'Neutral current' presentation slideshows

Presentation on Transmission Rings in Jaipur SSA

Presentation on Transmission Rings in Jaipur SSA. Network Elements of Jaipur SSA. Exchanges + RSUs + DLCs(Urban) 3 + 58 + 12 Exchanges Rural 143 TAX (L1 ) 03 GSM GMSC 01 GMSC/MSS 05

957 views • 94 slides

MiniBooNE and n Oscillations

D m 2. Sin 2 2 q m e. MiniBooNE and n Oscillations. Magnetic Focussing Horn. Neutrino Event Display. Inside View of Detector. Sensitivity to Oscillations. Outline. A short course in the physics of n oscillations What are neutrinos? Oscillations? n oscillation landscape

852 views • 84 slides

The Neutrino Story

The Neutrino Story. What We Think It Tells Us and Why We May Be Wrong C.P. Burgess. Outline. The Most Feebly-Interacting Observed Particles Why are they observed at all? Basic Neutrino Properties How many types are there? How massive are they? Do they decay?

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763 views • 58 slides

Recent Developments in Beauty and Charm Physics

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weak interactions

weak interactions. weak decays beta decay of neutron. e. p. n. neutrino. direct interaction of four fermions ? Enrico Fermi, ~1936. Enrico Fermil. 1964 ===>. gauge theory. electroweak. 1957. weak bosons. W. J. Schwinger. -. 1964 - 1968 gauge theory of the

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461 views • 37 slides

Thoughts about tagged neutrino beam, GELATRINO proposal at LHC

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Balanced poly phase circuits

509 views • 33 slides

NDM09, Madison, Wisconsin Sept. 2, 2009

Neutrino-Induced Reactions on Fe and Ni Isotopes and Nucleosynthesis in Stars Toshio Suzuki Nihon University. NDM09, Madison, Wisconsin Sept. 2, 2009. New evaluation of reaction rates in fp-shell and light (p-shell) nuclei ? New shell model Hamiltonians

442 views • 32 slides

HEP Experiment at Penn

HEP Experiment at Penn. Joseph Kroll for the Penn High Energy Group. Enquiring Minds Want to Know. What are the fundamental Constituents of matter?. What are the forces (interactions) that govern their behavior?. Overview of Penn HEP. Current Experiments:

416 views • 30 slides

1+1+1 = 4 ?* * (for larger values of 1) Masses, Mixings, and Sterile Neutrinos

1+1+1 = 4 ?* * (for larger values of 1) Masses, Mixings, and Sterile Neutrinos. Joseph A. Formaggio University of Washington. (My) Skill Level. ...Theory. ...Experiment. Our understanding of neutrinos has changed in light of new evidence:

366 views • 28 slides

Some Nuclear Physics with Solar Neutrinos

421 views • 26 slides

Disturbances due to high frequency signals (above 2 kHz)

Disturbances due to high frequency signals (above 2 kHz). Martin Lundmark EMC on Site martin.lundmark@ltu.se. OUTLINE. BACKGROUND CONDUCTIVE AND RADIATED EMISSION IN A THREE-PHASE GRID ORIGIN OF CONDUCTIVE HIGH-FREQUENCY LEAKAGE CURRENT MEASUREMENTS CONCLUSION. BACKGROUND

343 views • 23 slides

Tests of non-standard neutrino interactions (NSI)

Tests of non-standard neutrino interactions (NSI). Cecilia Lunardini Institute for Nuclear Theory University of Washington, Seattle. Menu. N on S tandard neutrino-matter I nteractions Accelerator limits Neutrino oscillation sensitivity NSI effects on solar neutrinos

382 views • 22 slides

Neutral Current Analysis in MINOS

Neutral Current Analysis in MINOS. Alexandre Sousa University of Oxford Harvard University* DOE Review of the Harvard HEP Group August 15, 2008. *After December 01, 2008. Neutrino Interactions in MINOS.

285 views • 21 slides

Chapter 3

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Studies of Proton Structure at HERA

New results on. Studies of Proton Structure at HERA. I. Tsurin. on behalf of ZEUS and H1. Neutral current (NC) Charged current (CC) Structure functions F 2 , xF 3 , F L Parton distribution functions (PDF) The strong coupling constant ? S. 12 th International QCD Conference.

254 views • 13 slides

V. Electroweak Precision Observables

V. Electroweak Precision Observables. What radiative corrections can teach us Basic formalism. g. g. Weak Decays: G F encodes information on the spectrum via radiative corrections. Muon Decay. D r m depends on parameters of particles inside loops. g. g.

232 views • 10 slides