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Book ; Online: Mechanical and Acoustic Studies of Deep Ocean Glass Sphere Implosions

Gorham, P. W. / Rosen, M. / Bolesta, J. W. / Learned, J. G. / Reise, J.

2023

Abstract: The recent likely implosion of the Titan deep ocean submersible's spherical pressure hull has elevated interest and concerns on the nature and dynamics of such events. Here we report on studies of three deep-ocean implosions of 43 cm diameter glass ... ...

Abstract	The recent likely implosion of the Titan deep ocean submersible's spherical pressure hull has elevated interest and concerns on the nature and dynamics of such events. Here we report on studies of three deep-ocean implosions of 43 cm diameter glass instrument housings, made by Benthos Inc. The goal of the studies was to determine the effects on their associated cabling, moorings, and other spheres as part of a larger deep sea observatory. High resolution acoustic profiles were also measured for two of the three implosions, allowing us to infer some of the dynamics and kinematics of the events. The mechanical forces on the ancillary mooring hardware during the entire implosive/explosive event were found to be most probably dominated by the explosive shock wave following the initial infall. A syntactic float at a distance of 16 m from the implosion center was probably shattered by such a shock wave, but 3 glass instrument housings apparently survived within a distance of 6 m from the same implosion. Comment: 13 pages, 8 figures
Keywords	Physics - Instrumentation and Detectors
Subject code	551
Publishing date	2023-09-18
Publishing country	us
Document type	Book ; Online
Database	BASE - Bielefeld Academic Search Engine (life sciences selection)

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Article ; Online: Corrigendum: AGM2015: Antineutrino Global Map 2015.

Usman, S M / Jocher, G R / Dye, S T / McDonough, W F / Learned, J G

Scientific reports

2015 Volume 5, Page(s) 15308

Language	English
Publishing date	2015-10-15
Publishing country	England
Document type	Published Erratum
ZDB-ID	2615211-3
ISSN	2045-2322 ; 2045-2322
ISSN (online)	2045-2322
ISSN	2045-2322
DOI	10.1038/srep15308
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article ; Online: AGM2015: Antineutrino Global Map 2015.

Usman, S M / Jocher, G R / Dye, S T / McDonough, W F / Learned, J G

Scientific reports

2015 Volume 5, Page(s) 13945

Abstract: Every second greater than 10(25) antineutrinos radiate to space from Earth, shining like a faint antineutrino star. Underground antineutrino detectors have revealed the rapidly decaying fission products inside nuclear reactors, verified the long-lived ... ...

Abstract	Every second greater than 10(25) antineutrinos radiate to space from Earth, shining like a faint antineutrino star. Underground antineutrino detectors have revealed the rapidly decaying fission products inside nuclear reactors, verified the long-lived radioactivity inside our planet, and informed sensitive experiments for probing fundamental physics. Mapping the anisotropic antineutrino flux and energy spectrum advance geoscience by defining the amount and distribution of radioactive power within Earth while critically evaluating competing compositional models of the planet. We present the Antineutrino Global Map 2015 (AGM2015), an experimentally informed model of Earth's surface antineutrino flux over the 0 to 11 MeV energy spectrum, along with an assessment of systematic errors. The open source AGM2015 provides fundamental predictions for experiments, assists in strategic detector placement to determine neutrino mass hierarchy, and aids in identifying undeclared nuclear reactors. We use cosmochemically and seismologically informed models of the radiogenic lithosphere/mantle combined with the estimated antineutrino flux, as measured by KamLAND and Borexino, to determine the Earth's total antineutrino luminosity at . We find a dominant flux of geo-neutrinos, predict sub-equal crust and mantle contributions, with ~1% of the total flux from man-made nuclear reactors.
Language	English
Publishing date	2015-09-01
Publishing country	England
Document type	Journal Article
ZDB-ID	2615211-3
ISSN	2045-2322 ; 2045-2322
ISSN (online)	2045-2322
ISSN	2045-2322
DOI	10.1038/srep13945
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Book ; Online: Design and Calibration of an Optically Segmented Single Volume Scatter Camera for Neutron Imaging

Galindo-Tellez, A. / Keefe, K. / Adamek, E. / Brubaker, E. / Crow, B. / Dorrill, R. / Druetzler, A. / Felix, C. J. / Kaneshige, N. / Learned, J. G. / Manfredi, J. J. / Nishimura, K. / Souza, B. Pinto / Schoen, D. / Sweany, M.

