Bulletin of the American Physical Society
5th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Volume 63, Number 12
Tuesday–Saturday, October 23–27, 2018; Waikoloa, Hawaii
Session LN: Neutrino Physics IV |
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Chair: Kate Scholberg, Duke University Room: Hilton Kohala 4 |
Saturday, October 27, 2018 9:00AM - 9:15AM |
LN.00001: Search for Invisible Nucleon Decay in the SNO+ Light Water Phase Morgan Askins Many Grand Unified Theories predict processes that would allow baryons to decay to leptons, violating baryon number conservation. The observation of baryon number violation in nucleon decay would be a revelation as well as being pivotal in understanding the apparent asymmetry between baryons and anti-baryons in the universe. This is manifest in some theories primarily through the decay of nucleons to three chargeless leptons (e.g. n -> 3ν), which can only be observed through the resulting nuclear deexcitation gamma. This "invisible" nucleon decay could be observable in water through the deexcitation of the resulting oxygen-15 nucleus which emits a 6.2 MeV gamma and requires that backgrounds at these energies, in a large detector, to be extremely low. Presented here are the first results from the SNO+ light water phase which consists of nearly 120 days of live data taking. A blind analysis was performed using a Poisson counting method and a maximum likelihood method independently to obtain the results. |
Saturday, October 27, 2018 9:15AM - 9:30AM |
LN.00002: Constraints on Neutrino Lifetime from the Sudbury Neutrino Observatory Benjamin Land As neutrinos are known to have a finite mass it is possible with new physics that neutrinos could decay to lighter states. On the long baseline between the Earth and the Sun, such decay could lead to an energy dependent disappearance of the solar neutrino flux. An analysis of SNO data has been developed to constrain the lifetime of neutrino mass state two by fitting for this energy dependent distortion to the survival probability of 8B solar neutrinos. |
Saturday, October 27, 2018 9:30AM - 9:45AM |
LN.00003: A Neutrino Disappearance Search for Sterile Neutrinos with the CAPTAIN-Mills Detector at the Los Alamos Neutron Science Center Robert Cooper MiniBooNE and LSND have shown compelling evidence for sterile neutrinos at Δm2 ∼1 eV2 in short baseline neutrino oscillations experiments. In these experiments, a pure muon neutrino beam is used to search for electron neutrino appearance, but muon neutrino disappearance searches have shown no anomalies. This talk will describe the CAPTAIN-Mills experiment which will use a 10-ton liquid argon scintillation detector to leverage the enhanced cross section from coherent elastic neutrino-nucleus scattering (CEvNS) to measure muon neutrino disappearance at the Lujan Center at the Los Alamos Neutron Science Center. Lujan is a 100-kW stopped pion source that nominally delivers a 290-ns wide, 800-MeV proton beam onto a tungsten target at 20 Hz, but the beam width can be significantly narrowed to 30 ns. Fast pulsing is critical for isolating the monoenergetic muon neutrino from the other neutrino flavors and neutron backgrounds. In this talk, I will describe the CAPTAIN-Mills detector, the Lujan neutrino source, the expected sensitivities for sterile neutrinos, and show results from the summer neutrino test run. |
Saturday, October 27, 2018 9:45AM - 10:00AM |
LN.00004: Abstract Withdrawn
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Saturday, October 27, 2018 10:00AM - 10:15AM |
LN.00005: Neutrino Quantum Kinetics in the Early Universe Evan Grohs, Vincenzo Cirigliano, George M Fuller, Mark W Paris, Shashank Shalgar Neutrinos decouple from the plasma at a temperature scale of 1 MeV in the early universe. The decoupling is an out-of-equilibrium process and requires the solution of the Quantum Kinetic Equations (QKEs) in a homogeneous and isotropic geometry. We present results from our code BURST on solving the complete set of QKEs relevant for neutrino energy transport. By using generalized density matrices, we follow the non-degenerate spectra of electron, muon, and tau flavor neutrinos. In addition, we are able to show how the coherence between the flavor states manifests itself in the off-diagonal elements of the density matrices. Our results have implications for both the primordial abundances predicted from big bang nucleosynthesis and neutrino observables in the cosmic microwave background. |
