SNS Spallation Neutrino Source 1 SNS layout 2 1.0 GeV proton linear accelerator Accumulator ring Main target Stripping foil.
LENR Transmutations on Earth vs Nucleosynthesis in Stars
ESS-Bilbao Initiative Workshop. Overview of Multi-MW Accelerator Projects
Proton Capabilities at Fermilab Steve Holmes Neutrino Summit 21 July 2014.
High Energy Neutrinos from Astrophysical Sources Dmitry Semikoz UCLA, Los Angeles & INR, Moscow.
Neutrino fluxes and flavor ratios from cosmic accelerators, and the Hillas plot Matter to the deepest 2011 September 13-18, 2011 Ustron, Poland Walter.
Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q= 0.27/26.73 = 1% ppIII loss: 28% Total loss: 2.3%
Neutrinos as probes of ultra-high energy astrophysical phenomena Jenni Adams, University of Canterbury, New Zealand.
Power generation in stars Astronomy 100. Energy transfer As the names of the layers imply, it is not the composition of the sun that is interesting, but.
Sean Grullon For the IceCube Collaboration Searching for High Energy Diffuse Astrophysical Neutrinos with IceCube TeV Particle Astrophysics 2009 Stanford.
2006-01-07Spåtind Norway P.O.Hulth Cosmic Neutrinos and High Energy Neutrino Telescopes Spåtind 2006 lecture 1 Per Olof Hulth Stockholm University [email protected].
Making a neutrino beam The neutrinos detected in the MINOS experiment are produced in the Neutrinos at the Main Injector (NuMI) beam line at Fermi National.
