neutrino

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「an elementary particle with zero charge and zero mass」

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「中性微子(放射性物質の崩壊のとき放出される素粒子)」

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出典(authority):フリー百科事典『ウィキペディア(Wikipedia)』「2016/02/26 05:39:26」(JST)

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英文文献

  • Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube.
  • Aartsen MG, Ackermann M, Adams J, Aguilar JA, Ahlers M, Ahrens M, Altmann D, Anderson T, Arguelles C, Arlen TC, Auffenberg J, Bai X, Barwick SW, Baum V, Bay R, Beatty JJ, Becker Tjus J, Becker KH, BenZvi S, Berghaus P, Berley D, Bernardini E, Bernhard A, Besson DZ, Binder G, Bindig D, Bissok M, Blaufuss E, Blumenthal J, Boersma DJ, Bohm C, Bos F, Bose D, Böser S, Botner O, Brayeur L, Bretz HP, Brown AM, Buzinsky N, Casey J, Casier M, Cheung E, Chirkin D, Christov A, Christy B, Clark K, Classen L, Clevermann F, Coenders S, Cowen DF, Cruz Silva AH, Daughhetee J, Davis JC, Day M, de André JP, De Clercq C, Dembinski H, De Ridder S, Desiati P, de Vries KD, de With M, DeYoung T, Díaz-Vélez JC, Dumm JP, Dunkman M, Eagan R, Eberhardt B, Ehrhardt T, Eichmann B, Eisch J, Euler S, Evenson PA, Fadiran O, Fazely AR, Fedynitch A, Feintzeig J, Felde J, Filimonov K, Finley C, Fischer-Wasels T, Flis S, Frantzen K, Fuchs T, Gaisser TK, Gaior R, Gallagher J, Gerhardt L, Gier D, Gladstone L, Glüsenkamp T, Goldschmidt A, Golup G, Gonzalez JG, Goodman JA, Góra D, Grant D, Gretskov P, Groh JC, Groß A, Ha C, Haack C, Haj Ismail A, Hallen P, Hallgren A, Halzen F, Hanson K, Hebecker D, Heereman D, Heinen D, Helbing K, Hellauer R, Hellwig D, Hickford S, Hill GC, Hoffman KD, Hoffmann R, Homeier A, Hoshina K, Huang F, Huelsnitz W, Hulth PO, Hultqvist K, Ishihara A, Jacobi E, Jacobsen J, Japaridze GS, Jero K, Jurkovic M, Kaminsky B, Kappes A, Karg T, Karle A, Kauer M, Keivani A, Kelley JL, Kheirandish A, Kiryluk J, Kläs J, Klein SR, Köhne JH, Kohnen G, Kolanoski H, Koob A, Köpke L, Kopper C, Kopper S, Koskinen DJ, Kowalski M, Kriesten A, Krings K, Kroll G, Kroll M, Kunnen J, Kurahashi N, Kuwabara T, Labare M, Lanfranchi JL, Larsen DT, Larson MJ, Lesiak-Bzdak M, Leuermann M, Lünemann J, Madsen J, Maggi G, Maruyama R, Mase K, Matis HS, Maunu R, McNally F, Meagher K, Medici M, Meli A, Meures T, Miarecki S, Middell E, Middlemas E, Milke N, Miller J, Mohrmann L, Montaruli T, Morse R, Nahnhauer R, Naumann U, Niederhausen H, Nowicki SC, Nygren DR, Obertacke A, Olivas A, Omairat A, O'Murchadha A, Palczewski T, Paul L, Penek Ö, Pepper JA, Pérez de Los Heros C, Pfendner C, Pieloth D, Pinat E, Posselt J, Price PB, Przybylski GT, Pütz J, Quinnan M, Rädel L, Rameez M, Rawlins K, Redl P, Rees I, Reimann R, Relich M, Resconi E, Rhode W, Richman M, Riedel B, Robertson S, Rodrigues JP, Rongen M, Rott C, Ruhe T, Ruzybayev B, Ryckbosch D, Saba SM, Sander HG, Sandroos J, Santander M, Sarkar S, Schatto K, Scheriau F, Schmidt T, Schmitz M, Schoenen S, Schöneberg S, Schönwald A, Schukraft A, Schulte L, Schulz O, Seckel D, Sestayo Y, Seunarine S, Shanidze R, Smith MW, Soldin D, Spiczak GM, Spiering C, Stamatikos M, Stanev T, Stanisha NA, Stasik A, Stezelberger T, Stokstad RG, Stößl A, Strahler EA, Ström R, Strotjohann NL, Sullivan GW, Taavola H, Taboada I, Tamburro A, Ter-Antonyan S, Terliuk A, Tešić G, Tilav S, Toale PA, Tobin MN, Tosi D, Tselengidou M, Unger E, Usner M, Vallecorsa S, van Eijndhoven N, Vandenbroucke J, van Santen J, Vanheule S, Vehring M, Voge M, Vraeghe M, Walck C, Wallraff M, Weaver Ch, Wellons M, Wendt C, Westerhoff S, Whelan BJ, Whitehorn N, Wichary C, Wiebe K, Wiebusch CH, Williams DR, Wissing H, Wolf M, Wood TR, Woschnagg K, Xu DL, Xu XW, Xu Y, Yanez JP, Yodh G, Yoshida S, Zarzhitsky P, Ziemann J, Zoll M; IceCube Collaboration.
  • Physical review letters.Phys Rev Lett.2015 May 1;114(17):171102. Epub 2015 Apr 28.
  • A diffuse flux of astrophysical neutrinos above 100 TeV has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to 35 TeV and analyze its flavor composition by classifying events as showers or tracks. Taking advantage of lower atmosp
  • PMID 25978221
  • What is the Flavor of the Cosmic Neutrinos Seen by IceCube?
  • Palladino A1, Pagliaroli G2, Villante FL2,3, Vissani F1,2.
  • Physical review letters.Phys Rev Lett.2015 May 1;114(17):171101. Epub 2015 Apr 28.
  • We analyze the high-energy neutrino events observed by IceCube, aiming to probe the initial flavor of cosmic neutrinos. We study the track-to-shower ratio of the subset with energy above 60 TeV, where the signal is expected to dominate, and show that different production mechanisms give rise to dif
  • PMID 25978220
  • Neutrino oscillation studies with reactors.
  • Vogel P1, Wen LJ2, Zhang C3.
  • Nature communications.Nat Commun.2015 Apr 27;6:6935. doi: 10.1038/ncomms7935.
  • Nuclear reactors are one of the most intense, pure, controllable, cost-effective and well-understood sources of neutrinos. Reactors have played a major role in the study of neutrino oscillations, a phenomenon that indicates that neutrinos have mass and that neutrino flavours are quantum mechanical m
  • PMID 25913819

