Metal Abundance in the Solar Interior | Zendy

M. Fukugita | Zendy; Naoya Hata | Zendy

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Metal Abundance in the Solar Interior

Author(s) -

M. Fukugita,

Naoya Hata

Publication year - 1998

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/305608

Subject(s) - abundance (ecology) , solar neutrino , homogeneous , metal , neutrino oscillation , neutrino , physics , range (aeronautics) , oscillation (cell signaling) , materials science , chemistry , thermodynamics , composite material , nuclear physics , metallurgy , ecology , biology , biochemistry

It is shown that the metal abundance in the solar interior is constrainedfrom the current solar neutrino experiment, even if one allows neutrinoconversion in the sun due to neutrino oscillation. The result shows that themetal abundance in the interior should be within the range 0.4 - 1.4 times thatin the surface, supporting the idea that the sun formed by a contraction of agas cloud with an almost homogeneous composition.

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