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It is noticed that the total relative density of mass in the Universe Omega_tot should exceed 1, i.e. Omega_tot=1+f^2/6 according to the field relativistic theory of gravity (RTG), which is free of the cosmological singularity and which…

天体物理学 · 物理学 2009-11-07 S. S. Gershtein , A. A. Logunov , M. A. Mestvirishvili

Basing on the field theory of gravity and observable parameters of the expanding Universe the upper limit of $m_g \leq 4.5 . 10^{-66} g$. on the value of possible graviton mass is derived.

高能物理 - 理论 · 物理学 2016-09-06 S. S. Gershtein , A. A. Logunov , M. A. Mestvirishvili

It is shown that the accelerated expansion of the universe in the framework of the relativistic theory of gravitation can be achieved by the introduction of the quintessential term in the energy-momentum tensor. The value of the minimum…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. L. Kalashnikov

In the framework of the special theory of relativity, the relativistic theory of gravitation (RTG) is constructed. The energy-momentum tensor density of all the matter fields (including gravitational one) is treated as a source of the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. A. Logunov

The last decade has seen great advancements in the field of modified gravity, motivated by the dark energy problem, or by the search for a fundamental quantum gravity theory. With a phenomenologically-driven approach, we consider dRGT…

广义相对论与量子宇宙学 · 物理学 2020-01-17 Katarina Martinovic , Mairi Sakellariadou

We present gravitation as a theory in which the coordinates are distances and velocities between galaxies. We show that there are three possibilities for the Universe to expand: decelerating, constant and accelerating, and it is shown that…

天体物理学 · 物理学 2007-05-23 Moshe Carmeli

One of the greatest challenges of science is to understand the current accelerated expansion of the Universe. In this work, we show that by considering the quantum nature of the gravitational field, its wavelength can be associated with an…

综合物理 · 物理学 2022-11-08 Tonatiuh Matos , Laura L-Parrilla

Quasidilaton massive gravity offers a physically well-defined gravitational theory with non-zero graviton mass. We present the full set of dynamical equations governing the expansion history of the universe, valid during radiation…

宇宙学与河外天体物理 · 物理学 2019-10-03 Tina Kahniashvili , Arjun Kar , George Lavrelashvili , Nishant Agarwal , Lavinia Heisenberg , Arthur Kosowsky

Under four assumptions such that 1) Einstein's theory of gravity is correct, 2) existence of foliation by geodesic slicing, 3) the trace of the extrinsic curvature, $K$, is negative at the present time in observed region, that is, the…

天体物理学 · 物理学 2016-06-08 Takashi Nakamura , Ken-ichi Nakao , Takeshi Chiba , Tetsuya Shiromizu

The gravitational equations were derived in general relativity (GR) using the assumption of their covariance relative to arbitrary transformations of coordinates. It has been repeatedly expressed an opinion over the past century that such…

广义相对论与量子宇宙学 · 物理学 2024-08-07 Alexander P. Sobolev

It was shown, that the presence of the so-called X-matter with an equation of state, which lies between limits of the strong and weak energy conditions, allows the variety of the cosmological scenarios in the relativistic theory of gravity.…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. L. Kalashnikov

We investigate the cosmological evolution in a universe governed by the extended, varying-mass, nonlinear massive gravity, in which the graviton mass is promoted to a scalar-field. We find that the dynamics, both in flat and open universe,…

广义相对论与量子宇宙学 · 物理学 2013-03-08 Emmanuel N. Saridakis

In Einstein's general relativity, gravity is mediated by a massless spin-2 metric field, and its extension to include a mass for the graviton has profound implication for gravitation and cosmology. In 2002, Finn and Sutton used the…

宇宙学与河外天体物理 · 物理学 2019-06-20 Xueli Miao , Lijing Shao , Bo-Qiang Ma

We show that the graviton acquires a mass in a de Sitter background given by $m_{g}^{2}=-{2/3}\Lambda.$ This is precisely the fine-tuning value required for the perturbed gravitational field to mantain its two degrees of freedom.

广义相对论与量子宇宙学 · 物理学 2017-08-23 M. Novello , R. P. Neves

The standard $\Lambda$-CDM predicts a growth of structures which tends to be higher than the values of redshift space distortion (RSD) measurements, if the cosmological parameters are fixed by the CMB data. In this paper we point out that…

宇宙学与河外天体物理 · 物理学 2017-03-08 Antonio De Felice , Shinji Mukohyama

We show from theoretical considerations, that if the graviton is massive, its mass is constrained to be about $10^{-32}~eV/c^2$. This estimate is consistent with those obtained from experiments, including the recent gravitational wave…

广义相对论与量子宇宙学 · 物理学 2016-10-10 Ahmed Farag Ali , Saurya Das

By applying the Palatini approach to the 1/R-gravity model it is possible to explain the present accelerated expansion of the Universe. Investigation of the late Universe limiting case shows that: (i) due to the curvature effects the…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Gilberto M. Kremer , Daniele S. M. Alves

We construct a phenomenological theory of gravitation based on a second order gauge formulation for the Lorentz group. The model presents a long-range modification for the gravitational field leading to a cosmological model provided with an…

广义相对论与量子宇宙学 · 物理学 2011-02-09 R. R. Cuzinatto , C. A. M. de Melo , L. G. Medeiros , P. J. Pompeia

The gravitational action of the smooth energy-matter components filling in the universe can affect the orbit of a planetary system. Changes are related to the acceleration of the cosmological scale size R. In a universe with significant…

天体物理学 · 物理学 2008-11-26 M. Sereno , Ph. Jetzer

It is shown that so-called dark energy could possible be a manifestation of the gravitational vortex producing the "gravitomagnetic" (GM) force field: associated with cosmic matter rotation and inertial spacetime frame dragging. The general…

综合物理 · 物理学 2018-01-24 Reva Kay Williams
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