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相关论文: An Alternative Explanation for Cosmological Redshi…

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The energy conditions give upper bounds on the luminosity distance. We apply these upper bounds to the 192 essence supernova Ia data to show that the Universe had experienced accelerated expansion. This conclusion is drawn directly from the…

天体物理学 · 物理学 2008-11-26 Yungui Gong , Anzhong Wang , Qiang Wu , Yuan-Zhong Zhang

In this paper we present an alternative explanation to the acceleration of the universe and the dark energy problems in terms of the Friedmann Thermodynamics. This model has the capability of making definite predictions in-line with the…

天体物理学 · 物理学 2007-05-23 Selcuk Bayin

The coincidence problem of late cosmic acceleration constitutes a serious riddle with regard to our understanding of the evolution of the Universe. Here we argue that this problem may someday be solved -or better understood- by expressing…

天体物理学 · 物理学 2008-11-26 Sergio del Campo , Ramon Herrera , Diego Pavon

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

The discovery that the Universe is accelerating in its expansion has brought the basic concept of cosmic expansion into question. An analysis of the evolution of this concept suggests that the paradigm that was finally settled into prior to…

物理学史与哲学 · 物理学 2014-09-12 Daryl Janzen

Subject of this contribution is to demonstrate that the observed faintness of the supernovae at the high redshift can be considered as a manifestation of quantum effects at cosmological scales. We show that observed redshift distribution of…

天体物理学 · 物理学 2007-05-23 V. V. Kuzmichev

The principles of General Relativity allow for a non-vanishing cosmological constant, which can possibly be interpreted at least partially in terms of quantum-fluctuations of matter fields. Depending on sign and magnitude it can cause…

天体物理学 · 物理学 2007-05-23 Domenico Giulini , Norbert Straumann

Understanding of the nature of dark energy, which appears to drive the expansion of the universe, is one of the central problems of physical cosmology today. In an earlier paper [Daly & Djorgovski (2003)] we proposed a novel method to…

天体物理学 · 物理学 2009-11-10 Ruth A. Daly , S. G. Djorgovski

Recently [arXiv:astro-ph/0612155] we presented a formal mathematical proof that, contrary to a widespread misconception, cosmological expansion cannot be understood as the motion of galaxies in non-expanding space. We showed that the…

天体物理学 · 物理学 2008-12-18 Marek A. Abramowicz , Stanislaw Bajtlik , Jean-Pierre Lasota , Audrey Moudens

The expansion of the Universe is the basis of modern cosmology. This chapter outlines the theory behind the expansion of the universe, including the cosmological principle, distances, velocities, and accelerations. We provide basic…

宇宙学与河外天体物理 · 物理学 2025-09-15 Tamara M. Davis

The cosmological redshift drift promises to be the first observable directly measuring the evolution of the cosmic expansion rate and should be detectable with upcoming surveys by the Square Kilometre Array and the Extremely Large…

宇宙学与河外天体物理 · 物理学 2025-11-13 Alexander Oestreicher , Chris Clarkson , Julian Adamek , Sofie Marie Koksbang

Many of the general-relativity-tests such as bending of light near a star and gravitational red/blue shift are explained without general-relativity and without Newtonian-approach. The author first casts doubts on both, the Newtonian and the…

综合物理 · 物理学 2007-05-23 Dr. R. C. Gupta

A new component of the Universe which leads to an accelerated cosmic expansion is found from the measurements of distances to high-redshift type Ia supernovae. We describe the method and the results obtained from the observations of distant…

天体物理学 · 物理学 2007-05-23 Bruno Leibundgut , Gertrud Contardo , Patrick Woudt , Jason Spyromilio

Under the assumption that General Relativity (GR) correctly describes the phenomenology of our Universe, astronomical observations provide compelling evidence that (1) the dynamics of cosmic structure is dominated by dark matter (DM), an…

天体物理学 · 物理学 2008-02-19 A. Diaferio

A photon's observed wavelength tells an astronomical detector about the amount of position information obtained by observing that photon. This amount of position information may depend on time in a way which, to first order over distances…

天体物理学 · 物理学 2007-05-23 Frederick W. Kantor

We show that the Supernovae results, implying evidence for an accelerating Universe, may be closely related to the recent discovery of redshift dependence in the fine structure constant $\alpha$. The link is a class of varying speed of…

天体物理学 · 物理学 2009-10-31 John D. Barrow , Joao Magueijo

In two recent papers, Abramowicz et al. claim that the expansion of the Universe can be interpreted only as the expansion of space. In fact, what they really prove is that the cosmological expansion cannot be described in terms of real…

天体物理学 · 物理学 2008-12-23 Michał Chodorowski

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

The exploration of the redshift drift, a direct measurement of cosmological expansion, is expected to take several decades of observation with stable, sensitive instruments. We introduced a new method to probe cosmology which bypasses the…

宇宙学与河外天体物理 · 物理学 2023-08-16 Chengyi Wang , Krzysztof Bolejko , Geraint F. Lewis

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