13–15 May 2013
Union South
US/Central timezone

Session

Accelerator-Based Neutrino Physics III

14 May 2013, 16:00
Union South

Union South

1308 West Dayton Street, Madison, WI 53706

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  1. Rex Tayloe (Indiana U.)
    14/05/2013, 16:00
    Accelerator-Based Neutrino Physics Parallel
    The MiniBooNE experiment, located at Fermilab on the Booster Neutrino Beamline, has searched for $\nu_\mu \rightarrow \nu_e$ and $\overline{\nu}_\mu \rightarrow \overline{\nu}_e$ oscillations in the range $0.1<\Delta m^2<5.0$~ev$^2$ as indicated by results from the LSND experiment. MiniBooNE has recently completed $\overline{\nu}_{\mu}$ running after collecting $11.3 \times 10^{20}$...
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  2. Dr Robert Cooper (Indiana University)
    14/05/2013, 16:25
    Accelerator-Based Neutrino Physics Parallel
    Low energy neutrinos (E $\lesssim$ 50~MeV) have a predicted, but unobserved, neutral-current coherent elastic scattering channel on nuclei. Coherent neutrino scattering are important in supernovae and can probe weak nuclear form factors at low $Q^2$. At these low energies, the coherent scattering cross section dominates, but it deposits very little energy and requires low detection...
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  3. Christina Ignarra (MIT)
    14/05/2013, 16:45
    Accelerator-Based Neutrino Physics Parallel
    MicroBooNE is a Liquid Argon Time Projection Chamber (LArTPC) currently under construction at Fermilab which will begin taking data in early 2014. It will use the unique resolution of a LArTPC to resolve whether the MiniBooNE low energy excess events are electron-like or photon-like as well as explore other aspects of neutrino interactions. MicroBooNE is also an important step towards the...
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  4. Prof. Nickolas Solomey (Wichita State University)
    14/05/2013, 17:10
    Accelerator-Based Neutrino Physics Parallel
    We will review recent new cross-section measurements from the Fermilab MIPP experiment. This demonstrated excellent operating conductions show that the experiment's data can produce improved cross-section measurements. Future extended running plans on Liquid Nitrogen for Cosmic Ray shower development are needed to do improved Cosmic-Ray studies. Plans and needs for a special cosmic-Ray Liquid...
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