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Supernova Neutrinos - Department of Theoretical Physics

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MULTIPLE SPECTRAL SPLITS IN THE COOLING PHASE<br />

[Dasgupta, Dighe, Raffelt & Smirnov, arXiv:0904.3542 [hep-ph]]<br />

x<br />

e<br />

F : F : F 0.85: 0.75:1.00<br />

n e n e n x<br />

=<br />

(typical in cooling phase)<br />

Splits possible in both normal and<br />

inverted hierarchy, for n & n !!<br />

Possible time-dependent signatures<br />

in the SN n signal<br />

Crucial both n and n detection<br />

[See also Fogli, Lisi, Marrone, Tamborra, arXiV:0907.5115]<br />

[Talks by Dasgupta, Marrone]<br />

Alessandro Mirizzi JIGSAW 2010 Mumbai, 22-02-2010

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