Cosmic microwave background anisotropy in the decaying neutrino cosmology
It is attractive to suppose for several astrophysical reasons that the universe has close to the critical density in light (~30 eV) neutrinos which decay radiatively with a lifetime of ~10^{23} sec. In such a cosmology the universe is reionized early and the last scattering surface of the cosmic mic...
Päätekijät: | Adams, J, Sarkar, S, Sciama, D |
---|---|
Aineistotyyppi: | Journal article |
Julkaistu: |
Oxford University Press
1998
|
Samankaltaisia teoksia
-
Determination of cosmological parameters by the data on anisotropy of cosmic microwave background
Tekijä: S. Ye. Apunevych
Julkaistu: (2000-12-01) -
Cosmological implications of the MAXIMA-I high resolution Cosmic
Microwave Background anisotropy measurement
Tekijä: Stompor, R, et al.
Julkaistu: (2001) -
Cosmological implications of the MAXIMA-1 high-resolution cosmic microwave background anisotropy measurement
Tekijä: Stompor, R, et al.
Julkaistu: (2001) -
Beta Decay and the Cosmic Neutrino Background
Tekijä: Faessler Amand, et al.
Julkaistu: (2014-04-01) -
Frequentist estimation of cosmological parameters from the MAXIMA-1 cosmic microwave background anisotropy data
Tekijä: Abroe, M, et al.
Julkaistu: (2002)