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I will review some results of observational cosmology which critically cast doubt upon the foundations of the standard cosmology: 1) The redshifts of the galaxies are due to the expansion of the Universe; 2) The cosmic microwave background…

天体物理学 · 物理学 2007-05-23 Martin Lopez-Corredoira

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

The large-scale dynamics of the universe is generally described in terms of the time-dependent scale factor $a(t)$. To make contact with observational data, the $a(t)$ function needs to be related to the observable $z(r)$ function, redshift…

综合物理 · 物理学 2025-06-17 Jan Stenflo

Although electromagnetic and acoustic waves profoundly differ in their nature, comparing their Doppler effects is instructive and reveals persistent conceptual traps. The principle of the Doppler effect was presented by Christian Doppler in…

经典物理 · 物理学 2022-02-23 Denis Michel

We consider the possibility of an alternative gravity theory explaining the dynamics of galactic systems without dark matter. From very general assumptions about the structure of a relativistic gravity theory we derive a general expression…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Vadim V. Zhytnikov , James M. Nester

A review of the development of the concept of dark matter is given. I begin the review with the description of the discovery of the mass paradox in our Galaxy and in clusters of galaxies. In mid 1970s the amount of observational data was…

宇宙学与河外天体物理 · 物理学 2010-10-20 Jaan Einasto

We study relativistic effects, arising from the light propagation in an inhomogeneous universe. We particularly investigate the effects imprinted in a cross-correlation function between galaxy positions and intrinsic galaxy shapes (GI…

宇宙学与河外天体物理 · 物理学 2023-08-16 Shohei Saga , Teppei Okumura , Atsushi Taruya , Takuya Inoue

Dark matter has been introduced to explain many independent gravitational effects at different astronomical scales, in galaxies, groups of galaxies, clusters, superclusters and even across the full horizon. This review describes the…

宇宙学与河外天体物理 · 物理学 2010-10-19 Matts Roos

Ortiz and Ibarra-Castor (2024) have presented a "Generalized redshift formula" taking account of only energy conservation considerations. Contrary to their claim, we emphasize to invoke both energy and momentum considerations in order to…

综合物理 · 物理学 2025-04-08 Klaus Wilhelm , Bhola N. Dwivedi

According to a new tired-light cosmological model, where H(z) = H 0 (1 + z), the number density of galaxies has been nearly constant over the last 10 Gyr, at least, meaning that, as far as galaxy counts are concerned, the Universe has been…

宇宙学与河外天体物理 · 物理学 2024-01-17 Yves-Henri Sanejouand

It is shown without making use of Lorentz transformation that there exists a phenomenon of relativistic zero-frequency shift in Doppler effect for a plane wave in free space, observed in two inertial frames of relative motion, and the zero…

综合物理 · 物理学 2012-12-14 Changbiao Wang

The discovery of dark matter particles would conclusively reject the MOND theory. MOND may violate Einstein's Strong Equivalence principle. However, as we show, there is already evidence that MOND is likely not required. MOND was invented…

天体物理学 · 物理学 2007-05-23 David B. Cline

The Hubble crisis is the discrepancy in the values of the Hubble constant inferred from diverse observations in the late and early Universe, being of the order 5$\sigma$. Instead of resolution, the conflict is getting larger with further…

宇宙学与河外天体物理 · 物理学 2025-04-29 Furkan Şakir Dilsiz , Cemsinan Deliduman , Selinay Sude Binici

The Hubble law, determined from the distance modulii and redshifts of galaxies, for the past 80 years, has been used as strong evidence for an expanding universe. This claim is reviewed in light of the claimed lack of necessary evidence for…

综合物理 · 物理学 2011-11-22 John G. Hartnett

In 1997, an extension of general relativity was proposed that predicts the dark energy density \Lambda\ to vary linearly with the total number of macroscopic black holes in the universe. We explore this prediction and find that \Lambda\…

宇宙学与河外天体物理 · 物理学 2012-04-20 A. Aykutalp , M. Spaans

Cosmology is living through fascinating times, where new observations from ground and space telescopes are questioning the established paradigm, the so-called Lambda Cold Dark Matter model. The particle nature of Dark Matter is severely…

宇宙学与河外天体物理 · 物理学 2026-04-15 Juan Garcia-Bellido

In our current cosmological model, the main constituents of the Universe are dark matter and dark energy, whose nature is unknown, and for which there is no place in the standard model of particle physics. How to include dark matter and…

宇宙学与河外天体物理 · 物理学 2009-10-31 Luc Blanchet , Francoise Combes

Assuming that the Universe at higher redshifts (z \sim 4 and beyond) is consistent with LCDM model as constrained by the Planck measurements, we reanalyze the low redshift cosmological data to reconstruct the Hubble parameter as a function…

宇宙学与河外天体物理 · 物理学 2020-02-18 Koushik Dutta , Ruchika , Anirban Roy , Anjan A. Sen , M. M. Sheikh-Jabbari

The anisotropy of clustering in redshift space provides a direct measure of the growth rate of large scale structure in the Universe. Future galaxy redshift surveys will make high precision measurements of these distortions, and will…

宇宙学与河外天体物理 · 物理学 2010-10-28 Elise Jennings , Carlton M. Baugh , Silvia Pascoli

Dark matter halos represent the highest density peaks in the matter distribution. Conversely, cosmic voids are under-dense patches of the universe. Probing the mass distribution of the universe requires various approaches, including weak…

宇宙学与河外天体物理 · 物理学 2021-12-09 Md Rasel Hossen , Sonia Akter Ema , Krzysztof Bolejko , Geraint F. Lewis