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Neutrino Oscillations and Beyond Standard Model Physics
Neutrino Oscillations and Beyond Standard Model Physics

The Physics of Particle Detectors
The Physics of Particle Detectors

Colloquium Slides
Colloquium Slides

... • One is the phase in the CKM phase. We have measured it, it is large, and we don’t understand its value. At all. • One is θQCD term (θGG̃). We don’t know its value but it is only constrained to be very small. We don’t know why (there are some good ideas, however). • Three are in the neutrino sector ...
Observation of New-Particle Production by High
Observation of New-Particle Production by High

13. Particle physics
13. Particle physics

Study of the Neutron Detection Efficiency of the CLAS12 Detector
Study of the Neutron Detection Efficiency of the CLAS12 Detector



ppt - UCSC Bayesian Data Analysis Workshop
ppt - UCSC Bayesian Data Analysis Workshop

Study of Neutrino Interactions at the T2K Near Detector Complex
Study of Neutrino Interactions at the T2K Near Detector Complex

Document
Document

ICHEP_2010_Electroweak_Stars
ICHEP_2010_Electroweak_Stars

PHY313 - CEI544 The Mystery of Matter From Quarks to the
PHY313 - CEI544 The Mystery of Matter From Quarks to the

The Integral Payload
The Integral Payload

Muon Lifetime
Muon Lifetime

... • muons are very penetrating particles is some reasonable probability that low energy muons range out • there [stop] in ordinary material from ionization energy loss - stopped µ can replace e in atoms: Bohr rad (r = [αmc] ) is 200 times smaller - µ can be captured by nuclear protons: µ + p -> n + ν ...
Weak interactions and nonconservation of parity
Weak interactions and nonconservation of parity

Plasma_02 - StealthSkater
Plasma_02 - StealthSkater

mc2007_ATLAS_Neil
mc2007_ATLAS_Neil

Lecture 3
Lecture 3

muonlife_tchr_v1.3
muonlife_tchr_v1.3

... In a cosmic ray detector, muon lifetimes are measured by the time for muons stopped in the detector to decay:  A low-energy muon enters a counter, causes an initial scintillation, and stops.  The time t1 of resulting signal is recorded.  After some time, the muon decays into an electron and two n ...
UvA-DARE (Digital Academic Repository)
UvA-DARE (Digital Academic Repository)

Probing the Structure of Matter - Rutgers Physics
Probing the Structure of Matter - Rutgers Physics

Air Cherenkov Methods in Cosmic Rays: A Review
Air Cherenkov Methods in Cosmic Rays: A Review

rutherford scattering
rutherford scattering

... the amplifier gain so that the largest pulses fall somewhat below 10V peak positive amplitude. Because our scintillator is a powder that scatters the scintillation light, the pulse amplitude is not very informative. Set the SCA switches for BIpolar input, INTegral mode so that it passes all amplifie ...
A boost for quantum reality
A boost for quantum reality

Lecture 10 - @let@token Neutrino physics I
Lecture 10 - @let@token Neutrino physics I

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Super-Kamiokande

Super-Kamiokande (full name: Super-Kamioka Neutrino Detection Experiment, abbreviated to Super-K or SK) is a neutrino observatory located under Mount Kamioka near the city of Hida, Gifu Prefecture, Japan. The observatory was designed to search for proton decay, study solar and atmospheric neutrinos, and keep watch for supernovae in the Milky Way Galaxy.
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