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相关论文: The New Redshift Interpretation Affirmed

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The standard model of cosmology posits that some time in the remote past, labelled as t=0, a Big-Bang occurred. However, it does not tell what caused the Big-Bang and subsequently the Inflation. In the present work the cause of the Big-Bang…

综合物理 · 物理学 2011-04-12 R. K. Thakur

The Hubble tension, known as a discrepancy between the local measurements vs. the CMB, SNe and galaxy clustering fits of the Hubble constant, the first measurement of the 21-centimeter high-redshift signal by EDGES, the high-redshift galaxy…

综合物理 · 物理学 2021-10-11 Davor Palle

There are two redshifts in cosmology: $z_{obs}$, the observed redshift computed via spectral lines, and the model redshift, $z$, defined by the effective FLRW scale factor. In general these do not coincide. We place observational…

宇宙学与河外天体物理 · 物理学 2015-10-06 Bruce A. Bassett , Yabebal Fantaye , Renée Hložek , Cristiano Sabiu , Mat Smith

Given there has been something where a big-bang origin of our evolutionary cosmos took place: What is the relativistic line element describing the energy density and pressure of such a pre-existing universal background? The simplest…

天体物理学 · 物理学 2013-05-14 Peter Ostermann

It has become common understanding that the recession of galaxies and the corresponding redshift of light received from them can only be explained by an expansion of the space between them and us. In this paper, for the presently favored…

宇宙学与河外天体物理 · 物理学 2012-12-27 Eckhard Rebhan

Not much by themselves, aparently. We try to reconstruct the scale factor $a(t)$ of the universe from the SNe Ia data, i.e. the luminosity distance $d_{L}(z)$, using only the cosmological principle and the assumption that gravitation is…

广义相对论与量子宇宙学 · 物理学 2017-06-19 İbrahim Semiz , A. Kazım Çamlıbel

Several key relations are derived for Cosmological General Relativity which are used in standard observational cosmology. These include the luminosity distance, angular size, surface brightness and matter density. These relations are used…

天体物理学 · 物理学 2008-11-26 John G. Hartnett , Firmin J. Oliveira

On the occasion of a century from the proposal of General relativity by Einstein, I attempt to tackle some open issues in modern cosmology, via a toy but non-trivial model. Specifically, I would like to link together: (i) the smallness of…

高能物理 - 理论 · 物理学 2016-11-23 Nick E. Mavromatos

Gravity whose nature is fundamental to the understanding of solar system, galaxies and the structure and evolution of the Universe, is theorized by the assumption of curved spacetime, according to Einstein`s general theory of relativity…

天体物理学 · 物理学 2007-10-22 Jin He

The accelerated expansion of the universe can be interpreted as a quest for satisfying holographic equipartition. It can be expressed by a simple law, $\Delta V = \Delta t\left(N_{surf}- N_{bulk}\right)$ which leads to the standard…

广义相对论与量子宇宙学 · 物理学 2019-02-06 Krishna P B , Titus K Mathew

Modifications to gravity that add additional functions of the Ricci curvature to the Einstein-Hilbert action -- collectively known as $f(R)$ theories -- have been studied in great detail. When considered as complete theories of gravity they…

天体物理学 · 物理学 2009-02-20 Simon DeDeo , Dimitrios Psaltis

We point out that $\Lambda$CDM cosmology has an ignored assumption. That is, the $\Lambda$ component of the universe moves synchronously with ordinary matters on Hubble scales. If cosmological constant is vacuum energy, this assumption may…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Ding-fang Zeng , Yi-hong Gao

Standard cosmology is constructed upon the (generally implicit) assumption of the ``large scale'' homogeneity of our Universe. Now, structures are observed at scales which become larger and larger as the observational distances increase.…

天体物理学 · 物理学 2007-05-23 Marie-Noelle Celerier

The observed accelerated cosmic expansion can be a signature of fourth\,-\,order gravity theories, where the acceleration of the Universe is a consequence of departures from Einstein General Relativity, rather than the sign of the existence…

宇宙学与河外天体物理 · 物理学 2015-06-03 Vincenzo F. Cardone , Stefano Camera , Antonaldo Diaferio

We study the present, flat isotropic universe in 1/R-modified gravity. We use the Palatini (metric-affine) variational principle and the Einstein (metric-compatible connected) conformal frame. We show that the energy density scaling…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Nikodem J. Poplawski

The Einstein Telescope and other third generation interferometric detectors of gravitational waves are projected to be operational post $2030$. The cosmological signatures of gravitational waves would undoubtedly shed light on any departure…

宇宙学与河外天体物理 · 物理学 2021-01-27 Ayan Mitra , Jurgen Mifsud , David F. Mota , David Parkinson

The dependence of luminosity distance on observed resdhift and the cosmological parameters H and q is derived for a contracting Friedmann universe with no cosmological constant. The result is consistent with recent supernovae observations.

天体物理学 · 物理学 2007-05-23 W. Q. Sumner , E. E. Vityaev

Theory of general relativity (GR) has been scrutinized by experts for almost a century and describes accurately all gravitational phenomena ranging from the solar system to the universe. However, this success is achieved provided one admits…

综合物理 · 物理学 2013-07-02 Ram Gopal Vishwakarma

Context: The cosmological concordance model ($\Lambda$CDM) matches the cosmological observations exceedingly well. This model has become the standard cosmological model with the evidence for an accelerated expansion provided by the type Ia…

宇宙学与河外天体物理 · 物理学 2017-06-19 Isaac Tutusaus , Brahim Lamine , Arnaud Dupays , Alain Blanchard

We propose and apply a new test of Einstein's Equivalence Principle (EEP) based on the gravitational redshift induced by the central super massive black hole of quasars in the surrounding accretion disk. Specifically, we compare the…

宇宙学与河外天体物理 · 物理学 2021-06-30 E. Mediavilla , J. JimÉnez-Vicente