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K2K: Long Baseline Neutrino Oscillation Experiment

Amioka- Long Baseline Neutrino Oscillation Experiment. K2K Long-baseline Neutrino Oscillation Experiment. K2K Collaboration, January, 2004. For official information about K2K, or to request a speaker. At a scientific conference, please contact the spokesperson. Final result of K2K oscillation measurement has been published in Physical Review D. Prof Koichiro Nishikawa was awarded the Nishina Memorial Prize. 200511.14) / Japanese. 200410.29) /KEK news [ Japanese Only. SciBar detector in operation! K2K Dat...

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K2K: Long Baseline Neutrino Oscillation Experiment | neutrino.kek.jp Reviews
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Amioka- Long Baseline Neutrino Oscillation Experiment. K2K Long-baseline Neutrino Oscillation Experiment. K2K Collaboration, January, 2004. For official information about K2K, or to request a speaker. At a scientific conference, please contact the spokesperson. Final result of K2K oscillation measurement has been published in Physical Review D. Prof Koichiro Nishikawa was awarded the Nishina Memorial Prize. 200511.14) / Japanese. 200410.29) /KEK news [ Japanese Only. SciBar detector in operation! K2K Dat...
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K2K: Long Baseline Neutrino Oscillation Experiment | neutrino.kek.jp Reviews

https://neutrino.kek.jp

Amioka- Long Baseline Neutrino Oscillation Experiment. K2K Long-baseline Neutrino Oscillation Experiment. K2K Collaboration, January, 2004. For official information about K2K, or to request a speaker. At a scientific conference, please contact the spokesperson. Final result of K2K oscillation measurement has been published in Physical Review D. Prof Koichiro Nishikawa was awarded the Nishina Memorial Prize. 200511.14) / Japanese. 200410.29) /KEK news [ Japanese Only. SciBar detector in operation! K2K Dat...

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1

K2K Current Status (July 2001)

http://neutrino.kek.jp/news/2001.07.10.News/index-e.html

July 10, 2001. New Results from Neutrino Oscillations Experiment. In a seminars at KEK, the Japanese national particle physics laboratory located in Tsukuba Science City, Ibaraki, Japan, and at several universities in the the USA and Korea, members of the K2K Collaboration described new results from a joint experiment designed to test whether neutrinos have mass. The new results from K2K represent the first significant data on neutrino oscillations using a man-made neutrino beam, whose flavor purity has ...

2

K2K: Long Baseline Neutrino Oscillation Experiment

http://neutrino.kek.jp/news/2002.06.12

Amioka- Long Baseline Neutrino Oscillation Experiment. ニュートリノ振動が起きないとした場合、予想される事象数は80.1 6.2 -5.4 である。 Chonnam National University (Korea). Seoul National University (Korea). University of California, Irvine (USA). University of Hawaii (USA). Massachusetts Institute of Technology. State University of New York, Stony Brook (USA). University of Washington (USA). Soltan Institute for Nuclear Studies (Poland). 高エネルギー加速器研究機構 KEK の12 GeV陽子シンクロトロンによりニュートリノビームを発生させる。 Last modified: Sat Jun 15 12:29:31 JST 2002.

3

K2K FAQ

http://neutrino.kek.jp/k2k_faq.html

Amioka- Long Baseline Neutrino Oscillation Experiment. What is the difference between electron neutrinos, muon neutrinos and tau neutrinos? What are solar neutrinos? What is the solar neutrino puzzle? What are atmospheric neutrinos? What is the atmospheric neutrino puzzle? Why is it important to learn if neutrinos have mass? What are neutrino oscillations? What is a water Cherenkov detector? How do you make a neutrino beam? What is a scintillating fiber (SciFi) tracking detector? What is a muon detector?

4

Neutrino mass was detected.

http://neutrino.kek.jp/news/980604.N98SK

Neutrino mass was detected at Super Kamiokande. The XVIIIth International Conference on Neutrino Physics and Astrophysics. Was held in Takayama near Kamioka, Japan on 4-9 June, 1998. Super Kamiokande is large water Cherenkov detector with 50000 metric tons of ultra-pure water viewed by 11146 20"-PMTs. The detector is located approximately 1000m under ground (2700m water equivalent) in the Mozumi mine, which lies in Kamioka town in Gifu Prefecture. Atmospheric neutrino results from Super-Kamiokande and Ka...

5

T2K Neutrino Experiment at J-PARC

http://neutrino.kek.jp/jhfnu

This page was moved to http:/ jnusrv01.kek.jp/public/t2k.

