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相关论文: A Complete Statistical Analysis for the Quadrupole…

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The recent three-year WMAP data have confirmed the anomaly concerning the low quadrupole amplitude compared to the best-fit \Lambda CDM prediction. We show that, allowing the large-scale spatial geometry of our universe to be…

天体物理学 · 物理学 2008-12-18 L. Campanelli , P. Cea , L. Tedesco

Recent Wilkinson Microwave Anisotropy Probe (WMAP) data confirm the Cosmic Microwave Background (CMB) quadrupole anomaly. We further elaborate our previous proposal that the quadrupole power can be naturally suppressed in axis-symmetric…

天体物理学 · 物理学 2008-11-26 L. Campanelli , P. Cea , L. Tedesco

Recent Planck data confirm that the cosmic microwave background displays the quadru-pole power suppression together with large scale anomalies. Progressing from previous results, that focused on the quadrupole anomaly, we strengthen the…

宇宙学与河外天体物理 · 物理学 2015-06-18 Paolo Cea

A Universe containing uniform magnetic fields, strings, or domain walls is shown to have an ellipsoidal expansion. This case has motivations from observational cosmology especially the anomaly concerning the low quadrupole amplitude…

广义相对论与量子宇宙学 · 物理学 2020-06-25 Mohamed Lamine Abdelali , Noureddine Mebarki

We point out that the recent WMAP findings of a suppressed large scale power in the Cosmic Microwave Background anisotropy power spectrum, if of cosmological origin, make the case for a new cosmic coincidence problem.The observed…

高能物理 - 唯象学 · 物理学 2007-05-23 Alessandro Melchiorri , Laura Mersini-Houghton

We compared the Planck 2018 data on the large-scale anisotropies in the cosmic microwave background to the results obtained in the slightly anisotropic ellipsoidal universe. We focused on the quadrupole temperature correlations to better…

宇宙学与河外天体物理 · 物理学 2019-11-12 Paolo Cea

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

We study a scenario of the ellipsoidal universe in the brane world cosmology with a cosmological constant in the bulk . From the five-dimensional Einstein equations we derive the evolution equations for the eccentricity and the scale factor…

高能物理 - 理论 · 物理学 2008-11-26 Xian-Hui Ge , Sang Pyo Kim

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

The detection of a time variation of the angle between two distant sources would reveal an anisotropic expansion of the Universe. We study this effect of "cosmic parallax" within the "ellipsoidal universe" model, namely a particular…

宇宙学与河外天体物理 · 物理学 2011-06-29 L. Campanelli , P. Cea , G. L. Fogli , L. Tedesco

We constrain several models of the early Universe that predict a statistical anisotropy of the cosmic microwave background (CMB) sky. We make use of WMAP9 maps deconvolved with beam asymmetries. As compared to previous releases of WMAP…

宇宙学与河外天体物理 · 物理学 2014-03-03 Sabir Ramazanov , Grigory Rubtsov

We investigate anomalies reported in the Cosmic Microwave Background maps from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite on very large angular scales and discuss possible interpretations. Three independent anomalies involve…

天体物理学 · 物理学 2009-07-09 Angelica de Oliveira-Costa , Max Tegmark , Matias Zaldarriaga , Andrew Hamilton

There is tentative evidence for a mismatch between the rest frames of matter and the cosmic microwave background, the "quasar dipole anomaly". We consider such a dipole in tilted anisotropic models, for a range of scenarios and sources:…

宇宙学与河外天体物理 · 物理学 2025-12-04 Alicia Martín , Constantinos Skordis , Deaglan J. Bartlett , Harry Desmond , Pedro G. Ferreira , Tariq Yasin

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

We repeat and extend the analysis of Eriksen et al 2004 and Hansen et al 2004 testing the isotropy of the Cosmic Microwave Background (CMB) fluctuations. We find that the hemispherical power asymmetry previously reported for the largest…

天体物理学 · 物理学 2014-11-18 F. K. Hansen , A. J. Banday , K. M. Gorski , H. K. Eriksen , P. B. Lilje

Recent measurements of the Cosmic Microwave Background Anisotropy have provided evidence for the presence of oscillations in the angular power spectrum. These oscillations are a wonderful confirmation of the standard cosmological scenario…

天体物理学 · 物理学 2007-05-23 Alessandro Melchiorri

Several early Universe scenarios predict a direction-dependent spectrum of primordial curvature perturbations. This translates into the violation of the statistical isotropy of cosmic microwave background radiation. Previous searches for…

宇宙学与河外天体物理 · 物理学 2017-03-22 S. Ramazanov , G. Rubtsov , M. Thorsrud , F. R. Urban

The low multipoles of the cosmic microwave background (CMB) anisotropy possess some strange properties like the alignment of the quadrupole and the octopole, and the extreme planarity or the extreme sphericity of some multipoles,…

天体物理学 · 物理学 2008-11-26 R. Aurich , S. Lustig , F. Steiner , H. Then

The WMAP and Planck observations show that the quadrupole and octopole orientations of the CMB might align with each other. We reveal that the quadrupole--octopole alignment is a natural implication of the primordial power spectrum in an…

宇宙学与河外天体物理 · 物理学 2015-03-12 Zhe Chang , Xin Li , Sai Wang

A cosmological model with anisotropic dark energy is analyzed. The amount of deviation from isotropy of the equation of state of dark energy, the skewness \delta, generates an anisotropization of the large-scale geometry of the Universe,…

宇宙学与河外天体物理 · 物理学 2011-06-28 L. Campanelli , P. Cea , G. L. Fogli , L. Tedesco
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