Atmospheric neutrino oscillation analysis with subleading effects in Super-Kamiokande I, II, and III
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2010-05-20
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We present a search for nonzero θ13 and deviations of sin2θ23 from 0.5 in the oscillations of atmospheric neutrino data from Super-Kamiokande I, II, and III. No distortions of the neutrino flux consistent with nonzero θ13 are found and both neutrino mass hierarchy hypotheses are in agreement with the data. The data are best fit at Δm2=2.1×10-3eV2, sin2θ13=0.0, and sin2θ23=0.5. In the normal (inverted) hierarchy θ13 and Δm2 are constrained at the one-dimensional 90% C.L. to sin2θ13<0.04(0.09) and 1.9(1.7)×10 -3<Δm2<2.6(2.7)×10-3eV2. The atmospheric mixing angle is within 0.407≤sin2θ23≤0.583 at 90% C.L. © 2010 The American Physical Society.
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Wendell, R, C Ishihara, K Abe, Y Hayato, T Iida, M Ikeda, K Iyogi, J Kameda, et al. (2010). Atmospheric neutrino oscillation analysis with subleading effects in Super-Kamiokande I, II, and III. Physical Review D - Particles, Fields, Gravitation and Cosmology, 81(9). p. 92004. 10.1103/PhysRevD.81.092004 Retrieved from https://hdl.handle.net/10161/4274.
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Kate Scholberg
Prof. Scholberg's broad research interests include experimental elementary particle physics, astrophysics and cosmology. Her main specific interests are in neutrino physics. She has long-term involvement in Super-Kamiokande in Japan and the T2K ("Tokai to Kamioka") high-intensity beam experiment that sends neutrinos 300 km from an accelerator at the J-PARC facility in Japan to Super-K. She is a member of DUNE (Deep Underground Neutrino Experiment), the next-generation U.S.-based international experiment designed to observe neutrinos beamed from Fermilab to a large liquid argon detector at an underground facility in South Dakota. One of Prof. Scholberg's particular interests on DUNE is the detector's sensitivity to the huge bursts of neutrinos from core-collapse supernovae.
Prof. Scholberg serves as spokesperson of COHERENT, a multi-detector experiment with the primary physics goal of measuring CEvNS (Coherent Elastic Neutrino Nucleus Scattering) using the high-quality, high-intensity neutrinos produced by the Spallation Neutron Source at Oak Ridge National Laboratory in Tennessee. CEvNS is the interaction of a neutrino with an entire nucleus, resulting in a very tiny nuclear recoil. CEvNS was measured for the first time by the collaboration in 2017. COHERENT is currently engaged in multiple measurements of CEvNS on different nuclear targets, as well as a broad program of neutrino interaction measurements and beyond-the-standard-model physics searches.
Prof. Scholberg was a co-founder of SNEWS, the SuperNova Early Warning System, an inter-experiment collaboration of detectors with Galactic supernova sensitivity. Neutrinos from a core collapse will precede the photon signal by hours; therefore coincident observation of a burst in several neutrino detectors will be a robust early warning of a visible supernova. The goals of SNEWS are to provide the astronomical community with a prompt alert of a Galactic core collapse, as well as to optimize global sensitivity to supernova neutrino physics.
Christopher Walter
I am a professor in the physics department studying particle physics and cosmology. I try to understand both the nature of the ghostly particles called neutrinos in giant detectors deep underground, and why the expansion of the universe is accelerating using telescopes on top of mountains. My background and training is originally in particle physics and I was part of the team that showed the sub-atomic particles called neutrinos have mass. The leader of our team, T. Kajita was co-awarded the 2015 Nobel Prize in Physics for this discovery which cited the work of our collaboration. I also began the effort in observational cosmology at Duke, joining the Vera C. Rubin Observatory, a giant telescope under construction in Chile designed to make a 10 year, three dimensional survey of the entire visible sky. Using the Rubin Observatory, we will focus on examining billions of galaxies, along with supernovae and other astronomical probes to try to determine the nature of the mysterious “Dark Energy” which is unaccountably causing the universe to pushed apart at a faster and faster rate.
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