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相关论文: A New Case For an Eternally Old Universe

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We show that the integration constant in the vacuum Schwarzschild solution has the unique value, alpha_0=0, accordingly Black Holes too have the same unique value of mass M0=0. Therefore the so-called Black Holes Candidates (BHC) cannot be…

综合物理 · 物理学 2009-07-16 Abhas Mitra

In this work, we outline a new general relativistic cosmology. In this cosmology, the universe originates in the infinite past from sparsely distributed neutral matter and ends in the infinite future as a hot, relativistic plasma. The…

天体物理学 · 物理学 2007-05-23 Sanjay M. Wagh

Our universe has multiple examples of unexplained gravitational losses in black holes and neutron stars. The smallest black holes of about 4 solar masses means the maximum baryon density \rho \approx 10^{17} grams/cm^3. Any collapse of the…

天体物理学 · 物理学 2025-05-02 David E. Rosenberg

We discuss cosmological models for an eternal universe. Physical observables show no singularity from the infinite past to the infinite future. While the universe is evolving, there is no beginning and no end - the universe exists forever.…

广义相对论与量子宇宙学 · 物理学 2014-08-27 C. Wetterich

Both from gravitational (G) experiments and from a new theoretical approach based on a particle model it is proved that the classical invariability of the bodies, after a change of relative rest-position with respect to other bodies, it is…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Rafael A. Vera

It is attractive to suppose for several astrophysical reasons that the universe has close to the critical density in light (~30 eV) neutrinos which decay radiatively with a lifetime of ~10^{23} sec. In such a cosmology the universe is…

天体物理学 · 物理学 2011-02-16 J. A. Adams , Subir Sarkar , D. W. Sciama

An initial state for the observable universe consisting of a finite region with a large vacuum energy will break-up due to near horizon quantum critical fluctuations. This will lead to a Friedmann-like early universe consisting of an…

宇宙学与河外天体物理 · 物理学 2010-05-04 George Chapline

The fundamental paradox of the incompatibility of the observed large-scale uniformity of the Universe with the fact that the age of the Universe is finite is overcome by the introduction of an initial a period of superluminal expansion of…

高能物理 - 唯象学 · 物理学 2010-11-02 Konstantinos Dimopoulos

Cosmological observations strongly suggest the presence of dark energy which comprises the majority of the current energy density of the universe. The equation of state relating the pressure and energy density of this dark energy, p = w…

天体物理学 · 物理学 2007-05-23 Eric Gawiser

Using an approximate solution to the $N$-body problem in general relativity, and the \emph{principle of local isotropy at any point}, we construct a cosmological model, with zero curvature, for a universe composed uniquely by collision-less…

广义相对论与量子宇宙学 · 物理学 2014-09-11 Miguel Portilla

An alternative cosmological model is presented, which avoids the requirement of dark energy and dark matter. Based on the proposition that energy conservation should be valid not only locally but also globally, the energy tensor of general…

综合物理 · 物理学 2007-08-30 Ernst Fischer

Although the current galaxy models yield calculations consistent with much of the data, many irregularities exist, exceptions have been found to the current models, the $\Lambda$CDM model apparently fails on galaxy scales, dark matter…

天体物理学 · 物理学 2007-05-23 John C. Hodge

Over the past three years we have determined the basic features of our Universe. It is spatially flat; accelerating; comprised of 1/3 a new form of matter, 2/3 a new form of energy, with some ordinary matter and a dash of massive neutrinos;…

天体物理学 · 物理学 2008-11-26 Michael S. Turner

I will review some results of observational cosmology which critically cast doubt upon the foundations of the standard cosmology: 1) The redshifts of the galaxies are due to the expansion of the Universe; 2) The cosmic microwave background…

天体物理学 · 物理学 2007-05-23 Martin Lopez-Corredoira

We propose that the totality of dark matter in the universe might ascribe its origin to one of the key properties of cosmological inflation, that it may be eternal: regions that at the end of the primordial accelerated expansion of the…

宇宙学与河外天体物理 · 物理学 2026-02-10 G. Franciolini , M. Peloso , A. Riotto

Over the past three years we have determined the basic features of the Universe -- spatially flat; accelerating; comprised of 1/3 a new form of matter, 2/3 a new form of energy, with some ordinary matter and a dash of massive neutrinos; and…

天体物理学 · 物理学 2009-11-07 Michael S. Turner

There are many observational evidences for the existence of massive compact condensations in the range $10^6 -10^{10} M_\odot$ at the core of various galaxies. At present such condensations are commonly interpreted as Black Holes (BHs).…

天体物理学 · 物理学 2007-05-23 Abhas Mitra

If our universe was born as a baby universe on the other side of the event horizon of a black hole existing in a parent universe, then the corresponding white hole at rest provides the absolute frame of reference in the universe. In this…

科普物理 · 物理学 2025-06-02 Nikodem Popławski

We develop a cosmological theory in which the evolution of the universe is controlled by the cosmological constant and dominated by the associated vacuum energy. The universe starts as a classical de Sitter space with an infinite effective…

综合物理 · 物理学 2023-03-21 J. M. Greben

Equations of cosmic dynamics for a model of the opaque Universe are derived and tested on supernovae (SNe) Ia observations. The model predicts a cyclic expansion/contraction evolution of the Universe within a limited range of scale factors.…

综合物理 · 物理学 2019-02-28 Vaclav Vavrycuk
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