A Seismic Solar Model Deduced from the Sound-Speed Distribution and an Estimate of the Neutrino Fluxes | Zendy

Hiromoto Shibahashi | Zendy; M. Takata | Zendy

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A Seismic Solar Model Deduced from the Sound-Speed Distribution and an Estimate of the Neutrino Fluxes

Author(s) -

Hiromoto Shibahashi,

M. Takata

Publication year - 1996

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/48.2.377

Subject(s) - physics , standard solar model , neutrino , flux (metallurgy) , astrophysics , boundary value problem , standard model (mathematical formulation) , speed of sound , solar core , solar neutrino , luminosity , neutrino oscillation , particle physics , thermodynamics , quantum mechanics , galaxy , materials science , archaeology , gauge (firearms) , metallurgy , history

We have deduced the density, pressure, temperature, and hydrogen profiles in the solar interior by solving the basic equations governing the stellar structure with the imposition that the sound-speed profile is that determined by the helioseismic data of Libbrecht et al. (1990; AAA 52.080.103) and Jiménez et al. (1988; AAA 45.080.041). This approach is completely different from that of the standar...

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