The magnitude of He-3 diffusion in the sun

Details The magnitude of He-3 diffusion in the sun The magnitude of He-3 diffusion in the sun

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...341.1108l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 341, June 15, 1989, p. 1108-1113.

Astronomy and Astrophysics

Astrophysics

10

Atmospheric Diffusion, Helium Isotopes, Plasma Diffusion, Solar Interior, Plasma Pressure, Radial Distribution, Solar Neutrinos, Solar Protons, Stellar Cores, Stellar Models

Scientific paper

The diffusion of He-3(2+) has been determined in the four-component solar plasma. It is found that the fractional diffusive changes in the solar lifetime are bounded by (-2, +5) percent of the standard solar model values for the He-3 abundance. These changes are shown to be negligible in the solar core due to the large rate of the destruction of diffused ions by the (He-3)-(He-3) and (He-3)-(He-4) reactions occurring there.

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