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相关论文: Hubble Redshift

200 篇论文

A higher value of Hubble constant has been obtained from measurements with nearby Type Ia supernovae, than that obtained at much higher redshift. With the peculiar motions of their hosts, we find that the matter content at such low redshift…

宇宙学与河外天体物理 · 物理学 2013-07-25 Shuang-Nan Zhang , Yin-Zhe Ma

We study some observational consequences of a recently proposed scale--dependent cosmological model for an inhomogeneous Universe. In this model the Universe is pictured as being inside a highly dense and rapidly expanding shell with the…

高能物理 - 唯象学 · 物理学 2009-10-28 C. W. Kim , T. H. Lee , J. Song

If gravitons are super-strong interacting particles and the low-temperature graviton background exists, the basic cosmological conjecture about the Dopplerian nature of redshifts may be false: a full magnitude of cosmological redshift would…

天体物理学 · 物理学 2014-10-13 Michael A. Ivanov

The Hubble diagram is one of the cornerstones of observational cosmology. It is usually analysed assuming that, on average, the underlying relation between magnitude and redshift matches the prediction of a…

宇宙学与河外天体物理 · 物理学 2017-04-05 Pierre Fleury , Chris Clarkson , Roy Maartens

The luminosity-redshift relation of cosmological standard candles provides information about the relative energy composition of our Universe. In particular, the observation of type Ia supernovae up to redshift of z~2 indicate a universe…

高能物理 - 唯象学 · 物理学 2009-09-02 Markus Ahlers

We determine the Hubble constant $H_0$ precisely ($2.3\%$ uncertainty) in a manner independent of cosmological model through Gaussian process regression, using strong lensing and supernova data. Strong gravitational lensing of a variable…

宇宙学与河外天体物理 · 物理学 2020-06-08 Kai Liao , Arman Shafieloo , Ryan E. Keeley , Eric V. Linder

In this paper we calculate the luminosity distance - redshift relation for a special type of flat Friedmann brane with cosmological constant. This special case is singled out by its simplicity, the luminosity distance being given in terms…

天体物理学 · 物理学 2007-05-23 Botond Nagy , Zoltán Keresztes

The results from the Supernova Cosmology Project indicate a relation between cosmic distance and redshift that corresponds to an accelerating Universe, and, as a consequence, the presence of an energy component with negative pressure. This…

天体物理学 · 物理学 2007-05-23 Daniel Enstrom , Sverker Fredriksson , Johan Hansson

Analysis of type 1a supernovae observations out to a redshift of $z$=1.6 shows that there is good agreement between the light-curve widths and $(1+z)$ which is usually interpreted as a strong support for time dilation due to an expanding…

综合物理 · 物理学 2010-09-12 David F. Crawford

In a series of articles, we have shown that the newly discovered plasma-redshift cosmology gives a simpler, more accurate and consistent explanation of many cosmological phenomena than the big-bang cosmology. The SNe Ia observations are in…

天体物理学 · 物理学 2007-05-23 Ari Brynjolfsson

On small scales the observable Universe is highly inhomogeneous, with galaxies and clusters forming a complex web of voids and filaments. The optical properties of such configurations can be quite different from the perfectly smooth…

宇宙学与河外天体物理 · 物理学 2017-07-19 Viraj A. A. Sanghai , Pierre Fleury , Timothy Clifton

The emergence of a highly improbable coincidence in cosmological observations speaks to a remarkably simple cosmic expansion. Compelling evidence now suggests that the Universe's gravitational horizon, coincident with the better known…

综合物理 · 物理学 2019-05-21 Fulvio Melia

In any Big Bang cosmology, the frequency $\omega$ of light detected from a distant source is continuously and linearly changing (usually redshifting) with elapsed observer's time $\delta t$, because of the expanding Universe. For small…

天体物理学 · 物理学 2008-05-19 Richard Lieu

Recently E. Harrison has argued the Red Shift distance law proposed by Hubble and velocity-distance law developed later on theoretical grounds has no general proof demonstrating the two laws are actually equivalent. It is the purpose of…

综合物理 · 物理学 2010-07-28 Walter J. Christensen

A nonhomogeneous universe with vacuum energy, but without spacetime expansion, is utilized together with gravitational and Doppler redshifts as the basis for proposing a new interpretation of the Hubble relation and the 2.7K Cosmic…

天体物理学 · 物理学 2009-10-30 Robert V. Gentry

Using the relation between distance modulus $(m - M)$ and redshift $z$, deduced from Friedman- Robertson-Walker (FRW) metric and assuming different values of deceleration parameter $q_0$. We constrained the Hubble parameter $h$. The…

综合物理 · 物理学 2016-06-03 C. C. Onuchukwu , A. C. Ezeribe

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

Redshift drift is the phenomenon whereby the observed redshift between an emitter and observer comoving with the Hubble flow in an expanding FLRW universe will slowly evolve -- on a timescale comparable to the Hubble time. There are…

广义相对论与量子宇宙学 · 物理学 2022-10-04 Francisco S. N. Lobo , Jose Pedro Mimoso , Matt Visser

The redshift-distance modulus relation, the Hubble Diagram, derived from Cosmological General Relativity has been extended to arbitrarily large redshifts. Numerical methods were employed and a density function was found that results in a…

综合物理 · 物理学 2008-10-03 John G. Hartnett

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