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Creators/Authors contains: "Adamson, P."

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  1. ; ; ; ; ( , 53rd Lunar and Planetary Science Conference (2022))
    USRA (Ed.)
    In this research, we present a study on the manner in which induced longitudinal (axial) and lateral (radial) shear flows differ experimentally when stimulated in a three-dimensional (3D) complex (dusty) plasma produced in the PlasmaKristal-4 (PK4- BU) at Baylor University.
    Free, publicly-accessible full text available May 18, 2023
  2. ; ; ; ; ; ; ; ; ; ; et al ( , Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment)
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  3. ; ; ; ; ; ; ; ; ; ; et al ( , Physical Review D)
    Free, publicly-accessible full text available August 1, 2023
  4. ; ; ; ; ; ; ; ; ; ; et al ( , Physical Review Letters)
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  5. ; ; ; ; ; ; ; ; ; ; et al ( , Physical Review Letters)
    Free, publicly-accessible full text available November 1, 2022
  6. ; ; ; ; ; ; ; ; ; ; et al ( , Physical Review D)
    Free, publicly-accessible full text available September 1, 2022
  7. ; ; ; ; ; ; ; ; ; ; et al ( , Physical Review D)
    null (Ed.)
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  8. ; ; ; ; ; ; ; ; ; ; et al ( , Physical Review D)
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  9. ; ; ; ; ; ; ; ; ; ; et al ( , The European Physical Journal C)
    Abstract The two-detector design of the NOvA neutrino oscillation experiment, in which two functionally identical detectors are exposed to an intense neutrino beam, aids in canceling leading order effects of cross-section uncertainties. However, limited knowledge of neutrino interaction cross sections still gives rise to some of the largest systematic uncertainties in current oscillation measurements. We show contemporary models of neutrino interactions to be discrepant with data from NOvA, consistent with discrepancies seen in other experiments. Adjustments to neutrino interaction models in GENIE are presented, creating an effective model that improves agreement with our data. We also describe systematic uncertainties onmore »these models, including uncertainties on multi-nucleon interactions from a newly developed procedure using NOvA near detector data.« less
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  10. ; ; ; ; ; ; ; ; ; ; et al ( , Journal of Cosmology and Astroparticle Physics)
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