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This paper has been withdrawn by the author(s), due to double submission. You can find it under: physics/0208019

数据分析、统计与概率 · 物理学 2007-05-23 Armin Bunde , Jan F. Eichner , Rathinaswamy Govindan , Shlomo Havlin , Eva Koscielny-Bunde , Diego Rybski , Dmitry Vjushin

Several anomalies appear to be present in the large-angle cosmic microwave background (CMB) anisotropy maps of WMAP. One of these is a lack of large-scale power. Because the data otherwise match standard models extremely well, it is natural…

天体物理学 · 物理学 2008-12-18 Emory F. Bunn , Austin Bourdon

This paper has been withdrawn by the authors. This is due to the fact that it has been substantially revised. As a consequence title and aim of the contents

其他凝聚态物理 · 物理学 2013-05-29 C. Lechner , U. Roessler

This article describes the Cosmic Microwave Background anisotropies expected in a closed universe with the topology of a lens space L(p,q) and with density parameter Omega_0 close to 1. It provides the first simulated maps for such spaces…

天体物理学 · 物理学 2009-11-07 Jean-Philippe Uzan , Alain Riazuelo , Roland Lehoucq , Jeffrey Weeks

A large peculiar velocity of the intergalactic medium produces a Doppler shift of the cosmic microwave background with a frequency-dependent quadrupole term. This quadrupole will act as a source for polarization of the cosmic microwave…

宇宙学与河外天体物理 · 物理学 2014-02-20 Elinore Roebber , Gilbert Holder

This article is a report of 25 years of Cosmic Microwave Background activities at INPE. Starting from balloon flights to measure the dipole anisotropy caused by the Earth's motion inside the CMB radiation field, whose radiometer was a…

宇宙学与河外天体物理 · 物理学 2010-03-01 C. A. Wuensche , T. Villela

We provide a new derivation of the anisotropies of the cosmic microwave background (CMB), and find an exact expression that can be readily expanded perturbatively. Close attention is paid to gauge issues, with the motivation to examine the…

天体物理学 · 物理学 2009-01-08 J. P. Zibin , Douglas Scott

We calculate the large scale polarization of the cosmic microwave background induced by the anisotropy of the spatial geometry of our universe. Assuming an eccentricity at decoupling of about $0.64 10^{-2}$, we find $\Delta T_{pol}/ T_0…

天体物理学 · 物理学 2007-10-24 Paolo Cea

In this paper we develop the theory of clusterization of peaks in a Gaussian random field. We have obtained new mathematical results from this theory and the theory of percolation and have proposed a topological method of analysis of sky…

天体物理学 · 物理学 2009-10-28 D. I. Novikov , H. E. Jorgensen

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

This paper has been withdrawn by authors for significant modification.

高能物理 - 唯象学 · 物理学 2007-05-23 Nikolai Kochelev , Vicente Vento

This paper has been withdrawn by the authors, due an error involving the weak* convergence argument in section 2

动力系统 · 数学 2007-05-23 Marcus Pivato , Reem Yassawi

Weak lensing distortion of the background cosmic microwave background (CMB) temperature and polarization patterns by the foreground density fluctuations is well studied in the literature. We discuss the gravitational lensing modification to…

天体物理学 · 物理学 2009-11-11 Chao Li , Asantha Cooray

Anisotropies in the cosmic microwave background radiation due to gravity waves are investigated. An initial spectrum of gravity waves may have been induced during an epoch of inflation. We study the propagation of such a spectrum in a…

天体物理学 · 物理学 2008-02-03 Ruth Durrer , Tina Kahniashvili

We re-analyze the issue of redshifts induced by a moving cosmic string by looking at moving sources and observers on a conical spacetime in a fully relativistic approach. By replacing the concept of a moving spacetime with the more clearly…

天体物理学 · 物理学 2007-05-23 Francine R. Marleau , Charles C. Dyer , Jody H. Palmer

We discuss effects of cosmological moduli fields on the cosmic microwave background (CMB). If a modulus field \phi once dominates the universe, the CMB we observe today is from the decay of \phi and its anisotropy is affected by the…

高能物理 - 唯象学 · 物理学 2007-05-23 Takeo Moroi , Tomo Takahashi

The temperature anisotropy power spectrum measured with the Wilkinson Microwave Anisotropy Probe (WMAP) at high multipoles is in spectacular agreement with an inflationary Lambda-dominated cold dark matter cosmology. However, the low order…

天体物理学 · 物理学 2009-11-07 G. Efstathiou

We summarise the current status of cosmic microwave background spectrum and anisotropy measurements, and their theoretical interpretation. This is the update of the mini-review for the 1997 web-version of the Review of Particle Properties.

天体物理学 · 物理学 2007-05-23 George Smoot , Douglas Scott

Following a self-contained review of the basics of the theory of cosmological perturbations, we discuss why the conclusions reached in the recent paper by Kaloper et al are too pessimistic estimates of the amplitude of possible imprints of…

高能物理 - 理论 · 物理学 2016-09-06 Robert H. Brandenberger , Jerome Martin

It is argued that large scale angle correlations of the Cosmic Microwave Background Radiation (CMBR) temperature fluctuations measured by Wilkinson Microwave Anisotropy Probe (WMAP) mission may have a trace of discrete symmetries of quantum…

宇宙学与河外天体物理 · 物理学 2014-06-18 M. V. Altaisky , N. E. Kaputkina