Excludes part of LSND region. backgrounds. Oscillation. signal expectation. n ... Excess from unmodeled ne from m decay will change by. 4 checks K background ...
Mixing angles in US, could there be two also in USM? If LSND is a manifestation ... Because the evolution of matter over anti-matter cannot be easily explained in ...
New detector technologies. Ultimately and inevitably lead to neutrino factories ... Houdini's escape from the BBN constraints. LSND sterile neutrino implies ...
MiniBooNE Motivation: Interpreting the LSND Signal. What to make of 3 independent Dm2 values? ... Main tracking detector: NOMAD drift chambers. Forward PID detectors ...
Compatibility between SBL (including KARMEN) and LSND of 30%, instead of 3.6 ... Oracular responses were given every month, on the 7th day, the birthday of Apollo ...
The LSND experiment took data from 1993 to 1997 at LAMPF, searching for electron ... Sterile neutrinos are like cherries, if you have one you probably have more than ...
... experiment results (except LSND, barring CPT violation that does not ... (here we are barring the possibility of a `singular' see-saw case where M1 = 0) ...
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 ...
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 ...
... can be largely eliminated with an energy dependent fiducial cut (rtowallb) ... Approximately 70-ton fiducial volume detector, located near MiniBooNE (cost $20M) ...
Grey College, Durham, UK, December 18-19, 2005. Sergio ... D. Dassie et al., Nucl. Phys. A678:341, 2000. D. I. Britton et al., Phys. Rev. D49:28, 1994 ...
Title: Expectations and predictions for neutrino observables Author: romanino Last modified by: Guest Created Date: 5/13/2003 4:57:52 PM Document presentation format
... a 1.7 interaction length beryllium target producing various secondaries (p's, p's, K's) ... MiniBooNE Beam : Beryllium Target. The MB target is ~71 cm long ...
Effects of physics beyond the SM as effective operators ... Something even more wild and wacky? Murayama, IHEP, June 12, 2006. 22. What it would take ...
The Fermilab Neutrino Program Status and Challenges Ahead Eric Prebys* Fermilab Accelerator Division/MiniBooNE *with acknowledgements to everyone who leaves talks ...
Title: Project Overview Author: School of Natural Science Last modified by: Carlos Pe a Created Date: 10/5/2002 5:46:21 PM Document presentation format
Wave-Particle Duality. Flavor states are comprised of mass states. ELECTRON. m1. m2. H. Ray ... the speed of light * in the medium* produce an E-M shock wave ...
Neutrino Physics - Lecture 7. Steve Elliott. LANL Staff Member. UNM Adjunct Professor ... From K- ne decay : Measure kaon-induced neutrino flux at high energies ...
Our understanding of neutrinos has changed in light of new evidence: Neutrinos no longer massless particles ... Urylon Liner and Radon Seal. Unique Experiment ...
Massachusetts Institute of Technology. J.Cao, Y.Liu, B.P.Roe, H.J.Yang. University of Michigan. A.O.Bazarko, E. M. Laird, P.D.Meyers, R.B.Patterson, F.C.Shoemaker, ...
Updates to the Low Energy Excess in MiniBooNE ... Old Solution: uniformly inflate HARP error until c2 is acceptable. Inflates HARP's ~7% error to closer to ~16 ...
Neutrino Phenomenology Boris Kayser Scottish Summer School August 11, 2006 + Are There Sterile Neutrinos? What Is the Pattern of Mixing? The Central Role of 13 Both ...
MiniBooNE asymmetry predicted based on. 3 2 best fit model. for CPV ... MiniBooNE data: important in addressing the viability of sterile neutrino models ...
(Status of ) The search for nm to ne. oscillations at MiniBooNE ... Laser flasks. four Ludox-filled flasks. fed by optical fiber from laser. 397 nm laser ...
T. L. Hart, R.H.Nelson, M.Tzanov, M.Wilking, E.D.Zimmerman. University of Colorado ... [Harvey, Hill, and Hill, hep-ph0708.1281] New light gauge boson [Nelson, ...
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
Also probe with 'long baseline' accelerator and reactor experiments ... First 'long baseline' accelerator experiment. Beam from KEK PS to Kamiokande, 250 km away ...
Most is Dark Matter and Dark Energy. Most Dark Matter is Cold (non relativistic ... Plumacher, Ellis, Lola, Giudice et al, Fujii et al. mi 10-1 eV. Baryogenesis ...
Kaon rates measured in low energy proton production experiments. New HARP experiment (CERN) ... 'Little Muon Counter' measures rate of kaons in situ ...
Dream case for neutrino oscillation physics! Dm2solar within reach of long-baseline expts ... Helps interpretation of CP violation, double beta decay data. 7% 1 ...
present in many GUTs as SO(10), E6,... dim=5 operator can be obtained ... and large lepton mixing angles in GUTs are available. If future date will require very small ...