2021

Abstract: The Optically Segmented Single Volume Scatter Camera (OS-SVSC) aims to image neutron sources for non-proliferation applications using the kinematic reconstruction of elastic double-scatter events. Our prototype system consists of 64 EJ-204 organic ... ...

Abstract	The Optically Segmented Single Volume Scatter Camera (OS-SVSC) aims to image neutron sources for non-proliferation applications using the kinematic reconstruction of elastic double-scatter events. Our prototype system consists of 64 EJ-204 organic plastic scintillator bars, each measuring 5 mm $\times$ 5 mm $\times$ 200 mm and individually wrapped in Teflon tape. The scintillator array is optically coupled to two silicon photomultiplier ArrayJ-60035 64P-PCB arrays, each comprised of 64 individual 6 $\times$ 6 mm J-Series sensors arranged in an 8 $\times$ 8 array. We detail our calibration efforts, beginning with calibrations for the electronics, based on the IRS3D application-specific integrated circuits, and their associated timing resolutions, ranging from 30 ps to 90 ps. With electronics calibrations applied, energy and position calibrations were performed for a set of edge bars using $^{22}$Na and $^{90}$Sr, respectively, reporting an average resolution of (12.07$\pm$0.03) mm for energy depositions between 900 keVee and 1000 keVee. We further demonstrate a position calibration method for the internal bars of the matrix using cosmic-ray muons as an alternative to emission sources that cannot easily access these bars, with an average measured resolution of (14.86$\pm$0.29) mm for depositions between 900 keVee and 1000 keVee. The coincident time resolution reported between pairs of bars measured up to 400 ps from muon acquisitions. Energy and position calibration values measured with muons are consistent with those obtained using particle emission sources. Comment: 24 pages, 32 figures. Manuscript submitted to Jinst
Keywords	Physics - Instrumentation and Detectors
Subject code	612
Publishing date	2021-02-04
Publishing country	us
Document type	Book ; Online
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Article ; Online: Search for the Majorana Nature of Neutrinos in the Inverted Mass Ordering Region with KamLAND-Zen.

Abe, S / Asami, S / Eizuka, M / Futagi, S / Gando, A / Gando, Y / Gima, T / Goto, A / Hachiya, T / Hata, K / Hayashida, S / Hosokawa, K / Ichimura, K / Ieki, S / Ikeda, H / Inoue, K / Ishidoshiro, K / Kamei, Y / Kawada, N /

Kishimoto, Y / Koga, M / Kurasawa, M / Maemura, N / Mitsui, T / Miyake, H / Nakahata, T / Nakamura, K / Nakamura, R / Ozaki, H / Sakai, T / Sambonsugi, H / Shimizu, I / Shirai, J / Shiraishi, K / Suzuki, A / Suzuki, Y / Takeuchi, A / Tamae, K / Ueshima, K / Watanabe, H / Yoshida, Y / Obara, S / Ichikawa, A K / Chernyak, D / Kozlov, A / Nakamura, K Z / Yoshida, S / Takemoto, Y / Umehara, S / Fushimi, K / Kotera, K / Urano, Y / Berger, B E / Fujikawa, B K / Learned, J G / Maricic, J / Axani, S N / Smolsky, J / Fu, Z / Winslow, L A / Efremenko, Y / Karwowski, H J / Markoff, D M / Tornow, W / Dell'Oro, S / O'Donnell, T / Detwiler, J A / Enomoto, S / Decowski, M P / Grant, C / Li, A / Song, H

Physical review letters

2023 Volume 130, Issue 5, Page(s) 51801

Abstract: The KamLAND-Zen experiment has provided stringent constraints on the neutrinoless double-beta (0νββ) decay half-life in ^{136}Xe using a xenon-loaded liquid scintillator. We report an improved search using an upgraded detector with almost double the ... ...

