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Supernova Detection

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Tagging efficiency and BG reduction<br />

Selection criteria of delayed signal:<br />

(1) Vertex position within 2m<br />

(2) Energy of delayed signal > 3MeV<br />

(3) Time after the prompt within 60µsec.<br />

(4) Ring pattern cuts<br />

Selection efficiency is ~74%.<br />

With 90% capture eff. by 0.2% Gd,<br />

Tagging efficiency is 67%<br />

While the chance coincidence<br />

prob. is estimated to be ~2×10 -4<br />

It almost satisfy the requirement to<br />

remove remaining spallation background<br />

at 10 MeV.<br />

H.Watanaba<br />

poster #94<br />

Number of events/day/22.5kt/0.5MeV<br />

SRN<br />

predictions<br />

10 4<br />

10 3<br />

10 2<br />

10<br />

SK-I final data sample<br />

1<br />

SSM(BP2004) * 0.4<br />

(efficiencies are considered)<br />

6 8 10 12 14 16 18 20<br />

Energy (MeV)<br />

10 -1<br />

10 -2<br />

10 -3<br />

10 -4<br />

Energy spectrum<br />

92 %<br />

MC simulation<br />

Recon. Energy [MeV]<br />

Current single BG rate<br />

(mainly due to spallation<br />

and solar 8 B)

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