SOLAR MODELS: AN HISTORICAL OVERVIEW
2003 ◽
Vol 18
(22)
◽
pp. 3761-3776
◽
Keyword(s):
I will summarize in four slides the 40 years of development of the standard solar model that is used to predict solar neutrino fluxes and then describe the current uncertainties in the predictions. I will dispel the misconception that the p-p neutrino flux is determined by the solar luminosity and present a related formula that gives, in terms of the p-p and 7 Be neutrino fluxes, the ratio of the rates of the two primary ways of terminating the p-p fusion chain. I will also attempt to explain why it took so long, about three and a half decades, to reach a consensus view that new physics is being learned from solar neutrino experiments. Finally, I close with a personal confession and some personal remarks.
1991 ◽
Vol 06
(01)
◽
pp. 15-20
◽
2001 ◽
Vol 16
(supp01b)
◽
pp. 721-723
1990 ◽
Vol 121
◽
pp. 171-177
◽
Philosophical Transactions of the Royal Society of London Series A Physical and Engineering Sciences
◽
1994 ◽
Vol 346
(1678)
◽
pp. 15-21
2006 ◽
Vol 69
(11)
◽
pp. 1805-1811
◽
Keyword(s):
Keyword(s):
1990 ◽
Vol 121
◽
pp. 179-186
◽
Keyword(s):