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相关论文: The Cosmic Time in Terms of the Redshift

200 篇论文

From the first observations made by Slipher, our understanding and interpretation of the cosmological redshift was evolving until reaching the current consensus, through the expanding universe and the emergence of modern physical cosmology…

宇宙学与河外天体物理 · 物理学 2020-02-28 Gabriel R. Bengochea

The large-scale dynamics of the universe is generally described in terms of the time-dependent scale factor $a(t)$. To make contact with observational data, the $a(t)$ function needs to be related to the observable $z(r)$ function, redshift…

综合物理 · 物理学 2025-06-17 Jan Stenflo

We present explicit expressions for the calculation of cosmological look back time, for zero cosmological constant and arbitrary density parameter $\Omega$, which, in the limit as redshift becomes infinite, give the age of the universe. The…

天体物理学 · 物理学 2007-05-23 Kevin Krisciunas

This paper presents alternative ideas on the physics of time that lead to a new interpretation of cosmological redshifts. These ideas are based on the close relationship between the speed of time and entropy processes in our universe. I…

天体物理学 · 物理学 2009-11-06 Vladimir I. Garaimov

In the standard cosmological theory one uses the Einstein concepts of space and time as were originally introduced for the special theory of relativity and the general relativity theory. According to this approach all physical quantities…

天体物理学 · 物理学 2007-05-23 Moshe Carmeli

The notion of time in cosmology is revealed through an examination of transition matrix elements of radiative processes occurring in the cosmos. To begin with, the very concept of time is delineated in classical physics in terms of…

广义相对论与量子宇宙学 · 物理学 2009-10-30 R. Brout , R. Parentani

Using cosmological relativity theory, we derive the formula for the cosmological redshift written explicitly in terms of 1 - "Omega", where "Omega" = "rho"/"rho"_c is the ratio of the average mass density to the critical "closure" density.…

天体物理学 · 物理学 2007-05-23 Moshe Carmeli

A photon's observed wavelength tells an astronomical detector about the amount of position information obtained by observing that photon. This amount of position information may depend on time in a way which, to first order over distances…

天体物理学 · 物理学 2007-05-23 Frederick W. Kantor

The redshift of galaxies is in general explained by the expansion of space. The flat space time theory of gravitation suggests an additional interpretation. In this theory gravitation is explained analogously to Maxwell's theory on a flat…

综合物理 · 物理学 2007-05-31 Walter Petry

A recent cosmological model is recapitulated which deduces the correct mass, radius and age of the universe as also the Hubble constant and other well known apparently coincidental relations. It also predicts an ever expanding accelerating…

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

On the base of the hypothesis about a nature of the time as a dimension of alien Universe relation between alteration of time with coordinates $\frac{\partial t}{\partial x}$ and time {t} offered: $ \frac{\partial t} {\partial x} = H_{t} t$…

综合物理 · 物理学 2007-05-23 L. Ya. Kobelev

The time-redshift relation of Carmeli et al. differs from that of the standard flat LambdaCDM model by more than 500 million years for 1 < z < 4.5.

广义相对论与量子宇宙学 · 物理学 2008-11-26 Alan Macdonald

Time has always played a crucial role in cosmology. I review some of the aspects of the present cosmological model which are more directly related to time, such as: the definition of a cosmic time; the existence of typical timescales and…

物理学史与哲学 · 物理学 2017-03-22 A. Balbi

The meaning of the expansion of the universe, or the `expansion of space,' is explored using two phenomena: the motion of a test particle against a homogeneous background and the cosmological redshift. Contrary to some expectations, a…

天体物理学 · 物理学 2007-05-23 Alan B. Whiting

A cosmology calculator that computes times and distances as a function of redshift for user-defined cosmological parameters is available on the World Wide Web. This note gives the formulae used by the cosmology calculator and discusses some…

天体物理学 · 物理学 2010-04-21 Edward L. Wright

The contribution of cosmological perturbations to the time drift of the cosmological redshift is derived. It is shown that the dominant correction arises from the local acceleration of both the emitter and the observer. The amplitude of…

天体物理学 · 物理学 2008-12-18 Jean-Philippe Uzan , Francis Bernardeau , Yannick Mellier

The relativity of cosmic time is developed within the framework of Cosmological Relativity in five dimensions of space, time and velocity. A general linearized metric element is defined to have the form $ds^2 = (1+\phi) c^2 dt^2 - dr^2 +…

综合物理 · 物理学 2016-05-30 Firmin J. Oliveira

We propose that cosmological time is {\it effectively} the conjugate of the constants of nature. Different definitions of time arise, with the most relevant related to the constant controlling the dynamics in each epoch. The Hamiltonian…

广义相对论与量子宇宙学 · 物理学 2021-06-30 Joao Magueijo

It is a remarkable fact that all processes occurring in the observable Universe are irreversible, whereas the equations through which the fundamental laws of physics are formulated are invariant under time reversal. The emergence of…

综合物理 · 物理学 2015-05-28 Gustavo E. Romero , Daniela Pérez

Redshift drift refers to the phenomena that redshift of cosmic objects is a function of time. Measurement of redshift drift is of fundamental importance in physical cosmology and can be utilized to distinguish different cosmological models.…

广义相对论与量子宇宙学 · 物理学 2020-06-16 Snehasish Bhattacharjee , P. K. Sahoo
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