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October 24, 2011 Bob Zwaska - Fermilab Intensity Frontier – Neutrino Working Group Meeting 3

WIMPS & Neutrinos

First measurement of pp neutrinos in real time in the Borexino …borex.lngs.infn.it/Thesis/P.Mosteiro_PhD_Thesis.pdf · 2016-10-19 · Chapter 1 Solar Neutrinos 1.1 Neutrinos Neutrinos

Dirac Materials QDM Mar 2015 short - Los Alamos National ... · The Dirac Equation P. Dirac: “The quantum theory of the electron” (1928) Describing electrons, protons, quarks,neutrinos

Hunting neutrinos

Main Sequence Stars Internal structure Nuclear fusion Protons, neutrons, electrons, neutrinos Fusion reactions Lifetime of the Sun Transport of energy

Target R & D Bob Zwaska LBNE Collaboration Meeting January 28, 2010

Atoms / Elements Different number of protons Protons found in nucleus # of protons = atomic number Since atom is electrically neutral: #protons = # electrons

Accelerator upgrades for NuMI Robert Zwaska Fermilab August 6, 2006 NBI 2006

LBNE Target Hall Instrumentation Bob Zwaska January 27, 2010

The Electron Cloud And Secondary Electron Yield Tom Schmit Mentor: Bob Zwaska

Mass # atomic # protons + neutrons = protons = Atomic Symbols

Neutrinos & the MINOS Experimentminos/seminaria/Seminarium_dyplomowe-MINOS2.pdf\2.5x1013 protons/pulse. Krzysztof W. Fornalski 12 Producing the neutrino beam - the scheme Proton beam

Number of Protons = Number of Electrons Number of Protons = Atomic Number Atomic Mass = Protons + Neutrons

Proton Improvement Plan Bob Zwaska August 3, 2015 All-Experimenters Meeting

Electron Cloud Results from ILCDR08 Bob Zwaska ECWG Meeting July 22, 2008

Superluminal neutrinos?

STERILE NEUTRINOS

Atmospheric Neutrinos

Electron Cloud Measurements and Plans at Fermilab · 2010. 10. 13. · Driving Protons at the Main Injector • Main Injector today produces 120 GeV proton beams for neutrinos and

LBNE Target Hall Instrumentation Bob Zwaska January 27, 2010

The Sun Internal structure of the Sun Nuclear fusion –Protons, neutrons, electrons, neutrinos –Fusion reactions –Lifetime of the Sun Transport of energy

Fermi National Accelerator Laboratory July 2020 PIP-II ...PIP-II Particle Accelerator Abundant neutrinos, powerful protons The PIP-II project is an essential upgrade of Fermilab’s

Neutrino-Astronomieparticle.astro.ru.nl/hs0607/V-Renz.pdf · -Neutrino-Oszillationen • Neutrinos bei mittleren Energien-Supernova-Neutrinos-Atmosphärische Neutrinos / Super-Kamiokande

Protons Identify an Element/atom (2 protons = Helium)

The Sun: Part 3 and Measuring the Stars: Part 1. Net result: 4 protons → 4 He + 2 neutrinos + energy Hydrostatic Equilibrium: pressure from fusion reactions

Supernova pointing with low- and high-energy neutrino ... · outburst of TeV neutrinos is expected due to pion production by protons accelerated in the SN shock @9#. This neutrino

Neutrinos TGIF.pdf

Neutrinos as Probes: Solar-, Geo-, Supernova neutrinos; Laguna

Supernova Neutrinos

Les oscillations de neutrinos Le faisceau de neutrinos CNGS

LHC – New era ? Large Hadron Collider (protons + protons)

The Particle Zoo. Too Many Particles Far from just finding Protons Neutrons Electrons Neutrinos and their antiparticles, during the 20 th century many

Atmosphärische Neutrinos

Particles and Cosmic Rays - University of Birmingham · 2017. 8. 3. · Primary high energy cosmic ray in upper atmosphere : 85% protons 12% alpha particles 2% electrons Neutrinos,