和文文献

  • Study on Correlation between Electrochemical-Neutrino-Detector Signal and Solar Wind Velocity
  • Nakamura Shouhei,Terao Norichika,Aida Nur,Ishibashi Kenji,石橋 健二,ナカムラ ショウヘイ,テラオ ノリチカ,イシバシ ケンジ
  • Memoirs of the Faculty of Engineering, Kyushu University 73(1), 39-46, 2013-06-24
  • We have developed an electrochemical detector which is sensitive to both reactor neutrinos and natural background neutrinos. The output current of the detector produces a peak at the first 1-3 days, a …
  • NAID 120005303387
  • Proposed Analysis on Output Currents of Electrochemical Apparatus with Regards to Weak Interaction
  • Aida Nur,Ishibashi Kenji,Imahayashi Youichi,Suda Shoya,Nakamura Shouhei,石橋 健二,イシバシ ケンジ,イマハヤシ ヨウイチ,スダ ショウヤ,ナカムラ ショウヘイ
  • Memoirs of the Faculty of Engineering, Kyushu University 73(1), 27-37, 2013-06-24
  • … We formulate the output current of neutrino interaction in the electrochemical apparatus with an electrochemical half-cell model under the postulated influence of weak interaction. … they are reactions by either environmental neutrinos or nuclear-reactor-neutrino irradiation. …
  • NAID 120005303386
  • 時刻・周波数標準の遠距離比較伝送技術の現状と将来
  • 井戸 哲也,藤枝 美穂
  • 日本物理學會誌 68(4), 209-216, 2013-04-05
  • 近年の光周波数標準の急速な発展や,長基線ニュートリノ振動実験により周波数標準や時刻の遠距離比較伝送技術が注目されている.現在,周波数の伝送については光ファイバを使用した伝送技術により19桁の不確かさでの伝送が可能になっており,また時刻比較では人工衛星を介することで数100ピコ秒の測定精度が得られている.本稿ではこれらの技術についてその概略を解説し,また具体的応用例として最近行われたNICT-東大間 …
  • NAID 110009603879

関連リンク

ニュートリノ(英: neutrino)は、素粒子のうちの中性レプトンの名称。中性微子とも書く。 電子ニュートリノ・ミューニュートリノ・タウニュートリノの3種類もしくはそれぞれの反粒子 をあわせた6種類あると考えられている。ヴォルフガング・パウリが中性子のβ崩壊で ...
A neutrino (pron.: /njuːˈtriːnoʊ/; Italian pronunciation: [neuˈtriːno]) is an electrically neutral, weakly interacting elementary subatomic particle with half- integer spin. The neutrino (meaning "small neutral one" in Italian) is denoted by the ...

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neutrinos neutrino physicists tend to have typical neutrino eventat Super KSolar neutrino oscillationNeutrino Detectors are the CoolestneutrinoElectron neutrino produces an electron


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拡張検索antineutrino

antineutrino」

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WordNet   license wordnet

「the antiparticle of a neutrino」

PrepTutorEJDIC   license prepejdic

「反中性微子」




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