'Cherenkov radiation' presentation slideshows

Air Cherenkov Methods in Cosmic Rays: A Review and Some History

Air Cherenkov Methods in Cosmic Rays: A Review and Some History. A.S. Lidvansky, Institute for Nuclear Research, Moscow. The Vavilov-Cherenkov radiation of high energy cosmic rays in air:.

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Cherenkov Radiation and RICH Detectors

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Neutrino Physics

Neutrino Physics. Neutrino mass and mixing No neutrinoless double beta decay. Nishikawa ? XXXIV International Meeting on Fundamental Physics April 3-7,2006. Neutrinos are Everywhere. Big Bang: They are still left over: ~300 neutrinos per cm 3 Natural sources

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Denumirea Proiectului: CERCETARI EXPLORATORII IN FIZICA

Denumirea Proiectului: CERCETARI EXPLORATORII IN FIZICA DEZINTEGRARILOR EXOTICE NUCLEARE SI SUBNUCLEARE DE TIP SUPER-CERENKOV. Director de Proiect Prof. Dr. Dumitru B. ION. ID-52-283/2007. Obiectivele Proiectului.

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PANDA Detector and Recent Development on DIRC & SiPM Bidyut Roy NPD, BARC, Mumbai

PANDA Detector and Recent Development on DIRC & SiPM Bidyut Roy NPD, BARC, Mumbai. An overview of FAIR accelerator Complex Over view of the PANDA detector Indian interest: Luminosity monitor and

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Radio Detection

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A Very High Momentum Particle Identification Detector for the ALICE experiment at the LHC.

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SUPER -KAMIOKANDE

SUPER -KAMIOKANDE. Kamiokande = Kamioka Nucleon Decay Experiment. Topics of Discussion. Detector Super-Kamiokande Solar neutrinos Results. Properties of Super-K. A Large Water Cherenkov Detector for Cosmic Particles Size: Cylinder of 41.4m (Height) x 39,9m (Diameter)

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Refraction of Light

Refraction of Light. Done by: Stephen Chow 3P304. Agenda. 5 technologies of Refraction Of Light Cherenkov Radiation Binoculars AIST innovations: Flat-Plate Lens Princeton Novel Semiconductor Structure Spectacles. Cherenkov Radiation. Cherenkov Radiation.

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Lecture 2.3: Wire-based Detectors

Lecture 2.3: Wire-based Detectors. Geiger-Muller Counter. 1928. Tube filled with a low pressure inert gas and an organic vapor or halogen and contains electrodes between which there is a voltage of several hundred volts but no current. Anode is a wire passing through it. Cathode is the walls.

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Solar Neutrinos and Earth Structures

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Feasibility of X-ray Cherenkov Diffraction radiation for beam diagnostics of linear accelerators

Feasibility of X-ray Cherenkov Diffraction radiation for beam diagnostics of linear accelerators. A.S. Konkov , A.P. Potylitsyn , A.S. Gogolev , Tomsk Polytechnic University P.V. Karataev , JAI at Royal Holloway, University of London. R ( t ). O. z ( t ). Introduction.

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Miscellaneous Topics

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Interactions of Electrons

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The Babar Cherenkov Detector D etection of I nternally R eflected C herenkov

The Babar Cherenkov Detector D etection of I nternally R eflected C herenkov. Yuen-Jung Chang. Cherenkov radiation. Charge particle passes through an insulator at a constant speed greater than the speed of light in that medium.

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Neutrino detectors

Neutrino detectors. Basic features: 1) Very small cross-sections of interactions ? very big volumes of detectors 2) Very effective shielding ? underground detectors, underwater,

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Cherenkov Radiation in Time Domain

Cherenkov Radiation in Time Domain. 2010.05.15 Chia -Yu, Hu. Cherenkov Pulse in Time Domain. Based on Alvarez-Muniz, arXiv : 1002.3873 Begin with Maxwell equations: Introducing potentials:. Transverse Gauge. Choosing transverse gauge (Coulomb gauge):

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Overview of Lectures (I)

Overview of Lectures (I). Introduction Fri. Week 1, Lindemann (L) Why do we study Nuclear Physics What will this course cover Shape and density of the nuclei 2. The Semi Empirical Mass Formula (SEMF) Thu. Week 2, Martin Wood (MW) The liquid drop model The Fermi Gas Model

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1998: Discovery that Neutrinos H ave S mall Mass

What is a Neutrino?. Detection of Neutrinos and the Super Kamiokande detector. Neutrino Oscillation and Mass. T . A neutrino is a subatomic particle with no charge. There are three flavors:

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