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The role of neutrinos in core collapse Supernova explosion - LUTh ...

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SNe history<br />

Before telescope <strong>in</strong>troduction (before 1885), naked-eye<br />

observations <strong>of</strong> some Galactic SNe<br />

after telescope <strong>in</strong>troduction (s<strong>in</strong>ce 1885), . . .<br />

. . . search for previous SNe remnants<br />

. . . discovery <strong>of</strong> extra-galactic SNe<br />

s<strong>in</strong>ce 1941, spectral analysis led to SNe classification<br />

type I → without H l<strong>in</strong>es<br />

type II → with H l<strong>in</strong>es<br />

after 60’s, quantitative models for SN <strong>explosion</strong><br />

SN Ia → thermonuclear <strong>explosion</strong> <strong>of</strong> a white dwarf<br />

(WD) or a neutron star (NS) <strong>in</strong> stellar b<strong>in</strong>ary systems<br />

SN II, Ib, Ic, . . . → <strong>core</strong> <strong>collapse</strong> SN <strong>explosion</strong> <strong>of</strong> a<br />

massive star<br />

Neutr<strong>in</strong>os <strong>in</strong> <strong>core</strong> <strong>collapse</strong> SN <strong>explosion</strong> - Paris, 10 September 2009 – p. 4/48

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