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- W189227583 abstract "Because of the dynamicaI reason, a clustering process must occurred in a region of horizon. As we know only the adiabatic perturbation whose extent is not smaller than Jeans limits can be growing. So the time when M_J=M_H is adopted as the initial time of perturbation growing. In a reasonable range of rest mass of relic neutrinos, it is conclude that the clustering time of the relic neutrinos is rather late, possibly later than the formation time of galaxies." @default.
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- W189227583 date "1984-03-01" @default.
- W189227583 modified "2023-09-25" @default.
- W189227583 title "An Analysis on the Clustering Time of the Relic Neutrinos" @default.
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