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Experiments

http://www.nu.to.infn.it/exp

Note: The process can take some time.). Types of Neutrino Experiments. Eutrinoless Double Beta Decay. High-Energy Astrophysical Neutrinos, Supernova Neutrinos. High-Energy Astrophysical Neutrinos, Supernova Neutrinos. Atmospheric and Supernova SN1987A Neutrinos. Accelerator SBL Oscillations, Neutrino Interactions. Accelerator SBL Oscillations, Muon Neutrino - Nucleon Scattering. Accelerator SBL Oscillations, Muon Neutrino - Nucleon Scattering. Double Beta Decay (. Double Beta Decay (. Double Beta Decay (.

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LBL

http://www.nu.to.infn.it/exp/lbl

Note: The process can take some time.). Types of Long-Baseline (LBL) Neutrino Oscillation Experiments. Large bar nu e to bar nu e$. Large nu mu to nu mu$. Large bar nu mu to bar nu mu$. Large nu mu to nu e$. Large bar nu mu to bar nu e$. Large nu mu to nu tau$. Reactor $ bar nu e to bar nu e$ Experiment. Reactor $ bar nu e to bar nu e$ Experiment. Reactor $ bar nu e to bar nu e$ Experiment. Accelerator $ nu mu to nu tau$ and $ nu mu to nu e$ Experiment. Reactor $ bar nu e to bar nu e$ Neutrino Experiment.

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HAP -Presse - Aktuelles - Aktuelles - 2015

http://www.hap-astroteilchen.de/aktuelles-2015.php

Helmholtz Allianz für Astroteilchenphysik. 08122015 - CTA Prototype Telescope Achieves First Light. Left: GCT camera; right: GCT prototype on site the Observatoire de Paris, Meudon, France. On 2015, November 26, a prototype telescope proposed for the Cherenkov Telescope Array. The Gamma-ray Cherenkov Telescope (GCT), recorded CTA’s first ever Cherenkov light. Captured the first optical image in May 2015 with its diagnostic camera. Image of an event captured by the GCT. With the tough weather conditions, ...

hepsrv.hepnet.scphys.kyoto-u.ac.jp hepsrv.hepnet.scphys.kyoto-u.ac.jp

リンク集 | KUHEP

http://hepsrv.hepnet.scphys.kyoto-u.ac.jp/link/index.html

OB • OG. 課題演習A1 • A2. 課題研究P1 • P2. 京都大学理学研究科 物理学第一 第二 宇宙物理学教室. Fermi National Accelerator Laboratory. SPIRES HEP Literature Database. Los Alamos arXiv.org e-Print archive. PhysRev., Phys.Rev.Lett., etc. 606-8502 京都市左京区北白川追分町 京都大学大学院理学研究科 物理学第二教室 高エネルギー物理学研究室. TEL:075-753-3870, FAX:075-753-3795,.

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Adam's Entropy: October 2008

http://adamgetchell.blogspot.com/2008_10_01_archive.html

One particular random walk through life. Sunday, October 05, 2008. Well, the Nobel Prizewinners are to be announced. Tuesday. In the spirit of fun (and to demonstrate how much science really does advance), here are some predictions and other fun facts gleaned from around the 'Net:. Can you predict the Nobel Prizewinners in Chemistry and Physics by counting citations? Http:/ www.symmetrymagazine.org/breaking/2008/08/27/nobel-prize-citations/. Seems to think citations count for potential Nobel prizewinners:.

hap-astroparticle.org hap-astroparticle.org

HAP -Press - News - News - 2015

http://www.hap-astroparticle.org/news-2015.php

Helmholtz Alliance for Astroparticle Physics. 08/12/2015 - CTA Prototype Telescope Achieves First Light. Left: GCT camera; right: GCT prototype on site the Observatoire de Paris, Meudon, France. On 2015, November 26, a prototype telescope proposed for the Cherenkov Telescope Array. The Gamma-ray Cherenkov Telescope (GCT), recorded CTA’s first ever Cherenkov light. Captured the first optical image in May 2015 with its diagnostic camera. Image of an event captured by the GCT. With the tough weather conditi...

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K2K: Long Baseline Neutrino Oscillation Experiment

Amioka- Long Baseline Neutrino Oscillation Experiment. K2K Long-baseline Neutrino Oscillation Experiment. K2K Collaboration, January, 2004. For official information about K2K, or to request a speaker. At a scientific conference, please contact the spokesperson. Final result of K2K oscillation measurement has been published in Physical Review D. Prof Koichiro Nishikawa was awarded the Nishina Memorial Prize. 200511.14) / Japanese. 200410.29) /KEK news [ Japanese Only. SciBar detector in operation! K2K Dat...

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LBNL Neutrino Astrophysics

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