-19 J. Alfaro

$\tilde{\delta}$ Gravity is a gravitational field model, where the geometry is governed by two symmetric tensors, $g_{\mu \nu}$ and $\tilde{g}_{\mu \nu}$, and new matter fields ($\tilde{\delta}$ Matter fields) are added to the original…

广义相对论与量子宇宙学 · 物理学 2017-12-08 Jorge Alfaro , Pablo González

$\tilde{\delta}$ Gravity is a gravitational field model, where the geometry is governed by two symmetric tensors, $g_{\mu \nu}$ and $\tilde{g}_{\mu \nu}$, and new matter fields ($\tilde{\delta}$ Matter fields) are added to the original…

广义相对论与量子宇宙学 · 物理学 2017-12-08 Jorge Alfaro , Pablo González

A gravitational field model based on two symmetric tensors, $g_{\mu \nu}$ and $\tilde{g}_{\mu \nu}$, is studied, using a Markov Chain Monte Carlo (MCMC) analysis with the most updated catalog of SN-Ia. In this model, new matter fields are…

宇宙学与河外天体物理 · 物理学 2019-02-12 Jorge Alfaro , Marco San Martin , Joaquin Sureda

A new model of nonlinear electrodynamics with a dimensional parameter $\beta$ coupled to gravity is considered. We show that an accelerated expansion of the universe takes place if the nonlinear electromagnetic field is the source of the…

广义相对论与量子宇宙学 · 物理学 2016-01-26 S. I. Kruglov

Three theoretical criteria for gravitational theories beyond general relativity are considered: obtaining the cosmological constant as an integration constant, deriving the energy conservation law as a consequence of the field equations,…

广义相对论与量子宇宙学 · 物理学 2023-08-17 Junpei Harada

A tetrad-based procedure is presented for solving Einstein's field equations for spherically-symmetric systems; this approach was first discussed by Lasenby et al. in the language of geometric algebra. The method is used to derive metrics…

广义相对论与量子宇宙学 · 物理学 2015-05-27 Roshina Nandra , Anthony N. Lasenby , Michael P. Hobson

We analyze an alternative theory of gravity characterized by metrics that are tensor density of rank(0,2)and weight-1/2.The metric compatibility condition is supposed to hold. The simplest expression for the action of gravitational field is…

广义相对论与量子宇宙学 · 物理学 2008-12-18 Amir H. Abbassi , Amir M. Abbassi

Under the assumption that General Relativity (GR) correctly describes the phenomenology of our Universe, astronomical observations provide compelling evidence that (1) the dynamics of cosmic structure is dominated by dark matter (DM), an…

天体物理学 · 物理学 2008-02-19 A. Diaferio

A metric-field approach to gravitation is presented. It is based on an idea of dependency of space-time properties on measuring instruments. Some bimetric equations that realize this idea are considered. They were tested by the binary…

广义相对论与量子宇宙学 · 物理学 2009-11-07 L. V. Verozub

A gravity theory is developed with the metric ${\hat g}_{\mu\nu}= {g}_{\mu\nu}+B\partial_\mu\phi\partial_\nu\phi$. In the present universe the additional contribution from the scalar field in the metric ${\hat g}_{\mu\nu}$ can generate an…

广义相对论与量子宇宙学 · 物理学 2009-10-31 M. A. Clayton , J. W. Moffat

Einstein gravity coupled to a massive skew symmetric field F_{\mu\nu\lambda} leads to an acceleration law that modifies the Newtonian law of attraction between particles. We use a framework of non-perturbative renormalization group…

天体物理学 · 物理学 2009-11-10 J. W. Moffat

Massless particles in General Relativity move with the speed of light, their trajectories in spacetime are described by null geodesics. This is independent of the electrical charge of the particle being considered, however, the charged…

广义相对论与量子宇宙学 · 物理学 2019-08-22 Christian G. Boehmer , Peter A. Hogan

A scalar-tensor theory of gravity is formulated in which $G$ and particle masses are allowed to vary. The theory yields a globally static cosmological model with no evolutionary timescales, no cosmological coincidences, and no flatness and…

综合物理 · 物理学 2015-10-01 Meir Shimon

In the context of the Teleparallel Equivalent of General Relativity (TEGR) one can obtain an alternative insight into General Relativity, as has been shown in addressing properties as energy, momentum and angular momentum of the…

广义相对论与量子宇宙学 · 物理学 2018-06-11 K. H. C. Castello-Branco , J. F. da Rocha-Neto

A ghost-free theory of gravity with two dynamical metrics both coupled to matter is shown to be consistent and viable. Its cosmological implications are studied, and the models, in particular in the context of partially massless gravity,…

高能物理 - 理论 · 物理学 2013-10-25 Yashar Akrami , Tomi S. Koivisto , David F. Mota , Marit Sandstad

Delta Gravity is a gravitational model based on an extension of General Relativity given by a new symmetry called $\tilde{\delta}$. In this model, new matter fields are added to the original matter fields, motivated by the additional…

宇宙学与河外天体物理 · 物理学 2021-07-01 Jorge Alfaro , Marco San Martín , Carlos Rubio

The gravitational field of a particle of small mass $\mu$ moving through curved spacetime, with metric $g_{ab}$, is naturally and easily decomposed into two parts each of which satisfies the perturbed Einstein equations through $O(\mu)$.…

广义相对论与量子宇宙学 · 物理学 2009-09-01 Steven Detweiler

We discuss the quantization of Delta gravity, a two symmetric tensors model of gravity. This model, in Cosmology, shows accelerated expansion without a cosmological constant. We present the $\tilde{\delta}$ transformation which defines the…

广义相对论与量子宇宙学 · 物理学 2015-05-19 Jorge Alfaro , Pablo González , Ricardo Avila
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