Cargando…
A map of the cosmic microwave background radiation from the Wilkinson Microwave Anisotropy Probe (WMAP), showing the large-scale fluctuations (the quadrupole and octopole) isolated by an analysis done partly by theorists at CERN.
A recent analysis, in part by theorists working at CERN, suggests a new view of the cosmic microwave background radiation. It seems the solar system, rather than the universe, causes the radiation's large-scale fluctuations, similar to the bass in a song.
Publicado: |
2004
|
---|---|
Materias: | |
Acceso en línea: | http://cds.cern.ch/record/804365 |
Ejemplares similares
-
Non-Gaussianity and the Cosmic Microwave Background Anisotropies
por: Bartolo, N., et al.
Publicado: (2010) -
Cosmic Microwave Background Anisotropies up to Second Order
por: Bartolo, Nicola, et al.
Publicado: (2007) -
Large-angle cosmic microwave background anisotropies in an open universe
por: Kamionkowski, M P, et al.
Publicado: (1993) -
MAXIMA: an experiment to measure temperature anisotropy in the cosmic microwave background
por: Lee, A.T., et al.
Publicado: (1999) -
Cosmic Microwave Background anisotropies and extra dimensions in String Cosmology
por: Melchiorri, A., et al.
Publicado: (1999)