Title: Piero Galeotti
1Piero Galeotti Università di Torino and
INFN GianVittorio Pallottino Università di Roma
and INFN Guido PizzellaUniversità di Roma Tor
VergataINFN- Frascati
SN1987A revisited
2Results from LSD and KAMIOKANDE
32h56m
7h35m
LSD
Kamioka
8
0
Hours of 23 February 1987
Mont Blanc 45 pulses/hour gt 5 MeV Kamiokande
85 pulses/hour gt 7.5 MeV
(7.5 MeV corresponds to Nhit20)
4Mont Blanc neutrino telescope 1987
5(No Transcript)
6Kamiokande neutrino telescope 1987
7(No Transcript)
8Hirata et al. PR D 448 (1988)
9May the Supernova Bang more than once ?
10Kamiokande neutrino telescope 1987
New analysis
- The data have been supplied to us by the
Kamiokande collaboration in 1987. We have
acknowledged the collaboration in several papers
11relative Kamiokande time
IMB
no IMB
1211 ? in 12 s Nhgt20
7 ? in 6 s Nh gt 21
13relative Kamiokande time
IMB Egt15 MeV
no IMB Elt15 MeV
14Correlation of the Kamiokande and LSD neutrino
detectors with the Rome and Maryland
gravitational wave detectors
15(No Transcript)
16We have searched for possible correlations
between the signals of the neutrino detectors and
those of the g.w. detectors
17The algorithm
C(f) 1/Nn Si ER(tif ) EM(tif )
Nn number of pulses (in the neutrino detector)
in a given period (say,
one hour) ti time of a pulse f common time
shift for a possible delay
18The background
Cb(f1, f2) 1/Nn S?? ER(f1) EM(f2)
Nn number of pulses (in the neutrino detector)
in a given period (say,
one hour) f1, f2 random time shifts for the
background
19We perform N random extractions of f1, f2 for the
background and count the number n of times when
Cb(f1, f2) gt C(f)
20N one million random data for the background
C(???1.?)72.6 K
Cb(f1, f2) with random f1, f2
21Mont Blanc 145 - 345 ( 5-neutrinos at 256
U.T.)
n
C(-1.1)
F 1.2 (second)
22What about Kamiokande ?
- (absolute time uncertainty 1 min)
23?c is the time correction in s
best ?c7.8 s
24Kamiokande has a time error 1 minute
Kamiokande time correction 7.8 s
Schramm and Truran (1990)
IMB
K
25(No Transcript)
26New analysis of the original data
27Periods of one hour moved in steps of 6 min
n (N105)
hours of 23 February
n (N104)
with time correction of 7.8 s
28CONCLUSIONSThis new analysis reinforces the
idea of a long duration activity of SN1987A in
the neutrino emission.
29noi non doviamo desiderare che la natura si
accomodi a quello che parrebbe meglio disposto et
ordinato a noi, ma conviene che noiaccomodiamo
lintelleto nostro a quello che ella ha fatto,
sicuri tale essere lottimo et non
altro.Galileo in 1612 to Federico Cesi.