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Quantum cosmology describes universe as a relativistic object with an evolution defined by an equation for the energy density corresponding to the least action principle: (Taganov, 2008). In quantum cosmology this equation plays the same…

综合物理 · 物理学 2008-11-26 Igor N. Taganov

The discovery that the expansion of the universe is accelerating in time is a major discovery which still awaits adequate explanation. It is generally agreed that this implies a cosmic repulsion as a result of the existence of a…

综合物理 · 物理学 2008-11-26 R. F. O'Connell

Recent observations of high-redshift supernovae seem to suggest that the global geometry of the Universe may be affected by a `cosmological constant', which acts to accelerate the expansion rate with time. But these data by themselves still…

天体物理学 · 物理学 2009-10-31 Idit Zehavi , Avishai Dekel

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 the context of the new standard LambdaCDM cosmology we resolve conflicts in the literature regarding fundamental aspects of the expansion of the universe and cosmic horizons and we link these concepts to observational tests. We derive…

天体物理学 · 物理学 2007-05-23 Tamara M. Davis

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

Cosmography is a model-independent phenomenological approach to observational cosmology, relying on Taylor series expansions of physical quantities as a function of the cosmological redshift or other analogous variables. A recent work…

宇宙学与河外天体物理 · 物理学 2025-08-27 C. J. A. P. Martins

With the next generation of big telescopes such as the ELT and SKA it might become possible to measure changes in the expansion rate of the Universe in real time by measuring the change of the redshifts of a large number of galaxies over a…

宇宙学与河外天体物理 · 物理学 2025-12-02 Nico Roos , Eric Sluimer , Bert van den Broek

We apply the property of selfsimilarity that corresponds to the concept of a fractal universe, to the dimension of time. It follows that any interval of time, given by any tick of any clock, is proportional to the age of the universe. The…

综合物理 · 物理学 2009-05-26 Antonio Alfonso-Faus

The product of two empirical constants, the dimensionless fine structure constant and the von Klitzing constant (an electrical resistance), turns out to be an exact dimensionless number. Then the accuracy and cosmological time variation (if…

综合物理 · 物理学 2014-11-20 Antonio Alfonso-Faus

The Big Bang frame of work for cosmology is a theoretical construct based upon one possible interpretation of the Hubble observation of the red shift from distant galaxies. Almost all of the scientific experimental evidence has been…

综合物理 · 物理学 2007-05-23 Antonio Alfonso-Faus

A range of cosmological observations demonstrate an accelerated expansion of the Universe, and the most likely explanation of this phenomenon is a cosmological constant. Given the importance of understanding the underlying physics, it is…

宇宙学与河外天体物理 · 物理学 2021-04-07 Karoline Loeve , Kristine Simone Nielsen , Steen H. Hansen

We advance the viewpoint that only relevant modes of the vacuum fluctuations, namely, with wavelengths conditioned by the size, homogeneity, geometry and topology of the Universe, do contribute into the cosmological constant. A formula is…

天体物理学 · 物理学 2014-10-13 V. G. Gurzadyan , She-Sheng Xue

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

A stationary line element of general relativity seems to be compatible to essential cosmological facts (though only as far as one can expect solving the nonlinear Einstein equations neglecting local cosmic evolution and all spatial…

综合物理 · 物理学 2007-05-23 Peter Ostermann

Wavepackets in quantum mechanics spread and the Universe in cosmology expands. We discuss a formalism where the two effects can be unified. The basic assumption is that the Universe is determined by a unitarily evolving wavepacket defined…

广义相对论与量子宇宙学 · 物理学 2016-04-22 Marek Czachor , Andrzej Posiewnik

We establish purely geometric or metric-based criteria for the validity of the separate universe ansatz, under which the evolution of small-scale observables in a long-wavelength perturbation is indistinguishable from a separate…

宇宙学与河外天体物理 · 物理学 2017-03-01 Wayne Hu , Austin Joyce

In the standard cosmological theory one uses the Einstein concepts of space and time as were originally introduced for the special theory of relativity and the general relativity theory. According to this approach all physical quantities…

天体物理学 · 物理学 2007-05-23 Moshe Carmeli

Astronomical observations have shown that the expansion of the universe is at present accelerating, in a way consistent with the presence of a positive cosmological constant. This is a major puzzle, because we do not understand: why the…

天体物理学 · 物理学 2007-05-23 Jordi Miralda-Escude

The idea that the cosmological term, Lambda, should be a time dependent quantity in cosmology is a most natural one. It is difficult to conceive an expanding universe with a strictly constant vacuum energy density, namely one that has…

宇宙学与河外天体物理 · 物理学 2015-03-18 Joan Sola