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相关论文: On Friedmann's universes

200 篇论文

We construct cosmological models consisting of large numbers of identical, regularly spaced masses. These models do not rely on any averaging procedures, or on the existence of a global Friedmann-Robertson-Walker (FRW) background. They are…

广义相对论与量子宇宙学 · 物理学 2015-05-18 Timothy Clifton

The metric of an FRW universe filled with pressureless dust is shown to agree, close to any spacetime point, with a curved Newtonian-type metric where Einstein's equations simplify to those of Newtonian gravity. The agreement is shown to…

广义相对论与量子宇宙学 · 物理学 2013-12-23 Nicholas S. Manton

The general relativistic non--linear dynamics of a self--gravitating collisionless fluid with vanishing vorticity is studied in synchronous and comoving -- i.e. {\em Lagrangian} -- coordinates. Writing the equations in terms of the metric…

天体物理学 · 物理学 2007-05-23 Sabino Matarrese

Well-known to specialists but little-known to the wider audience is that Newtonian gravity can be understood as geodesic motion in space-time, where time is absolute and space is Euclidean. Newtonian cosmology formulated by Heckmann agrees…

经典物理 · 物理学 2016-09-08 J. L. McCauley

Both for the background world model and its linear perturbations Newtonian cosmology coincides with the zero-pressure limits of relativistic cosmology. However, such successes in Newtonian cosmology are not purely based on Newton's gravity,…

天体物理学 · 物理学 2009-11-13 Jai-chan Hwang , Hyerim Noh

Very straightforward arguments proving the physical non-existence of GW's and of BH's. They are so simple that even the members of the Wheelerian establishment will understand them.

综合物理 · 物理学 2007-05-23 A. Loinger

A new approach for arbitrary dimension to the Friedmann cosmological models is presented. Taking suitable changes of the parameters of the spacetime the harmonic motion equations appear, where the curvature determines the angular frequency.…

广义相对论与量子宇宙学 · 物理学 2014-03-03 Rafael M. Rubio , Juan J. Salamanca

In gravitostatics, the minimally generalized Newtonian theory, the simplest cosmological model implies a cosmological redshift with acceleration parameter -1. If the gravitational potential satisfies a wave equation, the total mass density…

天体物理学 · 物理学 2007-05-23 Peter Rastall

Using an approximate solution to the $N$-body problem in general relativity, and the \emph{principle of local isotropy at any point}, we construct a cosmological model, with zero curvature, for a universe composed uniquely by collision-less…

广义相对论与量子宇宙学 · 物理学 2014-09-11 Miguel Portilla

General relativity is a mathematical model that uses sophisticated geometry to describe simple physics. It agrees with experiment in the few tests that can be made, but the whole edifice is not physics. Instead of using observations to test…

天体物理学 · 物理学 2007-05-23 Robert L. Kurucz

Gravitation is the common underlying texture between General Relativity and Quantum Mechanics. We take gravitation as the link that can make possible the marriage between these two sciences. We use here the duality of Nature for…

综合物理 · 物理学 2008-11-26 Antonio Alfonso-Faus

It is well known that, for pressureless matter, Newtonian and relativistic cosmologies are equivalent. We show that this equivalence breaks down in the quantum level. In addition, we find some cases for which quantum Newtonian cosmology can…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Juan M. Romero , Adolfo Zamora

A theory of gravitation is presented. This theory does not relate gravitation to curvature of space-time. It explains the three standard results of general relativity in agreement with observations and suggests new experiments.

综合物理 · 物理学 2007-05-23 Irshadullah Khan

The strong proper time dilation and radial contraction in the gravitational field of compact sources leads to a frozen state of matter. It is shown that the falling particles and photons can not cross the gravitational radius due to the…

综合物理 · 物理学 2014-12-17 Zahid Zakir

The vanishing of the anomaly in the recent example of Nappi and Witten, constructed from the Wess-Zumino-Witten model based on a certain non-semisimple group, follows from a more general result valid for gravitational waves. The…

高能物理 - 理论 · 物理学 2007-05-23 C. Duval , Z. Horváth , P. A. Horváthy

In the standard approach to studying cosmological structure formation, the overall expansion of the Universe is assumed to be homogeneous, with the gravitational effect of inhomogeneities encoded entirely in a Newtonian potential. A topic…

宇宙学与河外天体物理 · 物理学 2018-02-20 William E. East , Radosław Wojtak , Tom Abel

The existence of gravitational radiation is a natural prediction of any relativistic description of the gravitational interaction. In this chapter, we focus on gravitational waves, as predicted by Einstein's general theory of relativity.…

广义相对论与量子宇宙学 · 物理学 2017-04-26 Alexandre Le Tiec , Jérôme Novak

An earlier paper [1] presented a gravity theory based on the optics of de Broglie waves rather than curved space-time. While the universe's geometry is flat, it agrees with the standard tests of general relativity. A second paper [2] showed…

天体物理学 · 物理学 2007-05-23 Kris Krogh

Null cosmic strings are shown to disturb gravitational fields of massive bodies and create outgoing gravitational waves (GW). Perturbations of the metric caused by a straight null string and a point-like massive source are found as…

广义相对论与量子宇宙学 · 物理学 2024-04-11 D. V. Fursaev , E. A. Davydov , I. G. Pirozhenko , V. A. Tainov

According to General Relativity gravity is the result of the interaction between matter and space-time geometry. In this interaction space-time geometry itself is dynamical: it can store and transport energy and momentum in the form of…

广义相对论与量子宇宙学 · 物理学 2016-11-07 J. W. van Holten