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Title: Evolution of adiabatic irregularities during the recombination era, and the missing mass in the universe

Journal Article · · Sov. Astron. (Engl. Transl.); (United States)
OSTI ID:6059771

Primordial carriers of missing mass in the universe, such as finite-mass neutrinos, heavy (m/sub L/> or approx. =1 GeV) neutral leptons, or black holes, may have contributed to the evolution of pregalactic adiabatic irregularities during the cosmological era of hydrogen recombination. Equations previously derived by the authors are applied to a three-component (baryons, radiation, heavy but weakly interacting particles) model medium; dissipative effects are analyzed numerically, and the plasma velocity field is calculated at the epoch of decoupling. In a model with three massive-neutrino species (..nu../sub e/, ..nu../sub ..mu../, ..nu../sub tau/) of equal mass (roughly-equal30 eV) and thermodynamic number density, the perturbations in the plasma density when the redshift zroughly-equal10/sup 3/ would amount to 0.1% at most. If instead the gravitating-particle background consists of stable heavy leptons or primordial black holes, the maximum density contrast will be an order of magnitude lower. The gravitation of any density fluctuations in the ordinary collisional matter during the recombination and post-recombination eras will serve to modulate the amplitude of the small-scale part of the spectrum of inhomogeneities occurring in a background of massive neutrinos.

Research Organization:
Institute of Physics, Rostov University
OSTI ID:
6059771
Journal Information:
Sov. Astron. (Engl. Transl.); (United States), Vol. 29:4
Country of Publication:
United States
Language:
English