'Dark matter search' diaporamas de présentation

Wojtek Skulski University of Rochester

The Universe and the FPGA Digital Pulse Processing for Dark Matter Search. Wojtek Skulski University of Rochester. Contributors. Wojtek Skulski (University of Rochester and SkuTek Instrumentation). Frank Wolfs (University of Rochester). Eryk Druszkiewicz (University of Rochester).

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Indirect Dark Matter Search with AMS-02

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Highlight results from the MAGIC telescopes

Highlight results from the MAGIC telescopes. Elisa Prandini * Padova University & INFN From neutrino to multimessenger astronomy : status and perspectives Marseilles 4 th April 2011. *Mail to: prandini@pd.infn.it. Outline. MAGIC: a low energy threshold IACT Recent results Galactic

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Lepton - Photon 01 Francis Halzen

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AMS as an Astroparticle Physics Experiment

AMS as an Astroparticle Physics Experiment. ? 4 ? ?????? ???? 6 ? 19 ? ( ? ) ? ??. Astroparticl Physics is Connecting Quarks with the Cosmos. Neutron. Proton. Periodic System of Elementary Particles. What Powered the Big Bang?. Inflation (Big Bang plus 10 -34 Seconds).

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High Energy Gamma Ray Group

High Energy Gamma Ray Group. Observing Galactic Center & Dark Matter Search. MAGIC Team Ryoma Murata (UT B3) Hiroki Sukeno (UT B3) Tomohiro Inada (Kobe Univ. B3 ) Fermi Team Yuta Sato (TUS B4) Taketo Mimura ( Waseda Univ. B3) Masahiko Yamada (UT B3 ). a. Introduction.

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Fermi ????????????????

Fermi ????????????????. Apr. 4, 2013@Tokyo (2 nd Workshop on Particle Physics of the Dark Universe) T. Mizuno ( ????????????? ) On behalf of the Fermi-LAT collaboration. Dark Matter Search with Fermi Large Area Telescope. Apr. 4, 2013@Tokyo

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XMASS ?????? ??????

XMASS ?????? ??????. ??????????? 2011 ? 3 ? 7 ? ??????????????? 2011. Contents. Introduction The XMASS detector Current status of XMASS. Introduction. Solar neutrino. XMASS experiment. What is XMASS? Multi purpose low-background and low-energy threshold experiment with liquid Xenon.

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KIMS : Dark Matter Search Experiment in Korea

KIMS : Dark Matter Search Experiment in Korea. Jik Lee Seoul National University For the KIMS Collaboration. DSU2006, Madrid. KIMS. Korea Invisible Mass Search. H.C.Bhang, J.H.Choi, S.C.Kim, S.K.Kim, S.Y.Kim, J.W.Kwak, J.H.Lee H.S.Lee, S.E.Lee, J. Lee, S.S.Myung, H.Y.Yang

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Tatsuhiro NAKA KMI / IAR, Nagoya University

Tatsuhiro NAKA KMI / IAR, Nagoya University . Nuclear Emulsion Technology and Directional Dark Matter Study. KMI2013 @ Nagoya University, Dec. 12 th (11-13), 2013 . OPERA detector . Emulsion mass ~ 30 ton. Why is it capable of detection of tau neutrino ? .

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Neutrinoless Double Beta Decay Experiments

Lucifer. made in the frame of LUCIFER experiment FP7/2007-2013 ERC grant agreement n. 247115. XXIV SEMINARIO NAZIONALE di FISICA NUCLEARE E SUBNUCLEARE OTRANTO, Serra degli Alimini, 21-27 Settembre 2012 Argomento : Studio del decadimento doppio beta ai LNGS

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The Status of KIMS (Korea Invisible Mass Search)

Yeongduk Kim Sejong University. The Status of KIMS (Korea Invisible Mass Search). ICHEP 2012 , Melbourne . 2012. 7. 6. Yangyang (Y2L) Underground Laboratory. (Upper Dam). Korea Middleland Power Co. Yangyang Pumped Storage Power Plant. Y2L. Seoul. (Power Plant). RENO.

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K.L. Giboni, X. Ji, H. Lin, Y. Zhang, and L. Zhao Shanghai Jiao Tong University

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Status of PandaX II

Status of PandaX II. Karl Ludwig Giboni on behalf of the PandaX collaboration Shanghai Jiao Tong University. TPC Conference, Paris 5 -7 December, 2016. The PandaX Collaboration. Shanghai Jiao Tong University, SJTU (2009~ )

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