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Physics of the Cosmic Microwave Background and the Planck Mission

This lecture is a sketch of the physics of the cosmic microwave background. The observed anisotropy can be divided into four main contributions: variations in the temperature and gravitational potential of the primordial plasma, Doppler effect from its motion, and a net red/blueshift the photons acc...

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Detalles Bibliográficos
Autor principal: Kurki-Suonio, Hannu
Lenguaje:eng
Publicado: CERN 2010
Materias:
Acceso en línea:https://dx.doi.org/10.5170/CERN-2012-001.183
http://cds.cern.ch/record/1317697
Descripción
Sumario:This lecture is a sketch of the physics of the cosmic microwave background. The observed anisotropy can be divided into four main contributions: variations in the temperature and gravitational potential of the primordial plasma, Doppler effect from its motion, and a net red/blueshift the photons accumulate from traveling through evolving gravitational potentials on their way from the primordial plasma to here. These variations are due to primordial perturbations, probably caused by quantum fluctuations in the very early universe. The ongoing Planck satellite mission to observe the cosmic microwave background is also described.