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Re-ionization and decaying dark matterGunn-Peterson tests suggest that the Universe was reionized after the standard recombination epoch. A systematic treatment is presented of the ionization process by deriving the Boltzmann equations appropriate to this regime. A compact solution for the photon spectrum is found in terms of the ionization ratio. These equations are then solved numerically for the Decaying Dark Matter scenario, wherein neutrinos with mass of order 30 eV radiatively decay producing photons which ionize the intergalactic medium. It was found that the neutrino mass and lifetime are severely constrained by Gunn-Peterson tests, observations of the diffuse photon spectrum in the ultraviolet regime, and the Hubble parameter.
Document ID
19920002726
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Dodelson, Scott
(Fermi National Accelerator Lab. Batavia, IL, United States)
Jubas, Jay M.
(Massachusetts Inst. of Tech. Cambridge., United States)
Date Acquired
September 6, 2013
Publication Date
September 1, 1991
Subject Category
Astrophysics
Report/Patent Number
NAS 1.26:189009
FERMILAB-PUB-91/260-A
NASA-CR-189009
Accession Number
92N11944
Funding Number(s)
CONTRACT_GRANT: NAGW-1340
CONTRACT_GRANT: DE-FG02-84ER-40158
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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