The imprint of cosmological hydrogen recombination lines on the power spectrum of the CMB

Astronomy and Astrophysics

Volumn 438, Issue 2, 2005, Pages 461-473

  Rubino Martin J A ^a,b   Hernandez Monteagudo C ^a,d   Sunyaev, R A ^a,c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c Russian Academy of Sciences ^*  (Russian Federation)

^d UNIVERSITY OF PENNSYLVANIA   (United States)

Author keywords

Atomic processes; Cosmic microwave background; Cosmology: theory; Early universe

Indexed keywords

COSMIC RAYS; DAMPING; HELIUM; HYDROGEN; NATURAL FREQUENCIES; PHOTONS; RAYLEIGH SCATTERING;

ATOMIC PROCESSES; COSMIC MICROWAVE BACKGROUND (CMB); COSMOLOGY: THEORY; EARLY UNIVERSE;

ASTROPHYSICS;

EID: 23244453404     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20052939     Document Type: Article

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