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Oscar Saavedra

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View from<br />

aside<br />

ν e<br />

ν ν~<br />

,<br />

The Two-Stage Gravitational Collapse Model<br />

[Imshennik V.S., Space Sci Rev, 74, 325-334 (1995)]<br />

ω r<br />

5 h later<br />

A rotating collapsar<br />

M <<br />

2<br />

υ > υ<br />

2<br />

υ r<br />

M<br />

1<br />

1<br />

υ r<br />

M<br />

2<br />

1<br />

1<br />

M<br />

2<br />

, J υr<br />

1<br />

, J<br />

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View from<br />

above<br />

The difference of neutrino emission in the standard<br />

model and in the model of rotating collapsar.<br />

Imshennik V.S., Ryazhskaya O.G., 2004

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