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 DN: Neutrino Physics I |
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Chair: Hamish Robertson, University of Washington Room: Hilton Kohala 4 |
Thursday, October 25, 2018 9:00AM - 9:15AM |
DN.00001: New MiniBooNE Oscillation Result Richard Van de Water, Robert L Cooper Over the last two years the MiniBooNE experiment at FNAL has double its neutrino data sample. An updated electron neutrino oscillation analysis will be presented with 12.84x1020 protons on target (POT) and in combination with the previous electron antineutrino data set of 11.27x1020 POT. A significant combined excess is observed for the electron-like charged current quasi-elastic events. The best fit for a simple two-neutrino oscillation model has a probability of 0.20, compared with a probability of 5x107 for the null hypothesis. The excess observed by the MiniBooNE experiment is consistent with the excess magnitude and L/E shape as reported by the Liquid Scintillator Neutrino Detector (LSND) experiment, indicating strong evidence for physics beyond the Standard Model. |
Thursday, October 25, 2018 9:15AM - 9:30AM |
DN.00002: Investigating the MiniBooNE Low Energy Excess With MicroBooNE Jarrett Moon The MicroBooNE experiment is an 85 ton Liquid Argon Time Projection Chamber (LArTPC) located on the Booster Neutrino Beam at Fermi National Accelerator Laboratory. The primary goal of the experiment is to investigate the low energy excess of electron neutrino like events observed by the MiniBooNE experiment. I will present a brief overview of MicroBooNE and the advantages of using a LArTPC detector to study the MiniBooNE anomaly and identify its origin. I will also describe the state our search for the low energy excess, where we employ multiple analysis approaches in parallel that utilize new reconstruction techniques, including Deep Learning. |
Thursday, October 25, 2018 9:30AM - 9:45AM |
DN.00003: Neutrino-induced Reactions on $^{16}$O: Supernova Neutrino Detection and Nucleosynthesis of Light Elements Toshio Suzuki, Satoshi Chiba, Ken'ichiro Nakazato, Makoto Sakuda, Takashi Yoshida Neutrino-induced reactions on $^{16}$O are investigated by shell-model calculations with new shell-model Hamiltonians, which can describe well the structure of $p$-shell and $p$-$sd$ shell nuclei. Spin-dipole strength distributions in $^{16}$O are studied with the new Hamiltonians. Muon-capture rates on $^{16}$O are evaluated to discuss the quenching of the axial-vector coupling in nuclear medium. Charged-current and neutral-current reaction cross sections are obtained in various particle and $\gamma$ emission channels as well as the total ones at neutrino energies up to $E_{\nu$ = 100 MeV. Partial cross sections for single- and multi-particle emission channels are evaluated by using the branching ratios obtained by the Hauser-Feshbach model. Event spectra of the charged-current reactions as function of recoil energy of electron/positron are discussed for future supernova (SN) neutrino detection at the Super-Kamiokande. Effects of multi-particle emission channels on nucleosynthesis in core-collapse SN explosions are investigated. Inclusion of $\alpha$p emission channels is found to lead to an enhancement of the production yields of $^{11}$B and $^{11}$C. |
Thursday, October 25, 2018 9:45AM - 10:00AM |
DN.00004: Testing the Pauli Exclusion Principle in LNGS underground laboratory Johann Marton The VIP2 experiment is a good example for the spin-off of nuclear physics for underground experiments searching for “new” physics. VIP2 at the Gran Sasso underground laboratory (LNGS, Italy) is searching for possible violations of standard quantum mechanics predictions in atoms at very high sensitivity. We investigate atomic transitions with precision X-ray spectroscopy in order to test the Pauli Exclusion Principle (PEP) and therefore related the spin-statistics theorem. We will present our experimental method for the search for "anomalous" (i.e. Pauli-forbidden) X-ray transitions in copper atoms. We will describe the VIP2 experimental setup, which is taking data at LNGS presently. The goal of VIP2 is to test the PEP for electrons with unprecedented accuracy, down to a limit in the probability that PEP is violated at the level of 10E-31. We will present current experimental results and discuss implications of a possible violation. |
Thursday, October 25, 2018 10:00AM - 10:15AM |
DN.00005: Status of the KATRIN Experiment Bjoern Lehnert The Karlsruhe Tritium Neutrino (KATRIN) experiment investigates the effective electron anti-neutrino mass with tritium beta decays at a sensitivity of 0.2 eV (90% CL). This measurement approach to probe the neutrino mass scale is model independent, unlike cosmological fits or neutrinoless double beta decay experiments. The KATRIN experiment performs spectroscopy of $\beta$-electrons near the tritium endpoint at 18.6 keV by employing a high intensity windowless gaseous tritium source and a high-precision electrostatic spectrometer based on the MAC-E filter principle. The required sensitivity demands novel hardware operating with unprecedented stability, and a precise understanding of all systematic effects and their correlations. The experiment has been under extensive commissioning and first tritium was injected in May 2018. In this talk, the principle and experimental challenges of the neutrino mass measurement with KATRIN, as well as the current status of the experiment, will be presented. |
