'Electron neutrino' presentation slideshows

Neutrino Masses, Double Beta Decay and Nuclear Structure

970 views • 84 slides

Precision Measurements after the Higgs Discovery

738 views • 62 slides

Solar Neutrino Physics

Solar Neutrino Physics. Aksel Hallin PIC 2010 University of Alberta. Solar Neutrino Physics. Neutrino Physics (the sun is a very intense and quite well understood source of neutrinos) Neutrino Oscillations Non standard neutrino interactions

962 views • 60 slides

Neutrino Masses and Mixings

584 views • 41 slides

NEUTRINO PHYSICS AND COSMOLOGY

NEUTRINO PHYSICS AND COSMOLOGY. n e n m n t. STEEN HANNESTAD, Aarhus University BLOIS, 31 MAY 2012. FLAVOUR STATES. PROPAGATION STATES. MIXING MATRIX (UNITARY). LATE-TIME COSMOLOGY IS (ALMOST) INSENSITIVE TO THE MIXING STRUCTURE.

502 views • 38 slides

KATRIN - The Ka rlsruhe Tri tium N eutrino Experiment

465 views • 35 slides

THE NUCLEUS OF THE ATOM

THE NUCLEUS OF THE ATOM. Potential Energy of any Body of Mass. The Proton. Rest Mass =1.007276466812awu Average Lifetime years Discovered, described, and named by Ernest Rutherford over a three-year period (1917-1920). James Chadwick. Student of Rutherford

433 views • 32 slides

Tracking Cosmic Ray Muons Using a Cloud Chamber

Tracking Cosmic Ray Muons Using a Cloud Chamber. Leah Wilson and Lori Wilson duPont Manual High School and Dr. Akhtar Mahmood Bellarmine University. KAPT 2009 SPRING MEETING MARCH 7, 2009 BELLARMINE UNIVERSITY. Purpose and Hypothesis.

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Announcements

370 views • 27 slides

PARTICLE PHYSICS

459 views • 24 slides

Option J: Particle physics J5 Evidence for quark and standard model

J.5.1 State what is meant by deep inelastic scattering. J.5.2 Analyze the results of deep inelastic scattering. J.5.3 Describe what is meant by asymptotic freedom. J.5.4 Describe what is meant by neutral current.

358 views • 22 slides

354 views • 20 slides

Revisiting NuTeV -or- What Kevin Did Last Week

327 views • 19 slides

280 views • 19 slides

Great Observatories

Fermi Gamma ray Space Telescope (2008). Large Area Telescope. Gammas hit thin metal sheets, converting to electron-positron pairs via PP.

329 views • 17 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.

540 views • 13 slides

Chapters 9, 11, 12

Chapters 9, 11, 12. Concepts covered that will also be candidates for exam questions. Ionic bonds and different components of energy: ionization E, repulsion E, coulomb attraction E, disassociation E

254 views • 13 slides

Another Muon Neutrino (simulated)

175 views • 6 slides

LEPTONS

757 views • 6 slides

High Energy Physics Briefing to the Astronomy and Astrophysics Advisory Committee

High Energy Physics Briefing to the Astronomy and Astrophysics Advisory Committee. Dr. Robin Staffin Associate Director, Office of High Energy Physics DOE Office of Science February 8, 2007. The DOE HEP program in FY 2008. Overall HEP budget and priorities in FY 2008:

133 views • 4 slides