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相关论文: What do we talk about when we speak of cosmologica…

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A common belief about big-bang cosmology is that the cosmological redshift cannot be properly viewed as a Doppler shift (that is, as evidence for a recession velocity), but must be viewed in terms of the stretching of space. We argue that,…

科普物理 · 物理学 2010-11-02 Emory F. Bunn , David W. Hogg

In cosmology one labels the time t since the Big Bang in terms of the redshift of light emitted at t, as we see it now. In this Note we derive a formula that relates t to z which is valid for all redshifts. One can go back in time as far as…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Moshe Carmeli , John G. Hartnett , Firmin J. Oliveira

The most exciting future observation in cosmology will feature a monitoring of the cosmic expansion in real time, unlike anything that has ever been attempted before. This campaign will uncover crucial physical properties of the various…

广义相对论与量子宇宙学 · 物理学 2022-12-14 Fulvio Melia

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 first and most compelling evidence of the universe's expansion was, and continues to be, the observed redshift of spectra from distant objects. This paper plays "devil's advocate" by providing an alternative explanation with elementary…

综合物理 · 物理学 2008-05-10 David Schuster

The standard interpretation of the observed redshifted spectra and luminosities towards distant astrophysical objects is that the universe is expanding, an inference which is found to be consistent with other cosmological probes as well.…

综合物理 · 物理学 2013-08-06 Meir Shimon

The main argument that Universe is currently expanding is observed redshift increase by distance. However, this conclusion may not be correct, because cosmological redshift depends only on the scaling factors, the change in the size of the…

综合物理 · 物理学 2012-07-05 Branislav Vlahovic

With the next generation of big telescopes such as the ELT and SKA it might become possible to measure changes in the expansion rate of the Universe in real time by measuring the change of the redshifts of a large number of galaxies over a…

宇宙学与河外天体物理 · 物理学 2025-12-02 Nico Roos , Eric Sluimer , Bert van den Broek

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

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

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

Recent observations of distant supernovae imply, in defiance of expectations, that the universe growth is accelerating, contrary to what has always been assumed that the expansion is slowing down due to gravity. In this paper a…

天体物理学 · 物理学 2007-05-23 M. Carmeli , S. Behar

We have had the chance to live through a fascinating revolution in measuring the fundamental empirical cosmological Hubble law. The key progress is analysed : 1) improvement of observational means (ground-based radio and optical…

宇宙学与河外天体物理 · 物理学 2018-01-10 Georges Paturel , Pekka Teerikorpi , Yurij Baryshev

The variation of the expansion rate of the Universe with time produces an evolution in the cosmological redshift of distant sources (for example quasar Lyman-$\alpha$ absorption lines), that might be directly observed by future ultra…

天体物理学 · 物理学 2009-11-13 A. Balbi , C. Quercellini

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

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

In classes on cosmology, students are often told that photons stretch as space expands, but just how physical is this picture? Does space really expand? In this article, we explore the notion of the redshift of light with Einstein's general…

科普物理 · 物理学 2016-06-08 Geraint F. Lewis

I examine the interpretation of photon redshifts in curved spacetime, as being gravitational or Doppler in origin. In Friedmann-Lema\^itre-Robertson-Walker spacetime, redshifts between comoving observers are often attributed to "expanding…

广义相对论与量子宇宙学 · 物理学 2019-11-14 Colin MacLaurin

We provide a consistency relation between cosmological observables in general relativity with the cosmological constant. Breaking of this relation at any redshift would imply the breakdown of the hypothesis of the cosmological constant as…

天体物理学 · 物理学 2009-06-23 Takeshi Chiba , Takashi Nakamura

We present the time drift of the cosmological redshift in a general spherically symmetric spacetime. We demonstrate that its observation would allow us to test the Copernican principle and so determine if our universe is radially…

天体物理学 · 物理学 2009-06-23 Jean-Philippe Uzan , Chris Clarkson , George F. R. Ellis
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