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For years, earth-based neutrino detectors have been run and operated to detect the elusive neutrino. These have historically been enormous underground detectors. The neutrino Solar Orbiting Laboratory ($\nu$SOL) project is working to design…

Instrumentation and Methods for Astrophysics · Physics 2022-10-17 Jonathan Folkerts

This thesis investigates the detection of ultra high energy (E > 1 EeV) cosmic neutrinos using acoustic sensors immersed in water. The method is based on the thermoacoustic model describing the production of microsecond bipolar acoustic…

Astrophysics · Physics 2007-05-23 Timo Karg

A possible detection of ultra-high-energy neutrinos has been attempted since decades through the Askarian radiation and different observation techniques. In fact, when such energetic neutrinos interact in a medium are able to produce a…

Instrumentation and Methods for Astrophysics · Physics 2023-01-09 Antonio Marinelli , Pasquale Migliozzi , Andreino Simonelli

With 2.5x the previously reported exposure, the Daya Bay experiment has improved the measurement of the neutrino mixing parameter sin^2(2theta_13) = 0.089+-0.010(stat)+-0.005(syst). Reactor anti-neutrinos were produced by six 2.9 GW(th)…

High Energy Physics - Experiment · Physics 2019-08-13 Daniel A. Dwyer

We compare the physics potential of two representative options for a SuperBeam in Europe, studying the achievable precision at 1\sigma with which the CP violation phase (\delta) could be measured, as well as the mass hierarchy and CP…

High Energy Physics - Phenomenology · Physics 2015-06-05 Pilar Coloma , Enrique Fernandez-Martinez , Luis Labarga

We present the results of a search for high energy neutrinos with the Baikal underwater Cherenkov detector NT-96. An upper limit to the flux of \nu_e + \nu_{\mu} + \bar{\nu_{\mu}} of E^2F_{\nu}(E)<1.4 10^{-5} cm^{-2} s^{-1} sr^{-1} GeV is…

Astrophysics · Physics 2007-05-23 BAIKAL Collaboration , V. Balkanov

We point out that with improving our present knowledge of experimental neutrino physics it will be possible to locate nuclear powered vehicles like submarines, aircraft carriers and UFOs and detect nuclear testing. Since neutrinos cannot be…

High Energy Physics - Phenomenology · Physics 2007-05-23 P. Panigrahi , U. Sarkar

We note that detector depth can influence the decay path length available for the primary and secondary particles that are the source of atmospheric neutrinos. As a consequence there is a location dependent modulation to the neutrino flux,…

High Energy Physics - Experiment · Physics 2009-11-10 John M. LoSecco

We examine the reach of a Beta-beam experiment with two detectors at carefully chosen baselines for exploring neutrino mass parameters. Locating the source at CERN, the two detectors and baselines are: (a) a 50 kton iron calorimeter (ICAL)…

High Energy Physics - Phenomenology · Physics 2008-11-26 Sanjib Kumar Agarwalla , Sandhya Choubey , Amitava Raychaudhuri

The ANTARES collaboration is constructing a neutrino telescope in the Mediterranean Sea at a depth of 2400 metres, about 40 kilometres off the French coast near Toulon. The detector will consist of 12 vertical strings anchored at the sea…

Astrophysics · Physics 2019-08-14 U. F. Katz

Next generation neutrino oscillation experiments like DUNE and T2HK are multi-purpose observatories, with a rich physics program beyond oscillation measurements. A special role is played by their near detector facilities, which are…

High Energy Physics - Phenomenology · Physics 2022-02-11 Moritz Breitbach , Luca Buonocore , Claudia Frugiuele , Joachim Kopp , Lukas Mittnacht

We investigate the problem of detecting the presence of clandestine neutron sources, such as would be produced by nuclear weapons containing plutonium, within cargo containers. Small, simple and economical semiconductor photodiode detectors…

Physics and Society · Physics 2012-05-22 J. I. Katz

We analyze the expected arrival time spectrum of supernova neutrinos using simulated luminosity and compute the expected number of events in future detectors such as the DUNE Far Detector and Hyper-Kamiokande. We develop a general method…

High Energy Physics - Phenomenology · Physics 2023-06-06 C. A. Moura , L. Quintino , F. Rossi-Torres

We report the first search result for the flux of astrophysical electron antineutrinos for energies O(10) MeV in the gadolinium-loaded Super-Kamiokande (SK) detector. In June 2020, gadolinium was introduced to the ultra-pure water of the SK…