Abstract	The KamLAND-Zen experiment has provided stringent constraints on the neutrinoless double-beta (0νββ) decay half-life in ^{136}Xe using a xenon-loaded liquid scintillator. We report an improved search using an upgraded detector with almost double the amount of xenon and an ultralow radioactivity container, corresponding to an exposure of 970 kg yr of ^{136}Xe. These new data provide valuable insight into backgrounds, especially from cosmic muon spallation of xenon, and have required the use of novel background rejection techniques. We obtain a lower limit for the 0νββ decay half-life of T_{1/2}^{0ν}>2.3×10^{26} yr at 90% C.L., corresponding to upper limits on the effective Majorana neutrino mass of 36-156 meV using commonly adopted nuclear matrix element calculations.
Language	English
Publishing date	2023-02-17
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.130.051801
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Book ; Online: Hanohano:A Deep Ocean Antineutrino Observatory

Batygov, M. / Dye, S. T. / Learned, J. G. / Matsuno, S. / Pakvasa, S. / Varner, G.

2008

Abstract: This paper presents the science potential of a deep ocean antineutrino observatory being developed at Hawaii and elsewhere. The observatory design allows for relocation from one site to another. Positioning the observaory some 60 km distant from a ... ...

Abstract	This paper presents the science potential of a deep ocean antineutrino observatory being developed at Hawaii and elsewhere. The observatory design allows for relocation from one site to another. Positioning the observaory some 60 km distant from a nuclear reactor complex enables preecision measurement of neutrino mixing parameters, leading to a determination of neutrino mass hierarchy and theta_13. At a mid-Pacific location, the observatory measures the flux of uranium and thorium decay series antineutrinos from earth's mantle and performs a sensitive search for a hypothetical natural fission reactor in earth's core. A subequent deployment at another mid-ocean location would test lateral homogeneity of uranium and thorium in earth's mantle. These measurements have significance for earth energy studies. Comment: Poster presented at ICHEP08, Philadelphia, USA, July 2008. 3 pages. PDF
Keywords	High Energy Physics - Experiment ; High Energy Physics - Phenomenology
Subject code	551
Publishing date	2008-10-02
Publishing country	us
Document type	Book ; Online
Database	BASE - Bielefeld Academic Search Engine (life sciences selection)

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Article ; Online: Invited Article: miniTimeCube.

Li, V A / Dorrill, R / Duvall, M J / Koblanski, J / Negrashov, S / Sakai, M / Wipperfurth, S A / Engel, K / Jocher, G R / Learned, J G / Macchiarulo, L / Matsuno, S / McDonough, W F / Mumm, H P / Murillo, J / Nishimura, K / Rosen, M / Usman, S M / Varner, G S

The Review of scientific instruments

2016 Volume 87, Issue 2, Page(s) 21301

Abstract: We present the development of the miniTimeCube (mTC), a novel compact neutrino detector. The mTC is a multipurpose detector, aiming to detect not only neutrinos but also fast/thermal neutrons. Potential applications include the counterproliferation of ... ...

Abstract	We present the development of the miniTimeCube (mTC), a novel compact neutrino detector. The mTC is a multipurpose detector, aiming to detect not only neutrinos but also fast/thermal neutrons. Potential applications include the counterproliferation of nuclear materials and the investigation of antineutrino short-baseline effects. The mTC is a plastic 0.2% (10)B-doped scintillator (13 cm)(3) cube surrounded by 24 Micro-Channel Plate (MCP) photon detectors, each with an 8 × 8 anode totaling 1536 individual channels/pixels viewing the scintillator. It uses custom-made electronics modules which mount on top of the MCPs, making our detector compact and able to both distinguish different types of events and reject noise in real time. The detector is currently deployed and being tested at the National Institute of Standards and Technology Center for Neutron Research nuclear reactor (20 MWth) in Gaithersburg MD. A shield for further tests is being constructed, and calibration and upgrades are ongoing. The mTC's improved spatiotemporal resolution will allow for determination of incident particle directions beyond previous capabilities.
Language	English
Publishing date	2016-02
Publishing country	United States
Document type	Journal Article
ZDB-ID	209865-9
ISSN	1089-7623 ; 0034-6748
ISSN (online)	1089-7623
ISSN	0034-6748
DOI	10.1063/1.4942243
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Article ; Online: Precision Analysis of the ^{136}Xe Two-Neutrino ββ Spectrum in KamLAND-Zen and Its Impact on the Quenching of Nuclear Matrix Elements.

