Abstract
A mechanism for generating baryon perturbations in the scalar field condensate baryogenesis scenario is proposed. This mechanism may naturally explain the observed periodic distribution of the luminous matter in the Universe with the characteristic scale of 128 h{sup -1} M pc. It is found that both the observed baryon asymmetry and the periodicity in the large structure of the Universe can be explained through the behaviour of a complex scalar field condensate formed at the inflationary stage. (author). 10 refs.; 2 figs.
Chizhov, M V;
[1]
Kirilova, D P
[2]
- Sofia Univ. (Bulgaria)
- Bylgarska Akademiya na Naukite, Sofia (Bulgaria)
Citation Formats
Chizhov, M V, and Kirilova, D P.
Large Scale Periodicity of the Universe and Baryogenesis.
JINR: N. p.,
1994.
Web.
Chizhov, M V, & Kirilova, D P.
Large Scale Periodicity of the Universe and Baryogenesis.
JINR.
Chizhov, M V, and Kirilova, D P.
1994.
"Large Scale Periodicity of the Universe and Baryogenesis."
JINR.
@misc{etde_10112483,
title = {Large Scale Periodicity of the Universe and Baryogenesis}
author = {Chizhov, M V, and Kirilova, D P}
abstractNote = {A mechanism for generating baryon perturbations in the scalar field condensate baryogenesis scenario is proposed. This mechanism may naturally explain the observed periodic distribution of the luminous matter in the Universe with the characteristic scale of 128 h{sup -1} M pc. It is found that both the observed baryon asymmetry and the periodicity in the large structure of the Universe can be explained through the behaviour of a complex scalar field condensate formed at the inflationary stage. (author). 10 refs.; 2 figs.}
place = {JINR}
year = {1994}
month = {Dec}
}
title = {Large Scale Periodicity of the Universe and Baryogenesis}
author = {Chizhov, M V, and Kirilova, D P}
abstractNote = {A mechanism for generating baryon perturbations in the scalar field condensate baryogenesis scenario is proposed. This mechanism may naturally explain the observed periodic distribution of the luminous matter in the Universe with the characteristic scale of 128 h{sup -1} M pc. It is found that both the observed baryon asymmetry and the periodicity in the large structure of the Universe can be explained through the behaviour of a complex scalar field condensate formed at the inflationary stage. (author). 10 refs.; 2 figs.}
place = {JINR}
year = {1994}
month = {Dec}
}