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相关论文: Missing Lorenz-boosted Circles-in-the-sky

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Physical constants and cosmological parameters could vary with position. On the largest scales such variations would manifest themselves as gradients across our Hubble volume, leading to dipole-modulation of the cosmic microwave…

宇宙学与河外天体物理 · 物理学 2011-08-12 Adam Moss , Douglas Scott , James P. Zibin , Richard Battye

The Cosmic Microwave Background provides our most ancient image of the Universe and our best tool for studying its early evolution. Theories of high energy physics predict the formation of various types of topological defects in the very…

天体物理学 · 物理学 2011-09-29 M. Cruz , N. Turok , P. Vielva , E. Martinez-Gonzalez , M. Hobson

Fluctuations in the temperature of the cosmic microwave background have now been detected over a wide range of angular scales, and a consistent picture seems to be emerging. This article describes some of the implications for cosmology.…

天体物理学 · 物理学 2009-10-28 Douglas Scott , Joe Silk , Martin White

The significance to which the cosmic microwave background observations by the satellite COBE can be used to refute a specific observationally based hypothesis for the global topology (3-manifold) of the Universe is investigated, by a new…

天体物理学 · 物理学 2009-10-31 Boudewijn F. Roukema

In the standard cosmological model, the temperature anisotropy of the cosmic microwave background is interpreted as variation in the gravitational potential at the point of emission, due to the emitter being embedded in a region ${\cal C}$…

天体物理学 · 物理学 2007-05-23 Richard Lieu

The peculiar motion of an observer relative to an ideal reference frame at rest with respect to the cosmic background produces boosting effects which modify and transfer at higher multipoles the frequency spectrum of the isotropic…

宇宙学与河外天体物理 · 物理学 2025-03-24 Tiziana Trombetti

The theoretical basis for the prediction of anisotropies in the cosmic microwave background is very well developed. Very low amplitude density and temperature perturbations produce small gravitational effects, leading to an anisotropy that…

天体物理学 · 物理学 2007-05-23 E. L. Wright

The universe displays a three-dimensional pattern of hot and cold spots in the radiation remnant from the big bang. The global geometry of the universe can be revealed in the spatial distribution of these spots. In a topologically compact…

天体物理学 · 物理学 2009-10-30 Janna Levin , Evan Scannapieco , Giancarlo de Gasperis , Joseph Silk , John D. Barrow

Instabilities and turbulence extending to the smallest dynamical scales play important roles in the deposition of energy and momentum by gravity waves throughout the atmosphere. However, these dynamics and their effects have been impossible…

We provide an informal discussion of pattern formation in a finite universe. The global size and shape of the universe is revealed in the pattern of hot and cold spots in the cosmic microwave background. Topological pattern formation can be…

天体物理学 · 物理学 2007-05-23 Janna Levin , Imogen Heard

A significant fraction of Milky Way (MW) satellites exhibit phase-space properties consistent with a coherent orbital plane. Using tailored N--body simulations of a spherical MW halo that recently captured a massive (1.8$\times…

Temperature and polarization variations across the microwave sky include the fingerprints of quantum fluctuations in the early universe. They may soon reveal physics at unprecedented energy scales.

宇宙学与河外天体物理 · 物理学 2018-05-18 John E. Carlstrom , Thomas M. Crawford , Lloyd Knox

Clusters of galaxies, the largest collapsed structures in the Universe, are located at the intersection of extended filaments of baryons and dark matter. Cosmological accretion onto clusters through large scale filaments adds material at…

Cosmic microwave background (CMB) anisotropies probe the primordial density field at the edge of the observable Universe. There is a limiting precision (``cosmic variance'') with which anisotropies can determine the amplitude of primordial…

天体物理学 · 物理学 2016-08-25 Marc Kamionkowski , Abraham Loeb

Aims: we propose that the condition of relative motion between us and the objects that we observe in the Universe should generate relativistic aberration on the photons that such objects emit, varying the observed flux similarly to the…

宇宙学与河外天体物理 · 物理学 2024-04-05 Nicolò Cedola

If the Universe has the topology of a 3-torus ($T^3$), then it follows from recent data on large-scale temperature fluctuations $\Delta T/T$ of the cosmic microwave background that either the minimal size of the torus is at least of the…

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

One of the external fields that influences the population of globular clusters is that due to galactic bulges. In extreme situations, perigalactic distances $r_p \le 100$ pc, globular clusters could suffer total disruption in a single…

天体物理学 · 物理学 2009-10-31 Holly K. Nordquist , Robert J. Klinger , Pablo Laguna , Jane C. Charlton

``One could imagine that as a result of enormously extended astronomical experience, the entire universe consists of countless identical copies of our Milky Way, that the infinite space can be partitioned into cubes each containing an…

天体物理学 · 物理学 2007-05-23 Jean-Pierre Luminet , Boudewijn F. Roukema

[Abridged] An observable signature of a detectable nontrivial spatial topology of the Universe is the circles-in-the-sky in the CMB sky. In the most general search, pairs of circles with deviation from antipodality $0^\circ \leq \theta \leq…

宇宙学与河外天体物理 · 物理学 2016-08-10 G. I. Gomero , B. Mota , M. J. Reboucas

We study the effect of a finite topology on the temperature correlations of the cosmic microwave background in a flat universe. Analytic expressions for the angular power spectrum are given for all possible finite flat models. We examine…

天体物理学 · 物理学 2009-10-31 Evan Scannapieco , Janna Levin , Joseph Silk