(Two) Open Questions in Stellar Nuclear Physics

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Work Supported by USDOE Grant No. DE-FG02-94ER40870. To appear in StuFiesta, Cocoyoc, Mexico, April 19-22, 2004

Scientific paper

10.1063/1.1805924

No doubt, among the most exciting discoveries of the third millennium thus far are {\bf Oscillations of Massive Neutrinos} and {\bf Dark Energy} that leads to an accelerated expansion of the Universe. Accordingly, Nuclear Physics is presented with two extraordinary challenges: the need for precise (5% or better) prediction of solar neutrino fluxes within the Standard Solar Model, and the need for an accurate (5% or better) understanding of stellar evolution and in particular of Type Ia super nova that are used as cosmological standard candle. In contrast, much confusion is found in the field with contradicting data and strong statements of accuracy that can not be supported by current data. We discuss an experimental program to address these challenges and disagreements.

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