Used VMS AUTOSUB to schedule dump database and dump transactions. ... Interrupted and failed copies need to be resubmitted. Where We are Going. Features Needed cont. ...
We have just started not to be in a time blind with ... Systematic shifts on (sin22q23,Dm232) are evaluated with following ... MINOS 90% 4. This was a very ...
Takaaki Kajita (ICRR, U.of Tokyo) Production of atmospheric neutrinos Some early history (Discovery of atmospheric neutrinos, Atmospheric neutrino anomaly)
Exploit alignment of prolonged CNGS beam with deep sea trench in Gulf of ... shield daylight. good transparency. 3x3 m2 cell size. 8000 light detection elements ...
The concept of a spherical TPC. Measurement of the angle q13 ,Neutrino magnetic moment, Neutrino ... 104 events/year to tackle a total number of events of 105 ...
Accelerator Neutrino Oscillation Physics Lecture I Deborah Harris SUSSP St. Andrews, Scotland August 15, 2006 What have Accelerator-based Experiments told us so far?
Kinematics of p Decay. Lab energy given by length of vector from origin to contour ... Kinematics Quantitatively. September 16, 2002. Stan Wojcicki, Physics at ...
Atsuko K. Ichikawa (Kyoto univeristy) For the T2K ... of disappearance nm. nx Discovery of CP violation (Phase2) 3. T2K Collaboration. 12 Countries ...
Medium energy beam. Off-axis detector: 14 mrad. Beam spectra. Signal. Sin2 2q13 = 0.04 ... European groups already in NOnA: Athens, College de France, Tech. ...
... Atsuko Ichikawa, Carol Johnstone, Steve Kahn, Boris Kayser, Chiang Kee Jung, Bruce ... Zohreh Parsa, Bernard Pope, Stefano Rigolin, Lee Roberts, Andrea ...
One near site mid site. Sensitivity ~ 0.03 in a one year run. 40 ... Geological Physical Survey, done. High Resolution electric resistance. seismic reflection ...
The European Long Baseline Program Les Houches, 21 June 2001 Dario Autiero CERN/EP nm nt ? Many thanks to A. Rubbia for providing material about ICARUS
Discovery of neutrino oscillations finite neutrino masses (n2 and n3) (1998 present) ... (a) Solar global: D2O day and night spectra, salt CC, NC, ES fluxes, ...
GUTS: relating properties of quarks and leptons. Is there a grand unified scheme? 17 March, 2003 ... GUTs: one can also imagine unifying quarks and lepton ...
Neutrino Flux is almost the same between and beams. q. Target. Horns ... Only the difference of rs,re between neutrino and anti neutrino appear in the asymmetry ...
LSND : L=30 m, 20 E 60 MeV. 3.5 to 7 s appearance signal ... Babu,Pakvasa, hep-ph/0204236. Bilenki, Giunti, GG, Valle, ... Baremboim et al, hep-ph/0212116 ...
Our understanding of neutrinos has changed in light of new evidence: Neutrinos no longer massless particles ... Urylon Liner and Radon Seal. Unique Experiment ...
NNN00, Fermilab: mini-workshop. NNN02, CERN. NNN05, Aussois ... See, an interesting talk by Vagins on GADZOOKS. LBNO: each detector has its own project ...
Fluxes from muon and radioactive b ions decay. Neutrino Factory. S. Geer. ADR, Gavela, Hern ndez ... physics potential (proton decay, supernova observatory) of ...
The sensitivity depends on statistics, backgrounds and systematics ... If the background level is satisfactory. Search for low mass dark matter candidates ...
How to solve the octant degeneracy? H. Minakata, T2KK06 ... Octant of q23. not resolved. Mass hierarchy not determined ... Octant ambiguity of q23 can be ...
MA-PMT (ADC,TDC) Summer, 2003- 20,480 channels. m. p. Electronics schematics. 64ch MA-PMT ... Inexpensive multi-channel electronics will be developed for the ...
In the Quark Sector, CP is violated. Then, also in the Lepton Sector? Leptogenesys ... CP Measurement is a final goal of flavor physics. Dec. 13, 2001 ...
No symmetry property or theoretical reason for mn = 0. Neutrinos are partners of the massive ... plus PHOBOS and Brahms. STAR. 22. What Makes the Matter? ...
1. Recoilless Resonant Emission and Capture of Electron Antineutrinos: M ssbauer ... Deuterium and Tritium. theoretical. experimental. activation energies. 40 ...
The decay ring will be equipped with 40 and 80 MHz systems (to give required ... High beam purity. High beam quality. More energies. More users. A next ...
Establish 3 flavor framework (or find something new) Discovery ... Give hint on Matter/Anti-matter asymmetry in the universe. What's super muon-neutrino beam? ...
(Safety gallery approved April 2006: opportunity) Distance: 130km ... CCLRC's Rutherford Appleton Laboratory will be the 'host laboratory' for the. Study. ...
Are there more than 3 neutrinos (sterile, heavier than Z)? Do neutrinos obey CP, CPT? ... Search for subdominant ne appearance. Compare n, n oscillations ...
Can we see CP-violation in leptons at FNAL? ... oscillations in the near future ... We have a large Dm2 range impossible to have only 3 involved if all of the ...
Challenging Technology: Detectors Beyond the LHC Craig Buttar Higgs-Maxwell Meeting Feb 06 Examples ATLAS SCT Future of Particle Physics in a nutshell ...
n gligeable en LBL pour L/E max. atm. Dans le vide. nm ne search: at CNGS ... Dans le vide. On peak Off peak. P. Migliozzi and F. Terranova hep-ph/0302274. On/off ...
CERN, WANF: narrow band beam (160-300 GeV), sevaral versions of WBB ... neutrinos is 1.5-2 GeV for all pion energies very intense, narrow band beam ...
Interaction Meeting on Linear Collider and Neutrino Physics. Delhi, India. Nov 12, 2003 ... A large detector of mass 500 kT natural extension of Super Kamiokande. ...
Confirm SuperK results with accelerator n's (K2K) Demonstrate oscillatory ... Understanding the demands on the accelerator complex and the need for possible ...
Test exotic models (decay, extra dimensions,....) Sign of ... Designed and optimized after the knowledge of Super-Kamiokande/K2K results. Primary goal: ne app. ...