'Neutrino' presentation slideshows

AS Physics Unit 1 1 Matter and Radiation

AS Physics Unit 1 1 Matter and Radiation. Ks5 AS Physics AQA 2450. Mr D Powell. 1. Matter & Radiation p4. 2. Quarks & Leptons p18. 3. Quantum Phenomena p30. 4. Electric Current p46. 5. Direct Current Circuits p58. 6. Alternating Currents p74. 7. Physics Skills / ISA p232.

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Outline

DUSEL Experiment Development and Coordination (DEDC) Internal Design Review July 16-18, 2008 Steve Elliott, Derek Elsworth, Daniela Leitner, Larry Murdoch, Tullis C. Onstott and Hank Sobel. Outline. Introduction - DEDC, who, what, why, when Physics Experiments Science Themes

735 views • 63 slides

Neutrina, co nowego w teorii?

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

744 views • 59 slides

686 views • 53 slides

First Results from BOREXINO and Prospects of Low Energy Neutrino Astronomy

565 views • 42 slides

Neutrino Masses and Mixings

584 views • 41 slides

Neutrino beams: prospects today & synergies with Eurisol

Neutrino beams: prospects today & synergies with Eurisol. V. Palladino Univ & INFN Napoli, Italy coordinator of the BENE NA FP6 Networking Activity Beams for European Neutrino Experiments within the CARE IA

519 views • 38 slides

High Energy Neutrino Astronomy

High Energy Neutrino Astronomy. Status and perspectives of the high energy neutrino observatories. Paolo Piattelli, INFN Laboratori Nazionali del Sud Catania. Layout of the talk. High Energy Neutrino Astronomy Scientific motivations Experimental techniques

532 views • 38 slides

MiniBooNE and SciBooNE experiments, and their cross section analyses

MiniBooNE and SciBooNE experiments, and their cross section analyses. outline 1. Booster Neutrino Beamline (BNB) 2. MiniBooNE detector 3. SciBooNE detector 4 . Conclusion. Teppei Katori Massachusetts Institute of Technology (and Cordao de Ouro Chicago)

427 views • 34 slides

Golden Littlest Seesaw

Golden Littlest Seesaw. Gui -Jun Ding. University of Science and Technology of China. Based on Nucl.Phys . B925 (2017) 470-499, arXiv:1705.05307 , in collaboration with Stephen F. King and Cai -Chang Li.

589 views • 33 slides

Evidence for Formation of K 0 S p Resonance's in (Anti)Neutrino

Evidence for Formation of K 0 S p Resonance's in (Anti)Neutrino Interactions.

381 views • 29 slides

B Meson Decays

B Meson Decays. Kirby Hermansen - Julia Cline. Motivation. We want to measure the ratio of the lifetime of and mesons. . Only a difference of quarks between the two Several other decays present (Julia). Goal.

474 views • 27 slides

Calculation of absolute neutrino masses in the seesaw extension

Calculation of absolute neutrino masses in the seesaw extension. D . J ur ?iukonis , T. Gajdosik and A. Juodagalvis. Vilnius University , Institute of Theoretical Physics and Astronomy. Content. Seesaw mechanism One-loop corrections Case n R = 1 Case n R = 2 Conclusions.

487 views • 24 slides

Imre Bartos Columbia University

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Physics 222 UCSD/225b UCSB

Physics 222 UCSD/225b UCSB. Lecture 4 Weak Interactions (continued) Neutrino scattering Unitarity bound GIM mechanism. Neutrino Electron Scattering. W. W. NC is different, e.g. it couples muon neutrinos to electrons, i.e. across flavor. Z. Historical aside.

342 views • 23 slides

Announcements

Announcements. Homework 13 due today Projects due Friday! Physics seminar today, 1:00 pm, SL 240, on Supernova Remnants!. The Early Universe. 29 November 2006. Today :. History of the early universe Remaining questions and speculations. Summary of Cosmological Facts.

311 views • 19 slides

Hot Relics in GRB Photosphere and GeV Photon Delay

Hot Relics in GRB Photosphere and GeV Photon Delay. Kunihito Ioka (KEK). Contents. Very High Lorentz Factor (VHLF) G max can be up to ~10 6 (> G max, conv ~10 3 ) Internal Shock Synchrotron ? Power-law component over >7 decades

240 views • 17 slides

Can WIMP Spin Dependent Couplings explain DAMA? Limits from DAMA and Other Experiments

274 views • 15 slides

The History of Standard Model

The History of Standard Model. 1. The Nobel Prize winner. 1979 Nobel Prize-- GLASHOW, SALAM and WEINBERG. the theory of the unified weak and electromagnetic interaction. 1984 Nobel Prize-- RUBBIA and VAN DER MEER.

539 views • 13 slides

Neutrinos

282 views • 5 slides