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Astronomy and Astrophysics

Volumn 488, Issue 3, 2008, Pages 861-865

Evolution of low-frequency features in the CMB spectrum due to stimulated Compton scattering and Doppler broadening

(2) Chluba, J a Sunyaev, A a,b

a MAX PLANCK INSTITUT FÜR ASTROPHYSIK (Germany)

b Department of Satellite Monitoring Technologies (Russian Federation)

Author keywords

Cosmology: cosmic microwave background; Cosmology: theory; Line: formation; Radiative transfer; Scattering

Indexed keywords

COSMOLOGY; DOPPLER EFFECT; EQUATIONS OF MOTION; HELIUM; HYDROGEN; INERT GASES; LIGHT; NONMETALS; PHOTONS; RADIO ASTRONOMY; RADIO WAVES; SCATTERING; THERMODYNAMICS;

ANALYTIC SOLUTIONS; ATOMIC TRANSITIONS; COMPTON; COSMIC MICROWAVE BACKGROUND; COSMOLOGY: COSMIC MICROWAVE BACKGROUND; COSMOLOGY: THEORY; DOPPLER; DOPPLER BROADENING; EARLY UNIVERSE; EXTRA-GALACTIC; FREE ELECTRONS; HIGHER FREQUENCIES; LINE BROADENING; LINE SHIFTING; LINE: FORMATION; LOW FREQUENCIES; POWER LAWS; RADIATION FIELDS; RADIATIVE TRANSFER; RADIO SOURCES; SPECTRAL DISTORTIONS; STIMULATED SCATTERING; WEAK LINES;

COMPTON SCATTERING;

EID: 51949108368 PISSN: 00046361 EISSN: 14320746 Source Type: Journal
DOI: 10.1051/0004-6361:200809920 Document Type: Article

Times cited : (21)

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