'Neutrino flux' presentation slideshows

Neutrino flux - PowerPoint PPT Presentation


Atmospheric Neutrino Anomaly

Atmospheric Neutrino Anomaly

Atmospheric Neutrino Anomaly. By Tasneem Mohsinally. History. Neutrino  - predicted by Pauli (1930’s) to explain Standard Model energy conservation in beta decay - neutral, spin 1/2 - 3 flavours: e   - weak force (short range) W, Z.

By vince
(4 views)

MiniBooNE, a neutrino oscillation experiment at Fermilab

MiniBooNE, a neutrino oscillation experiment at Fermilab

MiniBooNE, a neutrino oscillation experiment at Fermilab. Teppei Katori for the MiniBooNE collaboration Massachusetts Institute of Technology Southern Methodist-U HEP seminar, Dallas, September, 27, 2010. MiniBooNE, a neutrino oscillation experiment at Fermilab. Outline

By justus
(76 views)

Neutrinos from gamma-ray bursts, and tests of the cosmic ray paradigm

Neutrinos from gamma-ray bursts, and tests of the cosmic ray paradigm

Neutrinos from gamma-ray bursts, and tests of the cosmic ray paradigm. GGI seminar Florence, Italy July 2, 2012 Walter Winter Universität Würzburg. TexPoint fonts used in EMF: A A A A A A A A. Contents. Introduction Simulation of sources Neutrinos from gamma-ray bursts

By muncel
(132 views)

The NO n A Experiment Status

The NO n A Experiment Status

The NO n A Experiment Status. Leon Mualem California Institute of Technology (for the NO n A collaboration) Workshop on Next Generation Neutrino and Nucleon Detectors 2007 Hamamatsu, Japan. The NO n A Experiment. Uses a 15kT detector, NO n A Positioned off axis of the Fermilab NuMI beam

By baris
(125 views)

Hanohano

Hanohano

Hanohano. Mikhail Batygov, University of Hawaii. Brookhaven, UDiG workshop, October 17, 2008. Overview of the project goals. Main goals of the project Fundamental physics, esp.  oscillation studies Terrestrial antineutrinos Special advantages Reduced sensitivity to systematics

By osborn
(150 views)

VARIABILITY OF THE SOLAR NEUTRINO FLUX

VARIABILITY OF THE SOLAR NEUTRINO FLUX

VARIABILITY OF THE SOLAR NEUTRINO FLUX. David Caldwell - UC Santa Barbara Jeff Scargle - NASA Ames Research Center Peter Sturrock, Guenther Walther - Stanford University Mike Wheatland - Sydney University. S0306A06. SOLAR NEUTRINO PROBLEM STANDARD INTERPRETATION. Standard Solar Model

By hollis
(83 views)

Paolo Gondolo, Joakim Edsjö , Lars Bergström, Piero Ullio and Edward A. Baltz

Paolo Gondolo, Joakim Edsjö , Lars Bergström, Piero Ullio and Edward A. Baltz

Paolo Gondolo, Joakim Edsjö , Lars Bergström, Piero Ullio and Edward A. Baltz. Introduction. DarkSUSY is a set of Fortran routines for calculations of relic densities and different direct and indirect detection rates in supersymmetric models.

By bryce
(75 views)

Ultra-High Energy Neutrino Fluxes

Ultra-High Energy Neutrino Fluxes

Ultra-High Energy Neutrino Fluxes. Neutrinos: A general connection to cosmic rays Neutrino fluxes in top-down models The Z-burst Summary. HENA workshop Paris June 16-17. G ü nter Sigl GReCO, Institut d’Astrophysique de Paris, CNRS http://www.iap.fr/users/sigl/homepage.html.

By kerri
(94 views)

KM3NeT Status Report

KM3NeT Status Report

KM3NeT Status Report. Uli Katz ANTARES Meeting CERN, 11. December 2003. 1. What happened since last collaboration meeting 2. The FP6 Design Study proposal 3. A review of the KM3NeT talk in Munich. KM3NeT events after September 2003. Amsterdam, 4.-8. October 2003 VLVNT workshop

By cwen
(162 views)

Reactor related

Reactor related

Reactor related. Neutrino flux Location of Reactor and detector Interaction spectrum at a detector  Cross section  Target mass …. How to obtain RENO-specific neutrino flux. 1) 핵분열횟수 Reactor power: 2.73GW th (x 6 reactors)

By dex
(139 views)

Overview

Overview

Overview. Ultra High Energy Cosmic Rays and their connection to neutrinos The GZK Mechanism and the GZK neutrinos The IceCube detector Using IceCube to search for GZK neutrinos. Ultra High Energy Cosmic Rays.

