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The three-point correlation function of the cosmic microwave background in inflationary models
We analyze the temperature three-point correlation function and the skewness of the Cosmic Microwave Background (CMB), providing general relations in terms of multipole coefficients. We then focus on applications to large angular scale anisotropies, such as those measured by the {\em COBE} DMR, calc...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
1993
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1086/174421 http://cds.cern.ch/record/256503 |