Neutrinos from supernova and gamma-ray burst. Long baseline K2K neutrino experiment ... Gamma Ray Bursts (GRB) Search for neutrinos correlated with 1371 GRBs ...
Alec Habig, Univ. of Minnesota Duluth. For the Super-Kamiokande Collaboration. July 29, 2003. Alec Habig, Chiba UHE v Telescope Workshop. S. K. Upward-going m ...
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
Nuclear reactions Using the strong nuclear force to produce useful energy Micro-world Macro-world Lecture 17 Strong Nuclear Force It is very strong It overcomes the ...
... dei neutrini Nel 1940 Pontecorvo aveva applicato gli studi svolti nel gruppo di Roma inventando il neutron log uno strumeno ancora oggi usato per le ...
1960's muon neutrino observed, V-A physics & neutrino oscillations suggested ... The sun does not shine without Antimatter. 6. Solar Neutrino Experiments ...
Title: Slide 1 Last modified by: pcpaoloni2 Document presentation format: Custom Other titles: Times New Roman Nimbus Roman No9 L HG Mincho Light J;MS Gothic;HG ...
The Fermilab Neutrino Program Status and Challenges Ahead Eric Prebys* Fermilab Accelerator Division/MiniBooNE *with acknowledgements to everyone who leaves talks ...
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?
... scraper collimators and beam dump Slow resonance extraction for K-ARENA (Nuclear and Physics ... Length 0.7 m Number 72 Quadrupole Magnet (11 families ...
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
Gravitational Wave Detectors Course in Inflation, Structure formation and CMB 7 November 2002 Silvio Orsi GW: My presentation GW production Upper bounds on GW ...
Extend to make MC calculation more efficient, but do not want to extend in ... Shortcut in 1D, since ?P = ?D, generate primaries flat in cos?P, weight by cos?P ...
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 ...
Title: iThemba 25-11-05 Author: Rob de Meijer Last modified by: Software Group Created Date: 10/20/2004 12:52:25 PM Document presentation format: On-screen Show
1960's muon neutrino observed, V-A physics & neutrino ... Gallium. John Bahcall. The sun does not shine without Antimatter. 6. Solar Neutrino Experiments ...
Galactic Supernova neutrino detection with Lena. Electron Antineutrino spectroscopy ... Geo - neutrinos and LENA. what is the source of the terrestrial heat flow ? ...
Trieste 23-25 Sept. 2002 Nuclear reactions and solar neutrinos The basis of Nuclear Astrophysics The spies of nuclear reactions in the Sun The luminosity constraint ...
Solar Neutrino Problem. Rosa Mar a Dur n Delgado. Contents. Origin of solar neutrinos ... Inferred flux 2 or 3 lower than the prediction. Solar neutrino problem ...
is called the neutrino free-streaming. scale and roughly corresponds to the ... On scales much larger than the free streaming scale, on the other hand, ...
LENA. Low Energy Neutrino Astrophysics ... Possible locations for LENA. Underground mine ... The Kaon and the K-decay particles are visible in LENA ...
Il paradosso del test diretto: perch rimasto per cos tanto tempo al di fuori delle nostre capacit di sperimentatori? Studiare le oscillazioni nm nt con ...
Power and element generation in stars Astronomy 115 Higher temps, more massive nuclei Nuclei are fused at higher and higher temperatures in the core of a massive star ...
... Atsuko Ichikawa, Carol Johnstone, Steve Kahn, Boris Kayser, Chiang Kee Jung, Bruce ... Zohreh Parsa, Bernard Pope, Stefano Rigolin, Lee Roberts, Andrea ...
Detector Issues for Solar and Reactor Neutrinos. SLAC ... Poltergeist. CHOOZ. 6 m. 10% per year. KamLAND. 20 m. Long Baseline Reactor Neutrino Experiments ...
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 ...
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 ...
use large volumes of cheap materials. Detection techniques: radiochemical experiments ... colors time of every hit PMT corrected for photon flight time ...
A MUON (m) IS LIKE AN ELECTRON, ONLY. 200 TIMES HEAVIER. THE ELECTRON (e) IS THE LIGHTEST ... CHEAPER HIGH ENERGY COLLIDERS, BECAUSE MUONS RADIATE LESS THAN ELECTRONS. ...
The Solar Neutrino Problem Barbara Sylwester Zak ad Fizyki S o ca CBK PAN One page story - the short story Fusion reactions in the core of the Sun produce a huge ...
with acknowledgements to everyone who leaves talks where I can find them ... In 1956, Bruno Pontecorvo first shows that it might be possible for neutrinos to ...