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相关论文: The Apparent Fractal Conjecture

200 篇论文

The structures formation of the Universe appears as if it were a classically self-similar random process at all astrophysical scales. An agreement is demonstrated for the present hypotheses of segregation with a size of astrophysical…

天体物理学 · 物理学 2008-11-26 G. Iovane , E. Laserra , F. S. Tortoriello

According to the theory of general relativity, masses deflect light in a way similar to convex glass lenses. This gravitational lensing effect is astigmatic, giving rise to image distortions. These distortions allow to quantify cosmic…

宇宙学与河外天体物理 · 物理学 2016-12-21 Matthias Bartelmann , Matteo Maturi

Density fluctuations in the matter distribution lead to distortions of the images of distant galaxies through weak gravitational lensing effects. This provides an efficient probe of the cosmological parameters and of the density field. In…

天体物理学 · 物理学 2007-05-23 P. Valageas

We discuss the problem of galaxy correlations by considering the various methods by which this information can be obtained. We focus in particular on the volume limited three dimensional samples and discuss a new way to increase the scale…

天体物理学 · 物理学 2007-05-23 L. Pietronero , M. Montuori , F. Sylos Labini

It is shown that the observed fractal distribution of galaxies is, in fact, consistent with homogeneity of the Universe and observational limits on $ \Delta T/T$, if the presence of dark matter and dark charge predicted by the Modified…

天体物理学 · 物理学 2009-11-07 A. A. Kirillov

The fractal properties of models of randomly placed $n$-dimensional spheres ($n$=1,2,3) are studied using standard techniques for calculating fractal dimensions in empirical data (the box counting and Minkowski-sausage techniques). Using…

凝聚态物理 · 物理学 2009-10-28 Daniel A. Hamburger , Ofer Biham , David Avnir

From the standpoint of theoretical physics we can treat Newtonian cosmology as a problem in nonlinear dynamics. The attempt to average the density, in search of a method of making contact between theory and observation, is replaced by the…

天体物理学 · 物理学 2007-05-23 J. L. McCauley

Two-point correlation function of galaxy distribution shows that the structure in the present Universe is scale-free up to a certain scale (at least several tens Mpc), which suggests that a fractal structure may exist. If small primordial…

天体物理学 · 物理学 2009-10-31 Takayuki Tatekawa , Kei-ichi Maeda

We discuss various questions which arise when one considers the central projection of three dimensional fractal sets (galaxy catalogs) onto the celestial globe. The issues are related to how fractal such projections look. First we show that…

In this paper, we pose a hypothesis that the structure of communities in complex networks may result from their latent fractal properties. This hypothesis is based not only on the general observation that many real networks have multilevel…

物理与社会 · 物理学 2023-09-21 Mateusz Samsel , Kordian Makulski , Michał Łepek , Agata Fronczak , Piotr Fronczak

Observational evidence shows that gravitational lensing induces an angular correlation between the distribution of galaxies and much more distant QSOs. We use weak gravitational lensing theory to calculate this angular correlation, updating…

天体物理学 · 物理学 2009-10-31 Antonio C. C. Guimaraes , Carsten van de Bruck , Robert H. Brandenberger

We study the (newtonian) gravitational force distribution arising from a fractal set of sources. We show that, in the case of real structures in finite samples, an important role is played by morphological properties and finite size…

天体物理学 · 物理学 2019-08-17 A. Gabrielli , F. Sylos Labini , S. Pellegrini

Over the past two decades or so, it has become increasingly appparent that, out to quite large distances, galaxies are distributed in a quasi-fractal fashion with fractal dimension $D \approx 2$. Whether or not this behaviour continues onto…

天体物理学 · 物理学 2007-05-23 D F Roscoe

Modern astronomical observations in cosmology provide increasingly strong evidence that the expansion of the Universe is accelerating. Explanations of the cosmic acceleration within the framework of general relativity use the hypothesis…

综合物理 · 物理学 2015-04-10 I. K. Rozgacheva , A. A. Agapov

Models of structure formation in the universe postulate that matter distributions observed today in galaxy catalogs arise, through a complex non-linear dynamics, by gravitational evolution from a very uniform initial state. Dark matter…

统计力学 · 物理学 2009-11-11 Luciano Pietronero , Francesco Sylos Labini

We review a cosmology in which particles are fluctuationally created from a background Zero Point Field. This cosmology is consistent with recent observations of an ever expanding and accelerating universe, as also the recently confirmed…

综合物理 · 物理学 2015-06-26 B. G. Sidharth

The nearest neighbor distribution (Chandrasekhar 1943) is generalized to fractal stellar systems.For such systems an asymptotic distribution of the magnitude of large random forces and a formula for the effective mean interparticle spacing…

星系天体物理 · 物理学 2016-06-01 Oleg V. Chumak , Alexey S. Rastorguev

We revise the statistical properties of the primordial cosmological density anisotropies that, at the time of matter radiation equality, seeded the gravitational development of large scale structures in the, otherwise, homogeneous and…

高能物理 - 唯象学 · 物理学 2008-11-26 David H. Oaknin

CONTEXT: Cosmic voids are observed in the distribution of galaxies and, to some extent, in the dark matter distribution. If these distributions have fractal geometry, it must be reflected in the geometry of voids; in particular, we expect…

天体物理学 · 物理学 2008-02-05 Jose Gaite

An empirically validated, phenomenological model relating the parameters of an astronomical body to the stochastic fluctuations of its granular components is generalized in terms of fractal scaling laws. The mass of the particle…

综合物理 · 物理学 2008-11-06 Scott Funkhouser , Nicola Pugno