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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
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author Kurki-Suonio, Hannu
author_facet Kurki-Suonio, Hannu
author_sort Kurki-Suonio, Hannu
collection CERN
description 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.
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institution Organización Europea para la Investigación Nuclear
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publishDate 2010
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spelling cern-13176972022-08-10T20:17:21Zdoi:10.5170/CERN-2012-001.183http://cds.cern.ch/record/1317697engKurki-Suonio, HannuPhysics of the Cosmic Microwave Background and the Planck MissionAstrophysics and AstronomyThis 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.CERNarXiv:1012.5204oai:cds.cern.ch:13176972010-12-24
spellingShingle Astrophysics and Astronomy
Kurki-Suonio, Hannu
Physics of the Cosmic Microwave Background and the Planck Mission
title Physics of the Cosmic Microwave Background and the Planck Mission
title_full Physics of the Cosmic Microwave Background and the Planck Mission
title_fullStr Physics of the Cosmic Microwave Background and the Planck Mission
title_full_unstemmed Physics of the Cosmic Microwave Background and the Planck Mission
title_short Physics of the Cosmic Microwave Background and the Planck Mission
title_sort physics of the cosmic microwave background and the planck mission
topic Astrophysics and Astronomy
url https://dx.doi.org/10.5170/CERN-2012-001.183
http://cds.cern.ch/record/1317697
work_keys_str_mv AT kurkisuoniohannu physicsofthecosmicmicrowavebackgroundandtheplanckmission