Saturday, October 27, 2018 10:15AM - 10:30AM |
LN.00006: Search for Bosonic Dark Matter with the MAJORANA DEMONSTRATOR Jamin Rager The MAJORANA DEMONSTRATOR is a neutrinoless double-beta decay experiment operating at the 4850' level of the Sanford Underground Research Facility that uses modular arrays of High-Purity germanium detectors enriched in 76Ge in an ultra-low background environment. The DEMONSTRATOR has a low energy program that is capable of probing a variety of physics beyond the standard model; it has previously produced limits on bosonic dark matter candidates that come in two weakly coupling varieties, vector and pseudoscalar (axion-like). These particles would manifest as low energy peaks at their rest mass in the detector spectrum. I describe ongoing efforts in the MAJORANA DEMONSTRATOR's bosonic dark matter campaign, specifically to improve the limits on the coupling parameters of these dark matter candidates in the mass range 9 – 100 keV. |
Saturday, October 27, 2018 10:30AM - 10:45AM |
LN.00007: A Facility for Developing and Testing Ge Detectors and Related Components for the MAJORANA and LEGEND Experiments Morgan L Clark The GERDA and MAJORANA Collaborations have demonstrated that high purity germanium (HPGe) detectors enriched in 76Ge are an excellent choice in searching for neutrinoless double beta decay. We have developed a general facility at the University of North Carolina to facilitate detector R&D activities related to both the MAJORANA DEMONSTRATOR and the LEGEND experiment. The facility consists of clean-rooms, a glove box, a LN based N2 purge system, and special equipment for working on and testing cables, connectors and electronics. There is a cryostat, cooled by a pulse tube cooler, that can accommodate multiple strings of HPGe detectors similar to those used in the DEMONSTRATOR. Tools have been developed to allow for testing of HV cables. This facility has been used to fabricate and test improved custom cables and connectors for possible use in the DEMONSTRATOR, and will be used for upcoming LEGEND activities. A description of the facility and details of the R&D activities performed will be presented. |
Saturday, October 27, 2018 10:45AM - 11:00AM |
LN.00008: Spectral analysis for the MAJORANA DEMONSTRATOR Jordan William Myslik The MAJORANA DEMONSTRATOR is an experiment searching for neutrinoless double-beta decay in 76Ge. It consists of two modular arrays of natural and 76Ge-enriched high purity germanium detectors totalling 44.1 kg, operating on the 4850' level of the Sanford Underground Research Facility in Lead, South Dakota, USA. The ultra-low background achieved by the MAJORANA DEMONSTRATOR has an expected variation in measured rates among each constituent detector. I will discuss studies into how the geometrical distribution of background rates may be exploited to improve spectral analysis sensitivity, and statistical approaches used to analyze the measured spectrum. |
Saturday, October 27, 2018 11:00AM - 11:15AM |
LN.00009: Extensions of Higgs Universality in the Sterile Neutrino Sector T. Goldman, G. J. Stephenson Application of Higgs Universality to the neutrino sector provides coupling between the active neutrino sector and the sterile neutrino sector. For either Hierarchy, this leads to predictions for the mass ratios in the sterile sector. While the most natural result is that the ratios of sterile masses should be approximately the squares of the ratios of charged fermions, the ratios of the lighter masses can be modified. We show how these results are obtained. |
Saturday, October 27, 2018 11:15AM - 11:30AM |
LN.00010: Higgs Universality Description of Sterile Neutrino Properties: Consistency with experimental data. G. J. Stephenson, T. Goldman Application of Higgs Universality to the neutrino sector provides predictions for the coupling of sterile neutrinos to the well known active neutrinos. We examine two reported experimental results, the fit by Collin {\it et al.} \cite{Collin} to low energy oscillations and the fit by Cappelluti {\it et al.} \cite{Cappelluti} to a source of an observed $3.51 keV$ astrophysical line. We find that, for a range of parameters consistent with either hierarchy of active neutrinos, the expected coupling is consistent with the observations. \begin{thebibliography}{99} |
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