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相关论文: Redshift and Energy Conservation

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A hypotheses of energy loss for polarization of e-e+ vacuum by a photon passing interstellar space is considered. An excitation and relaxation of vacuum can't run with speed of light due to very small but finite fraction of e-e+ pair mass…

综合物理 · 物理学 2011-03-08 Yuriy A. Yatsunenko , Julian A. Budagov

The formula describing the explicit red-shift dependence for the distance covered by a signal in the expanding space, and also the expressions for Hubble law have been derived directly from the conformal group transformations taking into…

广义相对论与量子宇宙学 · 物理学 2015-03-19 L. M. Tomilchik

The expansion rate of the Universe changes with time, initially slowing (decelerating) when the universe was matter dominated, because of the mutual gravitational attraction of all the matter in it, and more recently speeding up…

宇宙学与河外天体物理 · 物理学 2013-09-17 Muhammad Omer Farooq

The cosmographic technique is a powerful model-independent tool for distinguishing between competing cosmological scenarios. The key strengths and weaknesses of standard cosmography are discussed in view of healing the convergence problem…

宇宙学与河外天体物理 · 物理学 2022-12-01 Salvatore Capozziello , Rocco D'Agostino

The interpretation of the expanding universe as an expansion of space has recently been challenged. From the geodesic equation in Friedmann universe models and the empty Milne model, we argue that a Newtonian or special relativistic…

天体物理学 · 物理学 2009-11-11 Oyvind Gron , Oystein Elgaroy

The clustering of galaxies observed in future redshift surveys will provide a wealth of cosmological information. Matching the signal at different redshifts constrains the dark energy driving the acceleration of the expansion of the…

In cosmology based on general relativity, the universe is modeled as a fluid. The transition from the Einstein field equation to its large-scale (cosmological) version is thus analogous to the transition, for a system consisting of a large…

综合物理 · 物理学 2018-10-18 Gregory Ryskin

We present an impact of coupling between dark matter and a scalar field, which might be responsible for dark energy, on measurements of redshift-space distortions. We point out that, in the presence of conformal and/or disformal coupling,…

宇宙学与河外天体物理 · 物理学 2018-08-22 Rampei Kimura , Teruaki Suyama , Masahide Yamaguchi , Daisuke Yamauchi , Shuichiro Yokoyama

A new redshift formula is obtained considering the longitudinal Doppler effect in the de Sitter expanding universe where the relative geodesic motion is governed by the Lorenzian isometries of our new de Sitter relativity [I. I. Cot\u…

广义相对论与量子宇宙学 · 物理学 2021-02-24 Ion I. Cotaescu

A new interaction, plasma redshift, is derived, which is important only when photons penetrate a hot, sparse electron plasma. The derivation of plasma redshift is based entirely on conventional axioms of physics. When photons penetrate a…

天体物理学 · 物理学 2009-09-29 Ari Brynjolfsson

In this letter, the old issue of whether redshifts of quasars are of cosmological origin is investigated. We make a plot of absorption redshifts versus emission redshifts for quasars with large amounts of data. Our study shows that, almost…

天体物理学 · 物理学 2007-05-23 Yi-Ping Qin , Guang-Zhong Xie , Xue-Tang Zheng , En-Wei Liang

The luminosity distance-redshift relation is one of the fundamental tools of modern cosmology. We compute the luminosity distance-redshift relation in a perturbed flat matter-dominated Universe, taking into account the presence of…

天体物理学 · 物理学 2009-11-10 Enrico Barausse , Sabino Matarrese , Antonio Riotto

The exploration of the redshift drift, a direct measurement of cosmological expansion, is expected to take several decades of observation with stable, sensitive instruments. We introduced a new method to probe cosmology which bypasses the…

宇宙学与河外天体物理 · 物理学 2023-08-16 Chengyi Wang , Krzysztof Bolejko , Geraint F. Lewis

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

This article presents a simple model that reproduces key concepts of modern cosmology within the framework of special relativity, at a level that is suitable for an undergraduate or high school setting. The model includes cosmic expansion…

广义相对论与量子宇宙学 · 物理学 2019-01-14 Markus Pössel

Motivated by results implying that the constituents of dark matter (DM) might be collisional, we consider a cosmological (toy-) model, in which the DM itself possesses some sort of thermodynamic properties. In this case, not only can the…

广义相对论与量子宇宙学 · 物理学 2015-03-19 Kostas Kleidis , Nicholas K. Spyrou

Mapping the expansion history of the universe is a compelling task of physical cosmology, especially in the context of the observational evidence for the recent acceleration of the universe, which demonstrates that canonical theories of…

宇宙学与河外天体物理 · 物理学 2022-11-30 B. A. R. Rocha , C. J. A. P. Martins

Earlier studies have conjectured that redshift drift is described by spatially averaged quantities and thus becomes positive if the average expansion of the Universe accelerates. This conclusion is reevaluated here by considering exact…

宇宙学与河外天体物理 · 物理学 2019-11-27 S. M. Koksbang

We use standard general relativity to illustrate and clarify several common misconceptions about the expansion of the Universe. To show the abundance of these misconceptions we cite numerous misleading, or easily misinterpreted, statements…

天体物理学 · 物理学 2009-11-10 Tamara M. Davis , Charles H. Lineweaver

Cosmic acceleration is explained quantitatively, purely in general relativity, as an apparent effect due to quasilocal gravitational energy differences that arise in the decoupling of bound systems from the global expansion of the universe.…

广义相对论与量子宇宙学 · 物理学 2008-11-26 David L. Wiltshire