Thursday, October 25, 2018 10:15AM - 10:30AM |
DN.00006: Multi-Isotope Theory Validation of Calorimetric Electron Capture Spectroscopy Katrina Koehler, Mark P. Croce, Michael A. Famiano, Christopher J. Fontes, Michael W. Rabin High statistics, high resolution calorimetric spectroscopy of electron capture in 163Ho using microcalorimeters has the potential to probe the neutrino kinematic mass with sub-eV mass sensitivity, but the theoretical description of the spectrum must be well-understood to determine the neutrino kinematic mass without bias or significant systematic uncertainty. We have recast the theoretical description in terms of four key categories: choice of atomic code, description of atomic-nucleus overlap, truncation of the overlap of two fully-antisymmetrized atomic wave functions, and complexity of atomic excitations considered. This decision-space is mapped out with predictions made for comparison to experimental observables. Spectra have been acquired with transition edge sensor microcalorimeters with 7–35 eV FWHM depending on source-absorber matrix properties. Multi-isotope cross validation experiments with 163Ho, 193Pt, and 55Fe and comparison to theoretical calculations are used to determine the level of fidelity needed in the calculations. |
Thursday, October 25, 2018 10:30AM - 10:45AM |
DN.00007: Project 8: A frequency-based approach to measure the absolute neutrino mass scale Martin Fertl Neutrino flavor oscillation experiments prove that neutrinos do have non- zero masses. Extensions to the Standard Model of Particle Physics have been developed to explain the non-zero masses and can be directly tested by a measurement of the absolute neutrino mass scale. A highest precision measurement of the β−-decay spectrum of tritium around its endpoint region (Q = 18.6 keV) can reveal the antielectron neutrino mass mν. The current state of the art experiment stretches all technological limits to probe mν down to 200 meV/c2. The Project 8 collaboration envisions a completely new path to measure mν. The recently demonstrated technique of Cyclotron Radiation Emission Spectroscopy (CRES) allows for a frequency-based measurement of the decay electron energy. I will present this new approach and the collaboration’s staged approach to devise an experiment that combines CRES with an atomic tritium source to achieve a neutrino mass sensitivity of 40meV/c2, below the minimum mν ̄e allowed for the inverted neutrino mass ordering scheme. |
Thursday, October 25, 2018 10:45AM - 11:00AM |
DN.00008: Project 8 Phase II: Measuring the Tritium Beta-Decay Spectrum using Cyclotron Radiation Emission Spectroscopy Walter C Pettus Project 8 is a tritium endpoint neutrino mass experiment utilizing a phased program to achieve sensitivity to the range of neutrino masses allowed by the inverted mass hierarchy. The Cyclotron Radiation Emission Spectroscopy (CRES) technique is employed to measure the differential energy spectrum of relativistic decay electrons with high precision. A proof of principle experiment (Phase I) has measured the monoenergetic conversion electrons of a gaseous 83mKr source using a small waveguide detector. Phase II will extend this work to a first demonstration of the CRES technique on a continuous spectrum, measuring the tritium beta-decay spectrum near the endpoint. Significant hardware modifications to the existing system have enhanced the radiofrequency properties and made the system compatible with the tritium source gas. Here we present the hardware upgrades and the data analysis challenges faced during the second phase of the Project 8 experiment. |
Thursday, October 25, 2018 11:00AM - 11:15AM |
DN.00009: Project 8 Phase III Design Progress Penny Slocum Project 8 is a tritium endpoint experiment to measure the mass of the neutrino using |
Thursday, October 25, 2018 11:15AM - 11:30AM |
DN.00010: Requirements for the final phase of Project 8 Kareem Kazkaz Project 8 is an atomic tritium-based experiment to directly measure the mass of the electron anti-neutrino via cyclotron radiation emission spectroscopy. We have adopted a four-phase approach to the measurement, with the final phase having a sensitivity goal of 40 meV. This sensitivity will allow us to either make a positive measurement of the mass or distinguish between normal and inverted neutrino mass ordering. In this presentation we will lay out the broad requirements to meet the scientific goals of Phase IV. We will also provide some details on our efforts to demonstrate key technologies, including the production / cooling / purification of atomic tritium, the design and testing of a magnetic trap for the atoms, methods to observe the femtowatt-scale cyclotron radiation, quantum-limited low-noise amplifiers, and data reduction. |
Thursday, October 25, 2018 11:30AM - 11:45AM |
DN.00011: Fast flavor conversion in dense neutrino media Sajad Abbar, Huaiyu Duan The flavor conversion of a neutrino usually occurs on length scales of its vacuum oscillation wavelength. In a dense neutrino medium such as that in a core-collapse supernova or a binary neutron star merger, this flavor conversion can be expedited by the large densities of the ambient matter and/or neutrinos. We explain the origin of this fast flavor conversion phenomenon and why it may be relevant to supernova physics. |
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