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%
The Diffuse Supernova Neutrino Background Louie Strigari The Ohio State University Collaborators: John Beacom, Manoj Kaplinghat, Gary Steigman, Terry Walker,
Neutrino Interactions with Nucleons and Nuclei Tina Leitner, Ulrich Mosel LAUNCH09 TexPoint fonts used in EMF. Read the TexPoint manual before you delete.
Neutrinos from Stellar Collapse Chris Fryer (LANL/UNM) “Normal” Core Collapse: Collapse and Bounce, Fallback and Cooling More massive Stars Low Mass Stars.
Status of the KM3NeT Project What happened so far The KM3NeT Conceptual Design Report The Preparatory Phase: Towards Implementation 3rd Workshop.
NuMI DOE Review May 25, 2004 Commissioning Page 1 NuMI Commissioning Overview CD-4 Goals Planning Pre-commissioning activities Commissioning Summary.
Studies of the Energy Resolution of the ANITA Experiment Amy Connolly University of California, Los Angeles CALOR06 June 6 th, 2006.
Inside the Tevatron Main Ring
KM3NeT Neutrino Telescope- Prospects for Dark Matter Detection Paschal Coyle, Centre de Physique des Particules de Marseille IDM08, Stockholm, 2 August.
Physics Topics in MINER A David Boehnlein - Fermilab for the MINERvA Collaboration Overview of MINERvA The high intensity of the NuMI beamline at Fermilab.
KM3NeT - a next generation neutrino telescope in the Mediterranean Sea
Mary Hall Reno High Energy Neutrino Cross Sections Neutrino 2004, 18 June 2004.
