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相关论文: Allan Sandage and the Cosmic Expansion

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The meaning of "linear expansion" is explained. Particularly accurate relative distances are compiled and homogenized a) for 246 SNe Ia and 35 clusters with v<30,000 km/s, and b) for relatively nearby galaxies with 176 TRGB and 30 Cepheid…

宇宙学与河外天体物理 · 物理学 2015-03-13 A. Sandage , B. Reindl , G. A. Tammann

Allan Sandage returned to the distance scale and the calibration of the Hubble constant again and again during his active life, experimenting with different distance indicators. In 1952 his proof of the high luminosity of Cepheids confirmed…

宇宙学与河外天体物理 · 物理学 2015-06-12 G. A. Tammann , B. Reindl

Four Hubble diagrams are combined to test for the linearity of the cosmic expansion field. The expansion rate, H_0, is found to decrease by ~5% out to 18000km/s. Beyond this distance the mean value of H_0 is close to the value at 10000km/s.…

天体物理学 · 物理学 2007-05-23 G. A. Tammann

Cepheid distances of local galaxies (<7 Mpc) are used to study the very nearby velocity field, as pioneered by Sandage (Sandage 1986) who also pointed out its remarkable properties: linearity and quietness. The new data show that the…

天体物理学 · 物理学 2007-05-23 T. Ekholm , Yu. Baryshev , P. Teerikorpi , M. O. Hanski , G. Paturel

The problem of the physical nature of the Hubble flow in the Local Volume ($D < 10$ Mpc) stated by Sandage(1986, 1999) is studied. New observational data on galaxy motions and matter distribution around the Local Group and nearby similar…

天体物理学 · 物理学 2007-05-23 Igor D. Karachentsev , Arthur D. Chernin , Pekka Teerikorpi

Recent observations of Cepheids in the Virgo cluster have bolstered the evidence that supports a Hubble constant in 70-90 km/s/Mpc range. This evidence, by and large, probes the expansion of the Universe within 100 Mpc. We investigate the…

天体物理学 · 物理学 2015-06-24 Xiangdong Shi , Lawrence M. Widrow , L. Jonathan Dursi

The validity of Hubble's law defies the determination of the center of the big bang expansion, even if it exists. Every point in the expanding universe looks like the center from which the rest of the universe flies away. In this article,…

天体物理学 · 物理学 2008-11-26 Yukio Tomozawa

A linearity test shows H_0 to decrease by 7% out to 18000 km/s. The value at 10000 km/s is a good approximation to the mean value of Ho over very large scales. The construction of the extragalactic distance scale is discussed. Field…

天体物理学 · 物理学 2007-05-23 G. A. Tammann

It is shown that the observed cmb dipole implies the existence of a center for the expansion of the universe, and that it can be explained by a combination of peculiar velocity and Hubble flow.

天体物理学 · 物理学 2007-10-30 Yukio Tomozawa

The Universe on scales $10-100~h^{-1}$ Mpc is dominated by a cosmic web of voids, filaments, sheets and knots of galaxy clusters. These structures participate differently in the global expansion of the Universe: from non-expanding clusters…

宇宙学与河外天体物理 · 物理学 2016-06-21 Krzysztof Bolejko , M. Ahsan Nazer , David L. Wiltshire

The cosmic microwave background (CMB) monopole temperature evolves with the inverse of the cosmological scale factor, independent of many cosmological assumptions. With sufficient sensitivity, real-time cosmological observations could thus…

宇宙学与河外天体物理 · 物理学 2020-05-14 Maximilian H. Abitbol , J. Colin Hill , Jens Chluba

An observer moving with respect to the cosmic rest frame should observe a concentration and brightening of galaxies in the direction of motion and a spreading and dimming in the opposite direction. The velocity inferred from this dipole…

宇宙学与河外天体物理 · 物理学 2022-06-08 Jeremy Darling

Measurements of the Hubble constant, and more generally measurements of the expansion rate and distances over the interval $0 < z < 1$, appear to be inconsistent with the predictions of the standard cosmological model ($\Lambda$CDM) given…

宇宙学与河外天体物理 · 物理学 2020-03-04 Lloyd Knox , Marius Millea

The local expansion rate of the Universe is parametrized by the Hubble constant, $H_0$, the ratio between recession velocity and distance. Different techniques lead to inconsistent estimates of $H_0$. Observations of Type Ia supernovae…

宇宙学与河外天体物理 · 物理学 2019-09-17 Inh Jee , Sherry Suyu , Eiichiro Komatsu , Christopher D. Fassnacht , Stefan Hilbert , Léon V. E. Koopmans

It has been demonstrated that a modern stage of the Universe expansion may be described in accordance with the observations within the scope of the space-time conformal geometry. The clock synchronization procedure in SR has been…

广义相对论与量子宇宙学 · 物理学 2010-01-21 L. M. Tomilchik , N. G. Kembrovskaya

Astrophysical observations indicate that the ``Local Universe" has a relatively lower matter density ($\Omega_0$) than the predictions of the standard inflation cosmology and the large-scale motions of galaxies which provide a mean mass…

天体物理学 · 物理学 2016-08-30 Xiang-Ping Wu , Zugan Deng , Zhenlong Zou , Li-Zhi Fang , Bo Qin

We have shown (Colin et al., 2019) that the acceleration of the Hubble expansion rate inferred from Type Ia supernovae (SNe Ia) is, at $3.9\sigma$ significance, a dipole approximately aligned with the CMB dipole, while its monopole…

宇宙学与河外天体物理 · 物理学 2020-03-24 Jacques Colin , Roya Mohayaee , Mohamed Rameez , Subir Sarkar

A significant tension has become manifest between the current expansion rate of our Universe measured from the cosmic microwave background by the Planck satellite and from local distance probes, which has prompted for interpretations of…

宇宙学与河外天体物理 · 物理学 2020-02-27 Lucas Lombriser

Monopole and dipole signatures of the peculiar velocity field as derived from the SFI sample of field spirals and the SCI and SC2 samples of cluster spirals are presented. The monopole exhibits no evidence of a `Hubble bubble' within 7000…

天体物理学 · 物理学 2007-05-23 R. Giovanelli

The present rate of the expansion of our Universe, the Hubble constant, can be predicted from the cosmological model using measurements of the early Universe, or more directly measured from the late Universe. But as these measurements…

宇宙学与河外天体物理 · 物理学 2020-01-14 Adam G. Riess
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