ELLIPTIC CMB SKY
The ellipticity of the anisotropy spots of the Cosmic Microwave Background measured by the Wilkinson Microwave Anisotropy Probe (WMAP) has been studied. We find an average ellipticity of about 2, confirming with a far larger statistics similar results found first for the COBE-DMR CMB maps, and then...
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| Veröffentlicht in: | Modern physics letters A 2005-04, Vol.20 (11), p.813-820 |
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| container_title | Modern physics letters A |
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| creator | GURZADYAN, V. G. DE BERNARDIS, P. DE TROIA, G. BIANCO, C. L. KASHIN, A. L. KULOGHLIAN, H. MASI, S. PIACENTINI, F. POLENTA, G. YEGORIAN, G. |
| description | The ellipticity of the anisotropy spots of the Cosmic Microwave Background measured by the Wilkinson Microwave Anisotropy Probe (WMAP) has been studied. We find an average ellipticity of about 2, confirming with a far larger statistics similar results found first for the COBE-DMR CMB maps, and then for the BOOMERanG CMB maps. There are no preferred directions for the obliquity of the anisotropy spots. The average ellipticity is independent of temperature threshold and is present on scales both smaller and larger than the horizon at the last scattering. The measured ellipticity characteristics are consistent with being the effect of geodesics mixing occurring in a hyperbolic Universe, and can mark the emergence of CMB ellipticity as a new observable constant describing the Universe. There is no way of simulating this effect. Therefore we cannot exclude that the observed behavior of the measured ellipticity can result from a trivial topology in the popular flat Λ-CDM model, or from a nontrivial topology. |
| doi_str_mv | 10.1142/S0217732305017111 |
| format | Article |
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G. ; DE BERNARDIS, P. ; DE TROIA, G. ; BIANCO, C. L. ; KASHIN, A. L. ; KULOGHLIAN, H. ; MASI, S. ; PIACENTINI, F. ; POLENTA, G. ; YEGORIAN, G.</creator><creatorcontrib>GURZADYAN, V. G. ; DE BERNARDIS, P. ; DE TROIA, G. ; BIANCO, C. L. ; KASHIN, A. L. ; KULOGHLIAN, H. ; MASI, S. ; PIACENTINI, F. ; POLENTA, G. ; YEGORIAN, G.</creatorcontrib><description>The ellipticity of the anisotropy spots of the Cosmic Microwave Background measured by the Wilkinson Microwave Anisotropy Probe (WMAP) has been studied. We find an average ellipticity of about 2, confirming with a far larger statistics similar results found first for the COBE-DMR CMB maps, and then for the BOOMERanG CMB maps. There are no preferred directions for the obliquity of the anisotropy spots. The average ellipticity is independent of temperature threshold and is present on scales both smaller and larger than the horizon at the last scattering. The measured ellipticity characteristics are consistent with being the effect of geodesics mixing occurring in a hyperbolic Universe, and can mark the emergence of CMB ellipticity as a new observable constant describing the Universe. There is no way of simulating this effect. 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The average ellipticity is independent of temperature threshold and is present on scales both smaller and larger than the horizon at the last scattering. The measured ellipticity characteristics are consistent with being the effect of geodesics mixing occurring in a hyperbolic Universe, and can mark the emergence of CMB ellipticity as a new observable constant describing the Universe. There is no way of simulating this effect. 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The average ellipticity is independent of temperature threshold and is present on scales both smaller and larger than the horizon at the last scattering. The measured ellipticity characteristics are consistent with being the effect of geodesics mixing occurring in a hyperbolic Universe, and can mark the emergence of CMB ellipticity as a new observable constant describing the Universe. There is no way of simulating this effect. Therefore we cannot exclude that the observed behavior of the measured ellipticity can result from a trivial topology in the popular flat Λ-CDM model, or from a nontrivial topology.</abstract><pub>World Scientific Publishing Company</pub><doi>10.1142/S0217732305017111</doi><tpages>8</tpages></addata></record> |
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| title | ELLIPTIC CMB SKY |
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