Nuclear, High-Energy, Accelerator and Gravitational Physics

Presentations

• Matrix continued fractions for relativistic equations

  ORAL

  Oct. 30, 2015, 5:00 PM – Oct. 30, 2015, 5:12 PM

  Authors

  • Zoltan Papp

    Cal State Univ- Long Beach

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• Appeal of seesaw mechanism for neutrino mass in supersymmetric grand unified theories

  ORAL

  Oct. 30, 2015, 5:12 PM – Oct. 30, 2015, 5:24 PM

  Authors

  • Nima Assad

    Univ of California - San Diego

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• Detecting Solar Relic Axions with ADMX

  ORAL

  Oct. 30, 2015, 5:24 PM – Oct. 30, 2015, 5:36 PM

  Authors

  • Hector Carranza Jr

    Presenter

  • Gray Rybka

    Author

  • Leslie Rosenberg

    author

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• Lambda Re-Scattering On the Proton

  ORAL

  Oct. 30, 2015, 5:36 PM – Oct. 30, 2015, 5:48 PM

  Authors

  • Juan Cardenas

    Presenter

  • John Price

    California State University, Dominguez-Hills, Mentor

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• Delayed Choice in Feynman's Neutron Scattering off a Crystal Experiment: The Effect of Information on the Neutron Distribution -2

  ORAL

  Oct. 30, 2015, 5:48 PM – Oct. 30, 2015, 6:00 PM

  Authors

  • Douglas Snyder

    None

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• Testing the behavior of gravity at the 20-micron distance scale.

  ORAL

  Oct. 30, 2015, 6:00 PM – Oct. 30, 2015, 6:12 PM

  Authors

  • Ian Guerrero

    Humboldt State University

  • Chi-Yu Hu

    University of California - Berkeley, National Institute for Materials Science, Caifornia State University, Long Beach, University of Michigan, Stockholm University, California State University, Long Beach, Utrecht University, Carl von Ossietzky University of Oldenburg, Germany, Hartnell Community College, Department of Physics, Stockholm University, GRAPPA, University of Amsterdam, Paul Scherrer Institute, Switzerland, California State University, Fresno, California State University Long Beach, Cal State Univ- Long Beach, University of Nevada, Reno, University of Rogensberg, Germany, Tribhuvan University, Nepal, University of Victoria and Perimeter Institute for Theoretical Physics, Institute of Physics, Jagiellonian University, Helmholtz Institute Mainz, Johannes Gutenberg University, Physics Department of the University of Nevada, Reno, Universita del Sannio, Cal Tech, California State University, Los Angeles, Univ of California - San Diego, UC Berkeley, Lawrence Livermore National Laboratory, Department of Physics & Astronomy, University of California, Irvine 92617, Department of Chemistry and of Physics & Astronomy, University of California, Irvine 92617, SLAC National Laboratory, Humboldt State University, Physics Department, University of Nevada, Reno, Univ of California - Merced

  • Chi-Yu Hu

    University of California - Berkeley, National Institute for Materials Science, Caifornia State University, Long Beach, University of Michigan, Stockholm University, California State University, Long Beach, Utrecht University, Carl von Ossietzky University of Oldenburg, Germany, Hartnell Community College, Department of Physics, Stockholm University, GRAPPA, University of Amsterdam, Paul Scherrer Institute, Switzerland, California State University, Fresno, California State University Long Beach, Cal State Univ- Long Beach, University of Nevada, Reno, University of Rogensberg, Germany, Tribhuvan University, Nepal, University of Victoria and Perimeter Institute for Theoretical Physics, Institute of Physics, Jagiellonian University, Helmholtz Institute Mainz, Johannes Gutenberg University, Physics Department of the University of Nevada, Reno, Universita del Sannio, Cal Tech, California State University, Los Angeles, Univ of California - San Diego, UC Berkeley, Lawrence Livermore National Laboratory, Department of Physics & Astronomy, University of California, Irvine 92617, Department of Chemistry and of Physics & Astronomy, University of California, Irvine 92617, SLAC National Laboratory, Humboldt State University, Physics Department, University of Nevada, Reno, Univ of California - Merced

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• Size Mass Relation of Galaxies at Redshift z = 4

  ORAL

  Oct. 30, 2015, 6:12 PM – Oct. 30, 2015, 6:24 PM

  Authors

  • Demitri Call

    Sonoma State Univ

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• Milimeter Wave Vacuum Electronic Devices Using Azimuthally Travelling Waves

  ORAL

  Oct. 30, 2015, 6:24 PM – Oct. 30, 2015, 6:36 PM

  Authors

  • Alysson Vrielink

    Caifornia State University, Long Beach, University of California, Merced, Stanford University

  • Chi-Yu Hu

    University of California - Berkeley, National Institute for Materials Science, Caifornia State University, Long Beach, University of Michigan, Stockholm University, California State University, Long Beach, Utrecht University, Carl von Ossietzky University of Oldenburg, Germany, Hartnell Community College, Department of Physics, Stockholm University, GRAPPA, University of Amsterdam, Paul Scherrer Institute, Switzerland, California State University, Fresno, California State University Long Beach, Cal State Univ- Long Beach, University of Nevada, Reno, University of Rogensberg, Germany, Tribhuvan University, Nepal, University of Victoria and Perimeter Institute for Theoretical Physics, Institute of Physics, Jagiellonian University, Helmholtz Institute Mainz, Johannes Gutenberg University, Physics Department of the University of Nevada, Reno, Universita del Sannio, Cal Tech, California State University, Los Angeles, Univ of California - San Diego, UC Berkeley, Lawrence Livermore National Laboratory, Department of Physics & Astronomy, University of California, Irvine 92617, Department of Chemistry and of Physics & Astronomy, University of California, Irvine 92617, SLAC National Laboratory, Humboldt State University, Physics Department, University of Nevada, Reno, Univ of California - Merced

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• A Neutron Gas Laser, can there be particle Lasers?

  ORAL

  Oct. 30, 2015, 6:36 PM – Oct. 30, 2015, 6:48 PM

  Authors

  • Richard Kriske

    University of Minnesota

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