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talk - International Workshop on Double Beta Decay and Neutrino

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Implicati<strong>on</strong> <strong>on</strong> solar physics<br />

• Metallicity c<strong>on</strong>troversy<br />

Fit to the available all solar<br />

neutrino data leaving free f Be<br />

<strong>and</strong> f B<br />

( f = Φ/Φ(SSM) )<br />

Hard to discriminate<br />

• Other solar neutrino sources<br />

Each solar neutrino flux can be calculated<br />

with solar luminosity c<strong>on</strong>straint.<br />

+0.02<br />

M.C.G<strong>on</strong>zalez-Garcia, M.Mart<strong>on</strong>i, J.Salvado<br />

JHEP 05(2010)072 / 0910.4584<br />

Φ pp = (6.06 - 0.06 )x10 10 cm -2 s -1 (f pp = 1.013)<br />

Φ CNO < 1.3x10 9 cm -2 s -1 (f CNO < 2.5) at 95%C.L.<br />

Andrea Pocar - DBD11 - November 15, 2011<br />

19

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