Neutrinos I

Presentations

• Solar neutrino flux results measured with the Neutral Current Detector array in the Sudbury Neutrino Observatory (SNO)

  ORAL

  April 13, 2008, 2:30 PM – April 13, 2008, 2:42 PM

  Authors

  • Keith Rielage

    • Los Alamos National Laboratory

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• A Monte Carlo Simulation of the SNO Neutral Current Detector Array

  ORAL

  April 13, 2008, 2:42 PM – April 13, 2008, 2:54 PM

  Authors

  • Jocelyn Monroe

    • Massachusetts Institute of Technology

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• Low Background Phase of KamLAND

  ORAL

  April 13, 2008, 2:54 PM – April 13, 2008, 3:06 PM

  Authors

  • Gregory Keefer

    • The University of Alabama

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• Probing the Mystery of Neutrino Mass with CUORE

  ORAL

  April 13, 2008, 3:06 PM – April 13, 2008, 3:18 PM

  Authors

  • Larissa Ejzak

    • University of Wisconsin-Madison

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• Systematic Effects on Pulse Shape Analysis in HPGe Detectors for 0$\nu\beta\beta$ Searches

  ORAL

  April 13, 2008, 3:18 PM – April 13, 2008, 3:30 PM

  Authors

  • Victor Gehman

    • Los Alamos National Laboratory

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• P-type Modified Electrode Germanium Detector Impurity Profiles

  ORAL

  April 13, 2008, 3:30 PM – April 13, 2008, 3:42 PM

  Authors

  • Jeremy Kephart

    • Pacific Northwest National Laboratory

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• The COBRA Neutrinoless Double Beta Experiment.

  ORAL

  April 13, 2008, 3:42 PM – April 13, 2008, 3:54 PM

  Authors

  • Qiang Li

    • Washington University in St. Louis

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• $^{112}$Sn Double-Electron Capture to Excited States - A Possible Alternative to Neutrinoless Double-Beta Decay

  ORAL

  April 13, 2008, 3:54 PM – April 13, 2008, 4:06 PM

  Authors

  • Mary Kidd

    • Duke University and TUNL

  • James Esterline

    • Duke University and TUNL
    • Duke University

  • Werner Tornow

    • Duke University and TUNL
    • Duke U and TUNL
    • Duke University \& TUNL

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• CLEAR: Prospects for a Low Threshold Neutrino Experiment at the Spallation Neutron Source

  ORAL

  April 13, 2008, 4:06 PM – April 13, 2008, 4:18 PM

  Authors

  • Kate Scholberg

    • Duke University

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