Lines in the cosmic microwave background spectrum from the epoch of cosmological hydrogen recombination

Monthly Notices of the Royal Astronomical Society

Volumn 371, Issue 4, 2006, Pages 1939-1952

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

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

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

Author keywords

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

Indexed keywords

ANGULAR MOMENTUM; HYDROGEN; QUANTUM THEORY;

ATOMIC PROCESS; BACKGROUND SPECTRUM; COSMIC MICROWAVES BACKGROUND; COSMOLOGY: THEORY; EARLY UNIVERSE; HYDROGEN LEVEL; QUANTUM NUMBERS; RED SHIFT; REDSHIFT RANGE; SPECTRAL DISTORTIONS;

COSMOLOGY;

EID: 33748701866     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10839.x     Document Type: Article

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