693 research outputs found

    Special values of finite multiple harmonic q-series at roots of unity

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    We study special values of finite multiple harmonic q-series at roots of unity. These objects were recently introduced by the authors and it was shown that they have connections to finite and symmetric multiple zeta values and the Kaneko-Zagier conjecture. In this note we give new explicit evaluations for finite multiple harmonic q-series at roots of unity and prove Ohno-Zagier-type relations for them

    Search for exotic neutrino-electron interactions using solar neutrinos in XMASS-I

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    We have searched for exotic neutrino-electron interactions that could be produced by a neutrino millicharge, by a neutrino magnetic moment, or by dark photons using solar neutrinos in the XMASS-I liquid xenon detector. We observed no significant signals in 711 days of data. We obtain an upper limit for neutrino millicharge of 5.4×\times10−12e^{-12} e at 90\% confidence level assuming all three species of neutrino have common millicharge. We also set flavor dependent limits assuming the respective neutrino flavor is the only one carrying a millicharge, 7.3×10−12e7.3 \times 10^{-12} e for νe\nu_e, 1.1×10−11e1.1 \times 10^{-11} e for νμ\nu_{\mu}, and 1.1×10−11e1.1 \times 10^{-11} e for ντ\nu_{\tau}. These limits are the most stringent yet obtained from direct measurements. We also obtain an upper limit for the neutrino magnetic moment of 1.8×\times10−10^{-10} Bohr magnetons. In addition, we obtain upper limits for the coupling constant of dark photons in the U(1)B−LU(1)_{B-L} model of 1.3×\times10−6^{-6} if the dark photon mass is 1×10−3\times 10^{-3} MeV/c2/c^{2}, and 8.8×\times10−5^{-5} if it is 10 MeV/c2/c^{2}

    Search for two-neutrino double electron capture on 124^{124}Xe with the XMASS-I detector

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    Double electron capture is a rare nuclear decay process in which two orbital electrons are captured simultaneously in the same nucleus. Measurement of its two-neutrino mode would provide a new reference for the calculation of nuclear matrix elements whereas observation of its neutrinoless mode would demonstrate lepton number violation. A search for two-neutrino double electron capture on 124^{124}Xe is performed using 165.9 days of data collected with the XMASS-I liquid xenon detector. No significant excess above background was observed and we set a lower limit on the half-life as 4.7×10214.7 \times 10^{21} years at 90% confidence level. The obtained limit has ruled out parts of some theoretical expectations. We obtain a lower limit on the 126^{126}Xe two-neutrino double electron capture half-life of 4.3×10214.3 \times 10^{21} years at 90% confidence level as well.Comment: 6 pages, 3 figures, accepted for publication in Physics Letters

    Direct dark matter search by annual modulation in XMASS-I

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    A search for dark matter was conducted by looking for an annual modulation signal due to the Earth's rotation around the Sun using XMASS, a single phase liquid xenon detector. The data used for this analysis was 359.2 live days times 832 kg of exposure accumulated between November 2013 and March 2015. When we assume Weakly Interacting Massive Particle (WIMP) dark matter elastically scattering on the target nuclei, the exclusion upper limit of the WIMP-nucleon cross section 4.3×\times10−41^{-41}cm2^2 at 8 GeV/c2^2 was obtained and we exclude almost all the DAMA/LIBRA allowed region in the 6 to 16 GeV/c2^2 range at ∼\sim10−40^{-40}cm2^2. The result of a simple modulation analysis, without assuming any specific dark matter model but including electron/γ\gamma events, showed a slight negative amplitude. The pp-values obtained with two independent analyses are 0.014 and 0.068 for null hypothesis, respectively. we obtained 90\% C.L. upper bounds that can be used to test various models. This is the first extensive annual modulation search probing this region with an exposure comparable to DAMA/LIBRA.Comment: 5 pages, 4 figure

    Distillation of Liquid Xenon to Remove Krypton

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    A high performance distillation system to remove krypton from xenon was constructed, and a purity level of Kr/Xe = ∼3×10−12\sim 3 \times 10^{-12} was achieved. This development is crucial in facilitating high sensitivity low background experiments such as the search for dark matter in the universe.Comment: 15 pages, 11 figure
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