Nonlinear Density Enhancement of 3He in the Sun’s Central Core
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Abstract
A flow velocity field that has a “sink” drives the core 3He nuclear reaction diffusion system to instability to jump from the original state to the new one, in which the total amout of 3He is enhanced. This alters the original competition between pp I and pp II +pp III chains, and thus potentially suppresses the production of both the 7Be and 8B neutrino fluxes.
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Cite this article:
DU Jiu-Lin. Nonlinear Density Enhancement of 3He in the Sun’s Central Core[J]. Chin. Phys. Lett., 2000, 17(3): 233-234.
DU Jiu-Lin. Nonlinear Density Enhancement of 3He in the Sun’s Central Core[J]. Chin. Phys. Lett., 2000, 17(3): 233-234.
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DU Jiu-Lin. Nonlinear Density Enhancement of 3He in the Sun’s Central Core[J]. Chin. Phys. Lett., 2000, 17(3): 233-234.
DU Jiu-Lin. Nonlinear Density Enhancement of 3He in the Sun’s Central Core[J]. Chin. Phys. Lett., 2000, 17(3): 233-234.
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