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 ...
5th International Workshop on Neutrino Factories & Superbeams ... S. Forte, M. L. Mangano, G. Ridolfi. Nucl. Phys. B602 (2001) 585. Quark spin content ...
What do we know now about solar neutrino branches ? ... 0.4 Mt Water Cherenkov (Memphis) 100 kt Liquid Argon (Glacier) 50 kt Liquid Scintillator (LENA) ...
Dustmaids Down a Drafty Hall: Neutrinos at the Sudbury Neutrino ... by John Updike. In. Telephone Poles. And. Other Poems (1960) e- n. Detecting Neutrinos ...
In less than two decades, atmospheric neutrinos have gone from being 'anomalous' ... 1980s 1990s: Skepticism was rampant! 'Neutrino experiments are hard! ...
Constraint on OSC parameters from the detection of supernova neutrino burst ... time neutrino burst model available ... Analysis by using the TBP burst model ...
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, ...
ns in matter can acquire an effective mass through scattering (analogous to ... Improved spectral shape and Zenith angle information * Anti-electron neutrino detection ...
neutrino puzzles Ulrich Heintz Boston University http://physics.bu.edu/quarknet/2002/neutrinos.ppt outline the neutrino atmospheric neutrinos solar neutrinos ...
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 ...
Probe to High Energies. Effects of physics beyond the SM as ... EGRET down to =2 10-8cm-2sec-1. GLAST down to ~10-11cm-2sec-1. Neutrinos/km3: ~4 10-10cm-2sec-1 ...
Antiparticles. 18. Standard model. 3 families of particles. 4 fundamental forces ... if the neutrino is its own antiparticle (like the photon, but different from the ...
Takaaki Kajita (ICRR, U.of Tokyo) Production of atmospheric neutrinos Some early history (Discovery of atmospheric neutrinos, Atmospheric neutrino anomaly)
Title: Neutrinos in Cosmology Author: G. Mangano Last modified by: infn Created Date: 1/16/2002 4:19:53 PM Document presentation format: Presentazione su schermo
The Fermilab Neutrino Program Status and Challenges Ahead Eric Prebys* Fermilab Accelerator Division/MiniBooNE *with acknowledgements to everyone who leaves talks ...
Tn = (4/11)1/3 Tg. Neutrinos are fermions while photons are bosons, so at a ... (Tn / Tg)3 ng0 ... neutrino properties or unconventional neutrino stories. ...
... the future of neutrino physics, sponsored by the American Physical Society Divisions of ... study like this, co-sponsored by several APS Divisions, is ...
Our motivation was to use neutrinos to look into the interior of the sun and ... Oscillation Formalism. Two Flavor Mixing: n1 n2. na cosq sinq. nb -sinq cosq ...
neutrino mass and mixing. Open questions about neutrinos and their ... Generically, grand unified models (GUTS) favor. GUTS relate the Leptons to the Quarks. ...
Title: Neutrino oscillations in dense neutrino media Author: SERGIO PASTOR Last modified by: Sergio Pastor Created Date: 1/16/2002 4:19:53 PM Document presentation format
Title: Neutrino oscillations in dense neutrino media Author: SERGIO PASTOR Last modified by: Sergio Pastor Created Date: 1/16/2002 4:19:53 PM Document presentation format