By dava
(103 views)

Potential Neutrino Signals from Galactic  -Ray Sources

Potential Neutrino Signals from Galactic  -Ray Sources

Potential Neutrino Signals from Galactic  -Ray Sources. Alexander Kappes , Christian Stegmann University Erlangen-Nuremberg Felix Aharonian, Jim Hinton MPI für Kernphysik, Heidelberg. Recontres du Vietnam, Particle Astrophysics Hanoi, August 7 – 12, 2006.

By olina
(103 views)

Baryo-through-Leptogenesis and CP violation in neutrino oscillations

Baryo-through-Leptogenesis and CP violation in neutrino oscillations

Baryo-through-Leptogenesis and CP violation in neutrino oscillations. José Bernabéu U. de Valencia and IFIC. MODERN COSMOLOGY INFLATION, CMB and LSS Centro de Ciencias de Benasque, August 2006. Baryo-through-Leptogenesis and CP violation in neutrino oscillations. Baryogenesis

By brandi
(153 views)

Alexandre Kisselev Institute for High Energy Physics Protvino, Russia

Alexandre Kisselev Institute for High Energy Physics Protvino, Russia

Extra dimensions and high energy cosmic neutrinos. Alexandre Kisselev Institute for High Energy Physics Protvino, Russia. Xth International School-Seminar “The Actual Problems o f Microworld Physics ” Belarus, Gomel, July 23 , 200 9. Outlook.

By nara
(87 views)

First Oscillation Results From MiniBooNE

First Oscillation Results From MiniBooNE

First Oscillation Results From MiniBooNE. Martin Tzanov University of Colorado. Outline. Neutrino oscillations. MiniBooNE experiment. Oscillation analysis. First oscillation result. Future. Neutrino Oscillations – Two Flavor. Simple Oscillation Model Two neutrinos

By glenna
(179 views)

G ü nter Sigl Astroparticule et Cosmologie, Université Paris 7

G ü nter Sigl Astroparticule et Cosmologie, Université Paris 7

Gamma-Rays, Cosmic Rays And Neutrinos. Introduction to the observational situation Introduction to the propagation of cosmic rays and electromagnetic cascades Applications to diffuse and point source fluxes of gamma-rays and neutrinos

By oral
(127 views)

Next Generation neutrino detector in the South Pole

Next Generation neutrino detector in the South Pole

AURA. Askaryan Under-Ice Radio Array. Next Generation neutrino detector in the South Pole. Hagar Landsman, University of Wisconsin, Madison. Outline . A skaryan. Askaryan Effect and neutrino detection. U nder ice. Why Ice? Why Radio?. R adio. Radio detection. A rray.

By farrah
(133 views)

Neutrinos and Ultra-High Energy Cosmic Rays

Neutrinos and Ultra-High Energy Cosmic Rays

Neutrinos and Ultra-High Energy Cosmic Rays. Dmitry Semikoz MPI, Munich & INR, Moscow in collaboration with F.Aharonian, O.Kalashev, V.Kuzmin, A.Neronov and G.Sigl. Overview:. Introduction Experimental detection of high energy neutrinos: Under/ground/water/ice Horizontal air showers

By tayte
(160 views)

EPS 2003, Aachen Particle Astrophysics (cosmic rays)

EPS 2003, Aachen Particle Astrophysics (cosmic rays)

EPS 2003, Aachen Particle Astrophysics (cosmic rays). Comparison of high-energy galactic and atmospheric tau neutrino flux. By G.-L. Lin. National Chiao-Tung U. Taiwan. glin@cc.nctu.edu.tw. Outline. Motivation The Intrinsic and Oscillated Tau Neutrino Fluxes

By roger
(122 views)

Imaging the High-Energy Neutrino Universe from the South Pole

Imaging the High-Energy Neutrino Universe from the South Pole

Imaging the High-Energy Neutrino Universe from the South Pole. Results from AMANDA and Status of IceCube. Kurt Woschnagg University of California - Berkeley. Les Rencontres de Physique de la Vall é e d’Aoste La Thuile, Feb 27 – Mar 5, 2005 Results and Perspectives in Particle Physics.

By lobo
(90 views)

View Neutrino flux PowerPoint (PPT) presentations online in SlideServe. SlideServe has a very huge collection of Neutrino flux PowerPoint presentations. You can view or download Neutrino flux presentations for your school assignment or business presentation. Browse for the presentations on every topic that you want.