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相关论文: Circles in the Sky: Finding Topology with the Micr…

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If the universe is finite and smaller than the distance to the surface of last scatter, then the signature of the topology of the universe is writ on the microwave background sky. Previous efforts to search for this topology have focused on…

广义相对论与量子宇宙学 · 物理学 2016-02-09 Neil J. Cornish , David N. Spergel , Glenn D. Starkman

If the universe is multiply-connected and sufficiently small, then the last scattering surface wraps around the universe and intersects itself. Each circle of intersection appears as two distinct circles on the microwave sky. The present…

天体物理学 · 物理学 2009-10-30 Jeffrey R. Weeks

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 a Universe with a detectable nontrivial spatial topology the last scattering surface contains pairs of matching circles with the same distribution of temperature fluctuations --- the so-called circles-in-the-sky. Searches undertaken for…

宇宙学与河外天体物理 · 物理学 2011-10-20 B. Mota , M. J. Reboucas , R. Tavakol

The shortest distance around the Universe through us is unlikely to be much larger than the horizon diameter if microwave background anomalies are due to cosmic topology. We show that observational constraints from the lack of matched…

[Abridged] In a Universe with a detectable nontrivial spatial topology the last scattering surface contains pairs of matching circles with the same distribution of temperature fluctuations - the so-called circles-in-the-sky. Searches for…

宇宙学与河外天体物理 · 物理学 2010-05-25 B. Mota , M. J. Reboucas , R. Tavakol

A topologically finite universe, smaller than the observable horizon, will have circles-in-the-sky: pairs of circles around which the temperature fluctuations in the cosmic microwave background are correlated. The circles occur along the…

天体物理学 · 物理学 2007-05-23 Janna Levin

Whether we live in a spatially finite universe, and what its shape and size may be, are among the fundamental long-standing questions in cosmology. These questions of topological nature have become particularly topical, given the wealth of…

天体物理学 · 物理学 2009-11-11 M. J. Reboucas

The Einstein field equations of general relativity constrain the local curvature at every point in spacetime, but say nothing about the global topology of the Universe. Cosmic microwave background anisotropies have proven to be the most…

Clues as to the geometry of the universe are encoded in the cosmic background radiation. Hot and cold spots in the primordial radiation may be randomly distributed in an infinite universe while in a universe with compact topology…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Janna Levin , Evan Scannapieco , Joseph Silk

While the topology of the Universe is at present not specified by any known fundamental theory, it may in principle be determined through observations. In particular, a non-trivial topology will generate pairs of matching circles of…

天体物理学 · 物理学 2010-04-21 B. Mota , M. J. Reboucas , R. Tavakol

The standard method for observationally confirming the existence of a predicted finite topology of the universe involves searching for the repetition of the same finite or extended source in different directions. However, serious problems…

天体物理学 · 物理学 2007-05-23 Reuven Opher

The first year data from the Wilkinson Microwave Anisotropy Probe are used to place stringent constraints on the topology of the Universe. We search for pairs of circles on the sky with similar temperature patterns along each circle. We…

天体物理学 · 物理学 2009-11-10 Neil J. Cornish , David N. Spergel , Glenn D. Starkman , Eiichiro Komatsu

The surface of last scattering of the photons in the cosmic microwave background is not a spherical shell. Apart from its finite width, each photon experiences a different gravitational potential along its journey to us, leading to…

宇宙学与河外天体物理 · 物理学 2019-08-07 Peikai Li , Scott Dodelson , Wayne Hu

We present an update to the search for a non-trivial topology of the universe by searching for matching circle pairs in the cosmic microwave background using the WMAP 7 year data release. We extend the exisiting bounds to encompass a wider…

宇宙学与河外天体物理 · 物理学 2013-05-30 Pascal M. Vaudrevange , Glenn D. Starkman , Neil J. Cornish , David N. Spergel

Multiply connected space sections of the universe on a scale smaller than the horizon size can leave an imprint on cosmic microwave background polarization maps, in such a way that the so-called ``circles-in-the-sky'' method can be used to…

天体物理学 · 物理学 2007-05-23 Alain Riazuelo , Samuel Caillerie , Marc Lachièze-Rey , Roland Lehoucq , Jean-Pierre Luminet

We examine the possibility that circles in the cosmic microwave background could be formed by the interaction of a gravitational wave pulse emitted in some pre-big-bang phase of the universe with the last scattering surface. We derive the…

广义相对论与量子宇宙学 · 物理学 2011-09-08 William Nelson , Edward Wilson-Ewing

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

It is shown here how prior estimates on the local shape of the universe can be used to reduce, to a small region, the full parameter space for the search of circles in the sky. This is the first step towards the development of efficient…

天体物理学 · 物理学 2007-05-23 G. I. Gomero

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
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