'Neutrino mass' diaporamas de présentation

30, 511, 1200 keV e- track reconstruction from a 1kg, 10bar Xe -TMA TPC with microbulk readout

30, 511, 1200 keV e- track reconstruction from a 1kg, 10bar Xe -TMA TPC with microbulk readout. Diego Gonzalez Diaz (diegogon@unizar.es) for the NEXT collaboration. 16/06/2014. Index. Short overview of NEXT. The Micromegas-TPC (NEXT-MM).

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Neutrina, co nowego w teorii?

Neutrina, co nowego w teorii?. Marek Zra?ek Instytut Fizyki Uniwersytetu ?l?skiego. Streszczenie.

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Andrew J. Lankford University of California, Irvine

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Cosmological Constraints on Active and Sterile Neutrinos Matteo Viel INAF / OATS & INFN/TS

Cosmological Constraints on Active and Sterile Neutrinos Matteo Viel INAF / OATS & INFN/TS From Majorana to LHC: Workshop on the Origin of Neutrino Mass ICTP-Trieste 2 nd October 2013. OUTLINE . THEORY: Effect of massive neutrinos and warm dark matter on the LSS/SSS

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neutrino mass

neutrino mass. a long wait for a little weight. Stuart Freedman memorial symposium Berkeley, Jan 11, 2014. Hamish Robertson, University of Washington. Neutrinos oscillate, have mass. SNO. KamLAND. Super- Kamiokande. What is the neutrino mass scale?.

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Probing Majorana Neutrinos ( in Rare Decays of Mesons)

Probing Majorana Neutrinos ( in Rare Decays of Mesons). arXiv:1005.4282 (PRD82,053010,2010) G. Cvetic, C. Dib, S.K. Kang, C.S. Kim. 11/17/2011 - DBD11 C. S. Kim. Outline. 1. Prologue 2. Issues on neutrino masses 3. Probing Majorana neutrinos via (a) 0 nbb

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Strasbourg , 11 July 200 6 Julien Lesgourgues (LAPTH , Annecy )

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Tsutomu T. TAKEUCHI Division of Particle and Astrophysical Science, Nagoya University, JAPAN with

Formation and Evolution of Galaxies: Point of View of H I Cosmology. Tsutomu T. TAKEUCHI Division of Particle and Astrophysical Science, Nagoya University, JAPAN with SKA-Japan high- z galaxy and cosmology WG. East-Asian SKA WS, 30 Nov .-2 Dec., 2011, KASI, Daejeon , Korea. Contents.

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??????? ??. ???????????????. ?????? ?????? 2012.10.18. ????. ????? ???????? ???????????? ??. ? . ?????. some problems in the hot Big Bang model ? flatness problem , horizon problem , relic density problem. slow-roll inflation. criterions: cosmic acceleration e-folding number

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Phenomenological Aspects of SUSY B-L Extension of the SM

Phenomenological Aspects of SUSY B-L Extension of the SM. Shaaban Khalil. Centre for Theoretical Physics British University in Egypt. Outline. TeV scale B-L : Minimal bottom-up extension of the SM B-L signatures at LHC Supersymmetric B-L B-L Right-handed (s)neutrino

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Probing Majorana Neutrinos in Rare Meson Decays

Probing Majorana Neutrinos in Rare Meson Decays. Claudio Dib UTFSM I.S. & B.K. Fest, UTFSM, May 2010. G. Cvetic, C.D., S.K. Kang, C.S. Kim, PRD 82, 053010, 2010 . Outline. 1. Recent history 2. Issues on neutrino masses 3. Probing Majorana neutrinos via (a) 0 nbb

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Renormalization in the Higgs triplet model

Renormalization in the Higgs triplet model . Mariko Kikuchi (Univ. of Toyama). Collaborators: Mayumi Aoki, Shinya Kanemura , Kei Y agyu. M . Aoki, S. Kanemura , M. Kikuchi, K. Yagyu , PLB 714, 279 ( 2012). Workshop on Multi-Higgs Models , 31. August, 2012, Lisbon. C ontents.

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The Solar Neutrino Problem

The Solar Neutrino Problem. Barbara Sylwester Zak?ad Fizyki S?o?ca CBK PAN. One page story - the short story.

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Cosmic Gall

Cosmic Gall.

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Nonzero and Neutrino Masses from Modified Tribimaximal Neutrino Mixing Matrix

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Search for the Cosmic Neutrino Background and the Nuclear Beta Decay .

Search for the Cosmic Neutrino Background and the Nuclear Beta Decay . Amand Faessler University of Tuebingen Germany. Publication : Amand F aessler, Rastislav Hodak , Sergey Kovalenko , Fedor Simkovic: arXiv : 1304.5632 [ nucl-th ] 20. April 2013. .

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Particle Physics Cosmology

Neutrino Mass Measurements. Particle Physics Cosmology. What is the neutrino mass scale?. Hamish Robertson, ESPP12, Kracow , Sept. 11, 2012 . Y.Y.Y. Wong. Y.Y.Y. Wong. Neutrino mass from Beta Spectra. With flavor mixing :. mixing. neutrino masses. from oscillations.

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NO?A Event Building, Buffering & Filtering From within the DAQ System

NO?A Event Building, Buffering & Filtering From within the DAQ System . 11520 FEBs (368,4600 det. channels). FEB. FEB. FEB. FEB. FEB. FEB. 11,160 Front End Boards. 5ms data blocks. FEB. FEB. FEB. FEB. DCM 1. FEB. FEB. Data Buffer. Far Det. FEB. FEB.

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