Constraint on particle physics from helioseismology

Details Constraint on particle physics from helioseismology Constraint on particle physics from helioseismology

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517...29s&link_type=abstract

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,

Mathematics

Logic

Helioseismology, Neutrino, Axion, Nuclear Cross Section

Scientific paper

Helioseismology used to be used to see what is the cause of the solar neutrino problem. Recent progress in experiments of neutrino detection showed, however, that neutrino oscillation accounts for this long-lived issue. This fact does not mean at all that helioseismology is not useful for elementary particle physics. Rather, combination of helioseismology and recent experiments of neutrino detection enables to give stringent constraint on some aspects of fundamental particle physics. We discuss what we should do and what we can do in this situation for elementary particle physics from the helioseismological side. We will demonstrate some examples; - limits on the neutrino parameters, the axion parameter, and the pp-nuclear cross section.

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