The thermonuclear instability of the solar core

Details The thermonuclear instability of the solar core The thermonuclear instability of the solar core

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000nuphs..85...52g&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 85, Issue 1-3, p. 52-57.

Physics

Nuclear Physics

Scientific paper

I present here a list of the most important astrophysical problems related to the energy and neutrino producing solar core. Attempting to find a physical connection between the solar activity and the nuclear processes of the solar core, I present the relation between the LOCAL thermal instability and the conditions in the solar core. The result show that if a mechanism would be able to produce a local heating above 108 K, this perturbation would push the local region of the core into the instability regime. Tidal-electromagnetic inductive coupling may elicit such a large local heating. Some consequences of the dynamic solar model are discussed

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