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相关论文: Self-accelerated Universe

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The accelerated expansion of the universe has been established through observations of supernovae, the growth of structure, and the cosmic microwave background. The most popular explanation is Einsteins cosmological constant, or dynamic…

综合物理 · 物理学 2021-09-08 Steen H. Hansen

Recent astronomical observations of distant supernovae light-curves suggest that the expansion of the universe has recently begun to accelerate. Acceleration is created by an anti-gravitational repulsive stress, like that produced by a…

天体物理学 · 物理学 2009-10-31 John Barrow , Rachel Bean , Joao Magueijo

By using an unmodified Einstein gravity theory it is shown that all of the speeding-up effects taking place in the current universe are entirely due to the quantum effects associated with the background radiation or to the combination of…

天体物理学 · 物理学 2009-11-11 Pedro F. Gonzalez-Diaz , Alberto Rozas-Fernandez

The expansion of the observed universe appears to be accelerating. A simple explanation of this phenomenon is provided by the non-vanishing of the cosmological constant in the Einstein equations. Arguments are commonly presented to the…

宇宙学与河外天体物理 · 物理学 2013-05-07 Eugenio Bianchi , Carlo Rovelli

In creating his gravitational field equations Einstein unjustifiedly assumed that inertial mass, and its energy equivalent, is a source of gravity. Denying this assumption allows modifying the field equations to a form in which a positive…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Homer G. Ellis

The analysis of the data from the distant supernovae (A.Riess et al, Astron.J. {\bf 116}, 1009, (1988)) for acceleration of the expending Universe from the viewpoint of the gravitation equations proposed by one of the authors (Phys.Lett.…

天体物理学 · 物理学 2007-05-23 L. Verozub , E. Kochetov

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

In this essay, I present an alternative explanation for the cosmic acceleration which appears as a consequence of recent high redshift Supernova data. In the usual interpretation, this cosmic acceleration is explained by the presence of a…

广义相对论与量子宇宙学 · 物理学 2009-10-31 J. -F. Pascual-Sánchez

It is generally argued that the present cosmological observations support the accelerating models of the universe, as driven by the cosmological constant or `dark energy'. We argue here that an alternative model of the universe is possible…

天体物理学 · 物理学 2009-11-07 J. V. Narlikar , R. G. Vishwakarma , G. Burbidge

Recent observations of distant supernovae imply, in defiance of expectations, that the universe growth is accelerating, contrary to what has always been assumed that the expansion is slowing down due to gravity. In this paper a…

天体物理学 · 物理学 2007-05-23 M. Carmeli , S. Behar

Observations of distant supernovae indicate that the Universe is now in a phase of accelerated expansion the physical cause of which is a mystery. Formally, this requires the inclusion of a term acting as a negative pressure in the…

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

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

The hypothesis that gravitational self-binding energy may be the source for the vacuum energy term of cosmology is studied in a Newtonian Ansatz. For spherical spaces the attractive force of gravitation and the negative pressure of the…

广义相对论与量子宇宙学 · 物理学 2007-10-02 Erhard Scholz

Recent studies of Type Ia Supernovae with redshifts up to about $z~\laq~1$ reveal evidence for a cosmic acceleration in the expansion of the Universe. The most straightforward explanation to account for this acceleration is a cosmological…

广义相对论与量子宇宙学 · 物理学 2009-10-31 O. Bertolami , P. J. Martins

Based on some observations, the apparent energy, associated with gravity, of vacuums is defined, with that of normal vacuums to be zero and that of the vacuums losing some energy to be negative. An important application of the energy is its…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Yi-Ping Qin

The existence of current-time universe's acceleration is usually modeled by means of two main strategies. The first makes use of a dark energy barotropic fluid entering \emph{by hand} the energy-momentum tensor of Einstein's theory. The…

广义相对论与量子宇宙学 · 物理学 2015-07-24 Orlando Luongo , Hernando Quevedo

It is shown here that a dynamical Planck mass can drive the scale factor of the universe to accelerate. The negative pressure which drives the cosmic acceleration is identified with the unusual kinetic energy density of the Planck field. No…

广义相对论与量子宇宙学 · 物理学 2010-11-01 Janna Levin

Recent experimental results from supernovae Ia observations have been interpreted to show that the rate of expansion of the universe is increasing. Other recent experimental results find strong indications that the universe is ``flat.'' In…

天体物理学 · 物理学 2021-11-03 George A. Baker

After a short history of the $\Lambda$-term it is explained why the (effective) cosmological constant is expected to obtain contributions from short-distance-physics, corresponding to an energy scale of at least 100 GeV. The actual tiny…

天体物理学 · 物理学 2009-10-31 N. Straumann
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