Gando, A / Gando, Y / Hachiya, T / Ha Minh, M / Hayashida, S / Honda, Y / Hosokawa, K / Ikeda, H / Inoue, K / Ishidoshiro, K / Kamei, Y / Kamizawa, K / Kinoshita, T / Koga, M / Matsuda, S / Mitsui, T / Nakamura, K / Ono, A / Ota, N /

Otsuka, S / Ozaki, H / Shibukawa, Y / Shimizu, I / Shirahata, Y / Shirai, J / Sato, T / Soma, K / Suzuki, A / Takeuchi, A / Tamae, K / Ueshima, K / Watanabe, H / Chernyak, D / Kozlov, A / Obara, S / Yoshida, S / Takemoto, Y / Umehara, S / Fushimi, K / Hirata, S / Berger, B E / Fujikawa, B K / Learned, J G / Maricic, J / Winslow, L A / Efremenko, Y / Karwowski, H J / Markoff, D M / Tornow, W / O'Donnell, T / Detwiler, J A / Enomoto, S / Decowski, M P / Menéndez, J / Dvornický, R / Šimkovic, F

Physical review letters

2019 Volume 122, Issue 19, Page(s) 192501

Abstract: We present a precision analysis of the ^{136}Xe two-neutrino ββ electron spectrum above 0.8 MeV, based on high-statistics data obtained with the KamLAND-Zen experiment. An improved formalism for the two-neutrino ββ rate allows us to measure the ratio of ... ...

Abstract	We present a precision analysis of the ^{136}Xe two-neutrino ββ electron spectrum above 0.8 MeV, based on high-statistics data obtained with the KamLAND-Zen experiment. An improved formalism for the two-neutrino ββ rate allows us to measure the ratio of the leading and subleading 2νββ nuclear matrix elements (NMEs), ξ_{31}^{2ν}=-0.26_{-0.25}^{+0.31}. Theoretical predictions from the nuclear shell model and the majority of the quasiparticle random-phase approximation (QRPA) calculations are consistent with the experimental limit. However, part of the ξ_{31}^{2ν} range allowed by the QRPA is excluded by the present measurement at the 90% confidence level. Our analysis reveals that predicted ξ_{31}^{2ν} values are sensitive to the quenching of NMEs and the competing contributions from low- and high-energy states in the intermediate nucleus. Because these aspects are also at play in neutrinoless ββ decay, ξ_{31}^{2ν} provides new insights toward reliable neutrinoless ββ NMEs.
Language	English
Publishing date	2019-05-31
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.122.192501
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Article ; Online: Search for Cosmic-Ray Boosted Sub-GeV Dark Matter Using Recoil Protons at Super-Kamiokande.

Abe, K / Hayato, Y / Hiraide, K / Ieki, K / Ikeda, M / Kameda, J / Kanemura, Y / Kaneshima, R / Kashiwagi, Y / Kataoka, Y / Miki, S / Mine, S / Miura, M / Moriyama, S / Nakano, Y / Nakahata, M / Nakayama, S / Noguchi, Y / Okamoto, K /