High Energy Astrophysical Phenomena · Physics 2023-08-02 M. Harada , K. Abe , C. Bronner , Y. Hayato , K. Hiraide , K. Hosokawa , K. Ieki , M. Ikeda , J. Kameda , Y. Kanemura , R. Kaneshima , Y. Kashiwagi , Y. Kataoka , S. Miki , S. Mine , M. Miura , S. Moriyama , Y. Nakano , M. Nakahata , S. Nakayama , Y. Noguchi , K. Okamoto , K. Sato , H. Sekiya , H. Shiba , K. Shimizu , M. Shiozawa , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , S. Watanabe , T. Yano , S. Han , T. Kajita , K. Okumura , T. Tashiro , T. Tomiya , X. Wang , S. Yoshida , G. D. Megias , P. Fernandez , L. Labarga , N. Ospina , B. Zaldivar , B. W. Pointon , E. Kearns , J. L. Raaf , L. Wan , T. Wester , J. Bian , N. J. Griskevich , S. Locke , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , J. Hill , S. H. Lee , D. H. Moon , R. G. Park , B. Bodur , K. Scholberg , C. W. Walter , A. Beauchene , O. Drapier , A. Giampaolo , Th. A. Mueller , A. D. Santos , P. Paganini , B. Quilain , T. Ishizuka , T. Nakamura , J. S. Jang , J. G. Learned , K. Choi , N. Iovine , S. Cao , L. H. V. Anthony , D. Martin , M. Scott , A. A. Sztuc , Y. Uchida , V. Berardi , M. G. Catanesi , E. Radicioni , N. F. Calabria , A. Langella , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , M. Mattiazzi , L. Ludovici , M. Gonin , G. Pronost , C. Fujisawa , Y. Maekawa , Y. Nishimura , R. Okazaki , R. Akutsu , M. Friend , T. Hasegawa , T. Ishida , T. Kobayashi , M. Jakkapu , T. Matsubara , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , N. Bhuiyan , G. T. Burton , F. Di Lodovico , J. Gao , A. Goldsack , T. Katori , J. Migenda , Z. Xie , S. Zsoldos , Y. Kotsar , H. Ozaki , A. T. Suzuki , Y. Takagi , Y. Takeuchi , J. Feng , L. Feng , J. R. Hu , Z. Hu , T. Kikawa , M. Mori , T. Nakaya , R. A. Wendell , K. Yasutome , S. J. Jenkins , N. McCauley , P. Mehta , A. Tarrant , Y. Fukuda , Y. Itow , H. Menjo , K. Ninomiya , J. Lagoda , S. M. Lakshmi , M. Mandal , P. Mijakowski , Y. S. Prabhu , J. Zalipska , M. Jia , J. Jiang , C. K. Jung , M. J. Wilking , C. Yanagisawa , Y. Hino , H. Ishino , H. Kitagawa , Y. Koshio , F. Nakanishi , S. Sakai , T. Tada , T. Tano , G. Barr , D. Barrow , L. Cook , S. Samani , D. Wark , A. Holin , F. Nova , B. S. Yang , J. Y. Yang , J. Yoo , J. E. P. Fannon , L. Kneale , M. Malek , J. M. McElwee , M. D. Thiesse , L. F. Thompson , S. T. Wilson , H. Okazawa , S. B. Kim , E. Kwon , J. W. Seo , I. Yu , A. K. Ichikawa , K. D. Nakamura , S. Tairafune , K. Nishijima , K. Nakagiri , Y. Nakajima , S. Shima , N. Taniuchi , E. Watanabe , M. Yokoyama , P. de Perio , K. Martens , K. M. Tsui , M. R. Vagins , J. Xia , M. Kuze , S. Izumiyama , R. Matsumoto , M. Ishitsuka , H. Ito , T. Kinoshita , Y. Ommura , N. Shigeta , M. Shinoki , T. Suganuma , K. Yamauchi , J. F. Martin , H. A. Tanaka , T. Towstego , R. Gaur , V. Gousy-Leblanc , M. Hartz , A. Konaka , X. Li , N. W. Prouse , S. Chen , B. D. Xu , B. Zhang , M. Posiadala-Zezula , S. B. Boyd , R. Edwards , D. Hadley , M. Nicholson , M. O Flaherty , B. Richards , A. Ali , B. Jamieson , Ll. Marti , A. Minamino , G. Pintaudi , S. Sano , S. Suzuki , K. Wada

We discuss several new ideas for reactor neutrino oscillation experiments with a Large Liquid Scintillator Detector. We consider two different scenarios for a measurement of the small mixing angle $\theta_{13}$ with a mobile $\bar{\nu}_e$…

High Energy Physics - Phenomenology · Physics 2010-10-27 Joachim Kopp , Manfred Lindner , Alexander Merle , Mark Rolinec

We study the advantages of a second identical detector at a medium baseline reactor neutrino experiment. A major obstruction to the determination of the neutrino mass hierarchy is the detector's unknown nonlinear energy response, which even…

High Energy Physics - Phenomenology · Physics 2014-04-23 Emilio Ciuffoli , Jarah Evslin , Zhimin Wang , Changgen Yang , Xinmin Zhang , Weili Zhong

The MINERvA experiment is designed to perform precision studies of neutrino-nucleus scattering using $\nu_\mu$ and ${\bar\nu}_\mu$ neutrinos incident at 1-20 GeV in the NuMI beam at Fermilab. This article presents a detailed description of…

A natural nuclear fission reactor with a power output of 3- 10 terawatt at the center of the earth has been proposed as the energy source of the earth's magnetic field. The proposal can be directly tested by a massive liquid scintillation…

High Energy Physics - Experiment · Physics 2007-05-23 R. S. Raghavan

The possibility to improve the CERN to Gran Sasso neutrino beam performances for theta_{13} searches is investigated. We show that by an appropriate optimization of the target and focusing optics of the present CNGS design, we can increase…

High Energy Physics - Phenomenology · Physics 2009-11-07 A. Rubbia , P. Sala

Research on accelerator driven systems (ADS), related new fuels and their ability for nuclear waste incineration has led to a revival of interest in nuclear cross sections of many nuclides over a large energy range. Discrepancies observed…

Nuclear Experiment · Physics 2007-05-23 L. Perrot , A. Billebaud , R. Brissot , A. Giorni , D. Heuer , J. -M. Loiseaux , O. Meplan , J. -B. Viano
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