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Is the low-l microwave background cosmic?
The examination of the cosmic microwave background (CMB) temperature anisotropies measured with the Wilkinson microwave anisotropy probe (WMAP) was discussed. It was found that the large-angle (low-l) correlations of the CMB exhibited several statistically significant anomalies compared to the stand...
| Autores principales: | , , , |
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| Lenguaje: | eng |
| Publicado: |
2004
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.93.221301 http://cds.cern.ch/record/725179 |