中文
相关论文

相关论文: Cosmological Redshift in FRW Metrics with Constant…

200 篇论文

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

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

The first principles analysis of the radiation by an arbitrary source in a flat Friedmann-Robertson-Walker space-time is presented. The obtained analytical solution explicitly shows that the cosmological redshift is not of kinematic origin…

经典物理 · 物理学 2009-07-03 Neil V. Budko

In this paper we suppose that the cosmological constant will change when the universe expends. For a general consideration, the cosmological constant is assumed to be a function of scale factor and Hubble constant. According to the ADM…

宇宙学与河外天体物理 · 物理学 2010-08-03 Jin-Zhang Tang , Qiang Xu

Hubble's correlation of red-shift with distance reveals that the universe is expanding, and that spacetime curvature has increased over time. And since time and space have equal status as dimensions, an object moving through time…

综合物理 · 物理学 2019-10-24 Michael Byrne

In all Friedman models, the cosmological redshift is widely interpreted as a consequence of the general-relativistic phenomenon of EXPANSION OF SPACE. Other commonly believed consequences of this phenomenon are superluminal recession…

天体物理学 · 物理学 2009-11-11 Michal Chodorowski

The cosmological redshifts z in the frequencies of spectral lines from distant galaxies as compared with their values observed in terrestrial laboratories, which are due to the scale factor a(t), frequently are interpret as a…

综合物理 · 物理学 2011-12-07 Branislav Vlahovic

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

The cosmological principle, promoting the view that the universe is homogeneous and isotropic, is embodied within the mathematical structure of the Robertson-Walker (RW) metric. The equations derived from an application of this metric to…

天体物理学 · 物理学 2014-11-18 Fulvio Melia

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

Almost a century ago, Hubble discovered the cosmological redshift of extragalactic objects. The Friedmann-Lema\^itre-Robertson-Walker (FLRW) metric was presented as a solution of Einstein's field equations for a homogeneous and isotropic…

宇宙学与河外天体物理 · 物理学 2025-02-25 Juan De Vicente

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

In this paper, we continue to examine the fundamental basis for the Friedmann-Robertson-Walker (FRW) metric and its application to cosmology, specifically addressing the question: What is the proper size of the visible universe? There are…

宇宙学与河外天体物理 · 物理学 2018-09-26 Fulvio Melia

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

We study the conditions for the consistency of the Friedmann-Robertson-Walker (FRW) metric with the dynamical Chern-Simons modified gravity. It turns out to be that in this situation the accelerated expansion of the Universe takes place,…

高能物理 - 理论 · 物理学 2011-07-14 C. Furtado , J. R. Nascimento , A. Yu. Petrov , A. F. Santos

We find an exact convergence in the local dynamics described by two supposedly antagonistic approaches in modern cosmology: one starting from an expanding universe perspective such as FLRW, the other based on a local model ignoring any…

广义相对论与量子宇宙学 · 物理学 2021-12-08 J. M. Pons , P. Talavera

In this methodological note we discuss several topics related to interpretation of some basic cosmological principles. We demonstrate that one of the key points is the usage of synchronous reference frames. The Friedmann-Robertson-Walker…

广义相对论与量子宇宙学 · 物理学 2015-11-20 A. V. Toporensky , S. B. Popov

Analysis of the gravitational source for the Schwarzschild metric indicates that the time and the radial components of the energy momentum tensor are equal. Imposing such a condition on cosmology, we propose a cosmological model that is a…

天体物理学 · 物理学 2007-05-23 Yukio Tomozawa

The real physics meaning of constant k in the Robertson-Walker metric is discussed when scalar factor R(t) is relative to time. Based on the curvature formula of the Riemannian geometry strictly, the spatial curvature of the R-W metric is…

综合物理 · 物理学 2010-06-24 Mei Xiaochun

The rather wide-spread belief that cosmological expansion of a flat 3D--space (with spatial curvature k=0) cannot be observationally distinguished from a kinematics of galaxies moving in a flat and non-expanding space is erroneous. We…

天体物理学 · 物理学 2007-05-23 Marek A. Abramowicz , Stanislaw Bajtlik , Jean-Pierre Lasota , Audrey Moudens
‹ 上一页 1 2 3 10 下一页 ›