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相关论文: Redshift and Energy Conservation

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We present a derivation of the cosmological distance-redshift relation up to second order in perturbation theory. In addition, we find the observed redshift and the lensing magnification to second order. We do not require that the density…

宇宙学与河外天体物理 · 物理学 2015-06-23 Obinna Umeh , Chris Clarkson , Roy Maartens

Deviations from geodesic motion caused by gravitational radiation have been discussed in the last decades to describe the motion of particles or photons in strong fields around collapsed objects. On cosmological scale this effect, which in…

天体物理学 · 物理学 2007-08-12 Ernst Fischer

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

The observed accelerated cosmic expansion is problematic in that it seems to require an otherwise unobserved dark energy for its origin. A possible alternative explanation has been recently given, which attempts to account for this…

广义相对论与量子宇宙学 · 物理学 2011-08-26 Daniel J. Cross

More than half of the volume of our Universe is occupied by cosmic voids. The lensing magnification effect from those under-dense regions is generally thought to give a small dimming contribution: objects on the far side of a void are…

宇宙学与河外天体物理 · 物理学 2013-01-18 Krzysztof Bolejko , Chris Clarkson , Roy Maartens , David Bacon , Nikolai Meures , Emma Beynon

Discoveries in the last few years have revolutionized our knowledge of the universe and our ideas of its ultimate fate. Measurements of the expansion of the universe show that it is not slowing down under normal gravity but accelerating due…

天体物理学 · 物理学 2007-05-23 Eric V. Linder

Recent observations of the luminosity-red shift relation of distant type Ia supernovae established the fact that the expansion of the universe is accelerated. This is interpreted by saying that there exists some kind of agent (called dark…

广义相对论与量子宇宙学 · 物理学 2009-11-23 Sergio L. Cacciatori

The total red shift $z$ might be recast as a combination of the expansion red shift and a static shift due to the energy-momentum tensor non-conservation of a photon propagating through Electro-Magnetic (EM) fields. If massive, the photon…

宇宙学与河外天体物理 · 物理学 2021-01-25 Alessandro D. A. M. Spallicci , José A. Helayël-Neto , Martin López-Corredoira , Salvatore Capozziello

The cosmological constant problem has become one of the most important ones in modern cosmology. In this paper, we try to construct a model that can avoid the cosmological constant problem and have the potential to explain the apparent…

宇宙学与河外天体物理 · 物理学 2017-09-26 Shuxun Tian

The acceleration of the cosmic expansion has been discovered as a consequence of redshift Supernovae data. In the usual way, this cosmic acceleration is explained by the presence of a positive cosmological constant or quantum vacuum energy,…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. -F. Pascual-Sánchez

A new mechanism of adjustment of vacuum energy down to the observed value from an initially huge one is considered. The mechanism is based on a very strong variation of the gravitational coupling constant in very early universe. The model…

天体物理学 · 物理学 2008-11-26 A. D. Dolgov , F. R. Urban

Understanding the physical nature of the dark energy which appears to drive the accelerated expansion of the unvierse is one of the key problems in physics and cosmology today. This important problem is best studied using a variety of…

天体物理学 · 物理学 2007-05-23 Ruth A. Daly , S. G. Djorgovski

Motivated by the observed cosmic matter distribution, we present the following conjecture: due to the formation of voids and opaque structures, the average matter density on the path of the light from the well-observed objects changes from…

天体物理学 · 物理学 2010-02-23 Teppo Mattsson

Astrophysical observations are pointing out huge amounts of dark matter and dark energy needed to explain the observed large scale structures and cosmic accelerating expansion. Up to now, no experimental evidence has been found, at…

天体物理学 · 物理学 2009-11-11 S. Capozziello , V. F. Cardone , A. Troisi

The redshifts and luminosities of Type 1A supernovae are conventionally fitted with the current paradigm, which holds that the galaxies are locally stationary in an expanding metric. The fit fails unless the expansion is accelerating;…

宇宙学与河外天体物理 · 物理学 2011-01-04 Francis J. M. Farley

The Friedmann equation is derived for a Newtonian universe. Changing mass density to energy density gives exactly the Friedmann equation of general relativity. Accounting for work done by pressure then yields the two Einstein equations that…

天体物理学 · 物理学 2015-06-24 Thomas F. Jordan

Within the context of standard cosmology, an accelerating universe requires the presence of a third `dark' component of energy, beyond matter and radiation. The available data, however, are still deemed insufficient to distinguish between…

天体物理学 · 物理学 2009-08-25 Fulvio Melia

Recent measurements of the parameters of the Concordance Cosmology Model ($\Lambda$CDM) done in the low-redshift Universe with Supernovae Ia/Cepheids, and in the distant Universe done with Cosmic Microwave Background (CMB) imply different…

Recent observations on the redshift and magnitude of distant supernovae have raised fundamental questions of the cosmological structure and the development of space. Interpretation of the observations with the standard cosmology model…

天体物理学 · 物理学 2007-05-23 Tuomo Suntola , Robert Day

Some recent supernovae studies have extended the distance versus velocity Hubble plot to very high redshift, and have revealed the apparent presence of a cosmic repulsion. We show that such a repulsion has a natural origin within conformal…

天体物理学 · 物理学 2007-05-23 Philip D. Mannheim