Sato, K / Sekiya, H / Shiba, H / Shimizu, K / Shiozawa, M / Sonoda, Y / Suzuki, Y / Takeda, A / Takemoto, Y / Takenaka, A / Tanaka, H / Watanabe, S / Yano, T / Han, S / Kajita, T / Okumura, K / Tashiro, T / Tomiya, T / Wang, X / Xia, J / Yoshida, S / Megias, G D / Fernandez, P / Labarga, L / Ospina, N / Zaldivar, B / Pointon, B W / Kearns, E / Raaf, J L / Wan, L / Wester, T / Bian, J / Griskevich, N J / Kropp, W R / Locke, S / Smy, M B / Sobel, H W / Takhistov, V / Yankelevich, A / Hill, J / Park, R G / Bodur, B / Scholberg, K / Walter, C W / Bernard, L / Coffani, A / Drapier, O / El Hedri, S / Giampaolo, A / Mueller, Th A / Santos, A D / Paganini, P / Quilain, B / Ishizuka, T / Nakamura, T / Jang, J S / Learned, J G / Choi, K / Cao, S / Anthony, L H V / Martin, D / Scott, M / Sztuc, A A / Uchida, Y / Berardi, V / Catanesi, M G / Radicioni, E / Calabria, N F / Machado, L N / De Rosa, G / Collazuol, G / Iacob, F / Lamoureux, M / Mattiazzi, M / Ludovici, L / Gonin, M / Pronost, G / Fujisawa, C / Maekawa, Y / Nishimura, Y / Friend, M / Hasegawa, T / Ishida, T / Kobayashi, T / Jakkapu, M / Matsubara, T / Nakadaira, T / Nakamura, K / Oyama, Y / Sakashita, K / Sekiguchi, T / Tsukamoto, T / Boschi, T / Di Lodovico, F / Gao, J / Goldsack, A / Katori, T / Migenda, J / Taani, M / Zsoldos, S / Kotsar, Y / Ozaki, H / Suzuki, A T / Takeuchi, Y / Bronner, C / Feng, J / Kikawa, T / Mori, M / Nakaya, T / Wendell, R A / Yasutome, K / Jenkins, S J / McCauley, N / Mehta, P / Tsui, K M / Fukuda, Y / Itow, Y / Menjo, H / Ninomiya, K / Lagoda, J / Lakshmi, S M / Mandal, M / Mijakowski, P / Prabhu, Y S / Zalipska, J / Jia, M / Jiang, J / Jung, C K / Wilking, M J / Yanagisawa, C / Harada, M / Ishino, H / Ito, S / Kitagawa, H / Koshio, Y / Nakanishi, F / Sakai, S / Barr, G / Barrow, D / Cook, L / Samani, S / Wark, D / Nova, F / Yang, J Y / Malek, M / McElwee, J M / Stone, O / Thiesse, M D / Thompson, L F / Okazawa, H / Kim, S B / Seo, J W / Yu, I / Ichikawa, A K / Nakamura, K D / Tairafune, S / Nishijima, K / Iwamoto, K / Nakagiri, K / Nakajima, Y / Taniuchi, N / Yokoyama, M / Martens, K / de Perio, P / Vagins, M R / Kuze, M / Izumiyama, S / Inomoto, M / Ishitsuka, M / Ito, H / Kinoshita, T / Matsumoto, R / Ommura, Y / Shigeta, N / Shinoki, M / Suganuma, T / Yamauchi, K / Martin, J F / Tanaka, H A / Towstego, T / Akutsu, R / Gousy-Leblanc, V / Hartz, M / Konaka, A / Prouse, N W / Chen, S / Xu, B D / Zhang, B / Posiadala-Zezula, M / Hadley, D / Nicholson, M / O'Flaherty, M / Richards, B / Ali, A / Jamieson, B / Marti, Ll / Minamino, A / Pintaudi, G / Sano, S / Suzuki, S / Wada, K

Physical review letters

2023 Volume 130, Issue 3, Page(s) 31802

Abstract: We report a search for cosmic-ray boosted dark matter with protons using the 0.37 megaton×years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric ... ...

Abstract	We report a search for cosmic-ray boosted dark matter with protons using the 0.37 megaton×years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric neutrino background from the vicinity of the Galactic Center. No such excess is observed, and limits are calculated for two reference models of dark matter with either a constant interaction cross section or through a scalar mediator. This is the first experimental search for boosted dark matter with hadrons using directional information. The results present the most stringent limits on cosmic-ray boosted dark matter and exclude the dark matter-nucleon elastic scattering cross section between 10^{-33}cm^{2} and 10^{-27}cm^{2} for dark matter mass from 1 MeV/c^{2} to 300 MeV/c^{2}.
Language	English
Publishing date	2023-02-11
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.130.031802
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Article ; Online: Erratum: Search for Cosmic-Ray Boosted Sub-GeV Dark Matter Using Recoil Protons at Super-Kamiokande [Phys. Rev. Lett. 130, 031802 (2023)].

Physical review letters

2023 Volume 131, Issue 15, Page(s) 159903

Abstract: This corrects the article DOI: 10.1103/PhysRevLett.130.031802. ...

Abstract	This corrects the article DOI: 10.1103/PhysRevLett.130.031802.
Language	English
Publishing date	2023-10-26
Publishing country	United States
Document type	Published Erratum
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.131.159903
Database	MEDical Literature Analysis and Retrieval System OnLINE

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