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相关论文: Fractal universe

200 篇论文

We discuss a cosmological model where the universe shrinks rather than expands during the radiation and matter dominated periods. Instead, the Planck mass and all particle masses grow exponentially, with the size of atoms shrinking…

宇宙学与河外天体物理 · 物理学 2013-11-13 C. Wetterich

Observations of microwave background fluctuations can yield information not only about the geometry of the universe, but potentially about the topology of the universe. If the universe is negatively curved, then the characteristic scale for…

天体物理学 · 物理学 2009-10-30 Neil J. Cornish , David N. Spergel , Glenn D. Starkman

In this paper we attempt to answer to the question: can cosmic acceleration of the Universe have a fractal solution? We give an exact solution of a Lema\^itre-Tolman-Bondi (LTB) Universe based on the assumption that such a smooth metric is…

宇宙学与河外天体物理 · 物理学 2019-01-30 Leonardo Cosmai , Giuseppe Fanizza , Francesco Sylos Labini , Luciano Pietronero , Luigi Tedesco

The study of the properties of cosmic structures in the universe is one of the most fascinating subject of the modern cosmology research. Far from being predicted, the large scale structure of the matter distribution is a very recent…

统计力学 · 物理学 2016-11-23 L. Pietronero , M. Bottaccio , M. Montuori , F. Sylos Labini

It is shown that any spatially flat and isotropic universe undergoing accelerated expansion driven by a self-interacting scalar field can be directly related to a contracting, decelerating cosmology. The duality is made manifest by…

广义相对论与量子宇宙学 · 物理学 2009-11-10 James E. Lidsey

We investigate the fractal structure of $2d$ quantum gravity coupled to matter by measuring the distributions of so-called baby universes. We demonstrate that the method works well as long as $c \leq 1$. For $c >1$ it is not clear what…

高能物理 - 理论 · 物理学 2009-10-22 J. Ambjorn , G. Thorleifsson

We investigate the fractal structure of $2d$ quantum gravity coupled to matter by measuring the distributions of so-called baby universes. We demonstrate that the method works well as long as $c \leq 1$. For $c >1$ it is not clear what…

高能物理 - 格点 · 物理学 2015-06-25 J. Ambjorn , G. Thorleifsson

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

With a method in which the Friedmann equation is written in a form such that evolution of the scale factor can be treated as that of a particle in a "potential", we classify all possible cosmic evolutions in the DGP braneworld scenario with…

广义相对论与量子宇宙学 · 物理学 2012-10-12 Kaituo Zhang , Puxun Wu , Hongwei Yu

Clouds in observations are fractals: they show self-similarity across scales ranging from one to 1000 km. This includes individual storms and large-scale cloud structures typical of organised convection. It is not known whether global…

大气与海洋物理 · 物理学 2022-01-05 Hannah M. Christensen , Oliver G. A. Driver

We discuss correlation properties of a general mass density field introducing a classification of structures based on their complexity. Standard cosmological models for primordial mass fluctuations are characterized by a sort of large-scale…

天体物理学 · 物理学 2009-11-10 Francesco Sylos Labini , Andrea Gabrielli

We show a relation between fractional calculus and fractals, based only on physical and geometrical considerations. The link has been found in the physical origins of the power-laws, ruling the evolution of many natural phenomena, whose…

流体动力学 · 物理学 2015-08-20 Salvatore Butera , Mario Di Paola

It is shown that the mysterious quantum prescription of microphysics has analogues at the scale of stars, galaxies and superclusters, the common feature in all these cases being Brownian type fractality. These considerations are shown to…

综合物理 · 物理学 2015-06-26 B. G. Sidharth

This comment is in response to the paper by L. Guzzo recently appeared in ``New Astronomy'' related to our work. The subject of the discussion concerns the correlation properties of galaxy distribution in the available 3-d samples. There is…

天体物理学 · 物理学 2016-08-30 F. Sylos Labini , M. Montuori , L. Pietronero

We study the formation of structure in the Universe assuming that dark matter can be described by a scalar field $\tilde{\Phi}$ with a potential $V(\Phi)=-\mathfrak{m}^{2}\tilde{\Phi}^{2}/2+\lambda\tilde{\Phi}^4/4$. We derive the evolution…

宇宙学与河外天体物理 · 物理学 2021-02-09 Juan Magaña , Tonatiuh Matos , Abril Suárez , F. J. Sánchez-Salcedo

The structure of the multiverse is determined by information flow.

量子物理 · 物理学 2007-05-23 David Deutsch

A finite universe naturally supports chaotic classical motion. An ordered fractal emerges from the chaotic dynamics which we characterize in full for a compact 2-dimensional octagon. In the classical to quantum transition, the underlying…

广义相对论与量子宇宙学 · 物理学 2010-04-06 Janna Levin , John D. Barrow

The power-law dependence of the angle in the angular projection of galaxy distribution is explained by assuming that in the spherical shells within a small angle the distributions are also fractal. If this local angular fractal is…

天体物理学 · 物理学 2008-02-03 Yu Shi

An oscillating universe cycles through a series of expansions and contractions. We propose a model in which ``phantom'' energy with $p < -\rho$ grows rapidly and dominates the late-time expanding phase. The universe's energy density is so…

天体物理学 · 物理学 2014-10-13 Matthew G. Brown , Katherine Freese , William H. Kinney