Cosmological hydrogen recombination: Influence of resonance and electron scattering

Astronomy and Astrophysics

Volumn 503, Issue 2, 2009, Pages 345-355

  Chluba, J ^a,b   Sunyaev, R A ^a,c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF TORONTO   (Canada)

^c Russian Academy of Sciences   (Russian Federation)

Author keywords

Cosmic microwave background; Cosmological parameters; Cosmology: Theory; Radiative transfer; Scattering

Indexed keywords

ABSORPTION PROCESS; COSMIC MICROWAVE BACKGROUNDS; COSMOLOGICAL PARAMETERS; COSMOLOGY: THEORY; DOPPLER; DOPPLER BROADENING; EMISSION PROFILE; FOKKER-PLANCK APPROXIMATION; FREQUENCY-DEPENDENT; HYDROGEN ATOMS; POWER-SPECTRA; QUANTUM-MECHANICAL CORRECTIONS; RECOIL EFFECT; REDISTRIBUTION FUNCTION; THERMODYNAMIC FACTORS; THOMSON; TIME DEPENDENCE; TIME-DEPENDENT; TWO PHOTON; VISIBILITY FUNCTION;

ABSORPTION; ATOMS; COSMIC RAY MEASUREMENT; DOPPLER EFFECT; ELECTRON ENERGY LOSS SPECTROSCOPY; ELECTRON SCATTERING; HYDROGEN; MULTIPHOTON PROCESSES; PHOTONS; RADIATIVE TRANSFER; RESONANCE;

COSMOLOGY;

EID: 77949337071     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912335     Document Type: Article

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