Muons traveling up into Super-K from high-energy nm reactions in the rock below ... a model to get a good fit over 5 orders of magnitude in energy and 4 in baseline ...
Build on successes of optical Cherenkov in IMB, Kam, SuperK - SN1987A & muon ... Using commercial hydrophones (Benthos, ITC, ..) 100 MeV beam at ITEP into water tank ...
Subdominant modes 'Solar' regime. Anomalies (LSND) 9/19/09 ... Subdominant mode: nm- ne (q13) SuperK atmospheric n data is not very sensitive here because the ...
Confirm SuperK results with accelerator n's (K2K) Demonstrate oscillatory ... Understanding the demands on the accelerator complex and the need for possible ...
Title: PDP for NSS Phys. Curriculum: The Stars and the Sun II Subject: Basic properties of the sun Author: Chu Ming-chung Last modified by: PHY Created Date
How neutrinos fit into the 'Standard Model' Grand ... Clyde Cowan. Fred Reines. Reines and Cowan's neutrinos produced in reaction: Observed reaction was: ...
neutrino puzzles Ulrich Heintz Boston University http://physics.bu.edu/quarknet/2002/neutrinos.ppt outline the neutrino atmospheric neutrinos solar neutrinos ...
Sampling Detectors for ne Detection and Identification. Adam Para, Fermilab. NuFact02 ... Needle in a Haystack ? NC Background. ne (|Ue3|2 = 0.001) ne background ...
The 'Dark Side' of solar neutrinos. Two 'flavors' are involved in ... HERON. CC. 60 t In load in scint. LENS ~250 keV. ES ~600 t liq scint. KamLAND ~250 keV ...
Proton Decay in GUTs. Hitoshi Murayama (IAS) DESY Theorie Workshop. Sep 24, 2003 ... A close look at the GUT-scale threshold correction allows us to extract MHc from ...
isotropy. J. Maneira NOW2006 Otranto - September 11, 2006. 9. 8B ... event variables R (radial position) 14(isotropy) cos sun and E(energy) ES separation ...
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
Oscillations: Particle Physics with Atmospheric ... Figures from Los Alamos Science 25 (1997) Oscillation Probability. Three Families? ... New Physics Effects ...
Supper Neutrino Source Neutrinos at the SNS (Spallation Neutron Source) Yu.Efremenko ORNL 0. A little bit of Modern Neutrino History Why Low Energy Neutrinos are Good
Galactic Supernova neutrino detection with Lena. Electron Antineutrino spectroscopy ... Geo - neutrinos and LENA. what is the source of the terrestrial heat flow ? ...
LEDs for HV status of each PMT channel on front panel (relay on/off display) ... Note: The LEDs monitor relay status only, NOT HV status! RE-ENABLE the selected ...
... Atsuko Ichikawa, Carol Johnstone, Steve Kahn, Boris Kayser, Chiang Kee Jung, Bruce ... Zohreh Parsa, Bernard Pope, Stefano Rigolin, Lee Roberts, Andrea ...
LENA. Low Energy Neutrino Astrophysics ... Possible locations for LENA. Underground mine ... The Kaon and the K-decay particles are visible in LENA ...
The Search for Proton Decay at Super-Kamiokande ASTR-007 Theodore Liu Proton Decay overview Protons not infinitely stable, as once thought Required for grand ...
Why should neutrinos oscillate? How can we search for neutrino oscillations? What is the Main Injector? How do we search for neutrino oscillations in MINOS?
The AMANDA-II neutrino telescope is buried in deep, clear ice, 1500m ... Universiteit Gent. Universit de Mons-Hainaut. Germany: Universit t Mainz. DESY-Zeuthen ...
powers of (low momenta)/(big mass scales) by this argument, gravity should be irrelevant ... then Kaluza-Klein parity (i.e. KK momentum) is conserved. ...
Model predictions of DSNB ne flux in range 22.9 En 36.9 MeV. 0.19 to 1.49 cm-2s-1 ... Discrimination. Preliminary Blind Analysis of NCD energy spectrum. En ...
Neutrino Astrophysics: PeV to ZeV (with some whacky particle physics) For the viewing pleasure of Alan, the only person to make me regret that I don t play (cough ...
MINOS Experiment: Oscillation Results from the First Two Years of Running Niki Saoulidou, Fermilab, For the MINOS Collaboration Wine and Cheese Seminar, Fermilab ...
In less than two decades, atmospheric neutrinos have gone from being 'anomalous' ... 1980s 1990s: Skepticism was rampant! 'Neutrino experiments are hard! ...
Neutron Detection Fast Neutrons 'Fast' neutrons are those with kinetic energy above ... detectors for use in measuring plutonium content in running reactors in situ ...
Dark matter 'burners' may appear as red giants (Salati ... The degenerate core WIMP burner hypothesis. Stars with degenerate electron cores are everywhere! ...
Reduced sensitivity to systematics. Big size and low energy ... PMT housing: Benthos glass boxes. Optical detector, prototypes OK. Need second round design ...
He was so unsure of this that he didn't even name his own particle. ... If you were in a Jupiter-type orbit a billion kilometers from SN1987A when it ...
Promotes the development of gravitational-wave detection as an ... (ALLEGRO, AURIGA, EXPLORER, NAUTILUS, and NIOBE), and space ... NAUTILUS (INFN- LNF) ...
1. The OPERA emulsion detector for a. long-baseline neutrino ... nm CC st/sm et x BR evert. sin2 2qmt ( large Dm2 ) 2 x 2.3 / (14930 x 0.48 x 0.36 x 0.90) ...
Long Baseline Neutrino Oscillation Experiments. Alfons Weber ... discriminates between nm nt and nm. ns A. Weber. LBL Experiments. 10. ? CC Energy Analysis ...
Accelerator ? physics has gained recognition in the (2006) CERN Council ... offering much higher rate and purer flavour content, allowing a more ambitious ...
Tests of Lorentz Invariance using Atmospheric Neutrinos and AMANDA-II ... but subdominant effects at high energies? For E 100 GeV and m 1 eV, Lorentz 1011 ...