3-11 July 2007
Merida, Mexico
Mexico/General timezone
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HE 2.2

Place

Location: Merida, Mexico
Room: Kabah (Holiday Inn)
Date: 7 Jul 12:05 - 13:30

Timetable | Contribution List

Displaying 7 contributions out of 7
Type: Oral Session: HE 2.2
Track: HE.2.2
The IceCube Neutrino Detector is a cubic kilometer ice-Cherenkov detector being constructed in the deep ice under the geographic South Pole. IceCube is sensitive to high-energy muon neutrinos and muon anti-neutrinos by detecting the secondary muon produced when the neutrino interacts in or near the instrumented volume. The principal source of muon neutrinos are atmospheric neutrinos which come ... More
Presented by Dr. John PRETZ on 7/7/2007 at 17:29
Type: Oral Session: HE 2.2
Track: HE.2.2
The Super-Kamiokande started observation in April of 1996 and continued the data taking for five years of initial running period (SK-I) till the maintenance in July of 2001. The Super-Kamiokande continued the data taking with the half PMT density in the second period (SK-II) from resuming in December of 2002 to shutdown for the reconstruction to return the PMT density in October 2005. Us ... More
Presented by Ms. Yumiko TAKENAGA on 7/7/2007 at 17:41
Type: Oral Session: HE 2.2
Track: HE.2.2
Muon neutrino disappearance probability as a function of neutrino flight lenght L over neutrino energy E was studied. A dip in the L/E distribution was bserved in the data from Super-Kamiokande-I+II, as perdicted from the sinusoidal flavor transition probability of neutrino oscillation. The observed L/E distribution onstrained nu_mu <-> nu_tau neutrino oscillation parameters. We also prese ... More
Presented by Dr. Itaru HIGUCHI on 7/7/2007 at 17:17
Type: Oral Session: HE 2.2
Track: HE.2.2
Super-Kamiokande-I studied low energy neutrino interactions above 4.5 MeV. Photo-cathode coverage has been restored to 40% in Super-Kamiokande-III in order to observe Cherenkov events with an energy even below 4.5 MeV. This is motivated by the transition of solar neutrino oscillations between vacuum and matter-dominated oscillations near 3 MeV and delayed neutron detection from inverse-beta in ... More
Presented by Dr. Michael SMY on 7/7/2007 at 18:05
Type: Oral Session: HE 2.2
Track: HE.2.2
We found 140 neutrino-induced muons in 854.24 live days in the MINOS far detector, which has an acceptance for neutrino-induced muons of 6.9e6 cm**2 sr. We looked for evidence of neutrino disappearance in this data set by computing the ratio of the number of low momentum muons to the sum of the number of high momentum and unknown momentum muons for both data and Monte Carlo expectation in the ... More
Presented by Prof. Stuart MUFSON on 7/7/2007 at 18:17
Type: Oral Session: HE 2.2
Track: HE.2.2
The Main Injector Neutrino Oscillation Search (MINOS) long baseline experiment has been actively taking beam data since 2005, having already accumulated 2.6E20 protons-on-target. MINOS uses the most powerful neutrino beam currently in operation measured in two locations: at Fermilab, close to beam production, and 735 km downstream, in Northern Minnesota. By observing the oscillatory structur ... More
Presented by Dr. Alexandre SOUSA on 7/7/2007 at 17:05
Type: Oral Session: HE 2.2
Track: HE.2.2
Fully reconstruction works of Super-Kamiokande, a large water cherenkov detector , has done in 2006 and data taking has been started from July 06' as SK-III with 11126 20inch PMTs. Calibration works were successfully done and now we are going to step into analiysis stage. In this talk, I will show the calibration data and some early data for atmospheric neutrino and solar neutrino from SK-III ... More
Presented by Dr. Makoto MIURA on 7/7/2007 at 17:53
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