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What does a spark chamber detect?
What does a spark chamber detect?

Flipped SU(5) - cosmology - Arizona State University
Flipped SU(5) - cosmology - Arizona State University

The CMS Fast Simulation
The CMS Fast Simulation

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Radon – Quick Facts - Take Action On Radon

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Search for Scalar Top Quark Partners and Parton Shower Tuning in

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The Family Problem: Extension of Standard Model with a

... -\bar{\nu}_\mu(u_{+} + \epsilon u_-)\nu_e , is off-diagonal, in the form similar to the Zee matrix[5], and can easily be fitted to the observed data[2]. (And i is needed to make it hermitian.) In other words, the “source” of the neutrino masses comes from the family Higgs and is different from those ...
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Document

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CMS Ecal Laser Monitoring System

... Higgs bosons can also be used as a probe of new physics. A search for chargino and neutralino associated production looks for Higgs coming from sparticle decays, followed by a decay to b-quarks. ...
The Standard Model and its Simple Extensions
The Standard Model and its Simple Extensions

... Experimental tests of electroweak interactions Gauge sector fully determined by three parameters: g, g 0, v (In practise the three best measured parameters are used: α(0), GF, mZ) Can test the model if more than three observables are measured Expect one-loop correction to be of order α ∼ 1% ➟ have ...
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Simulation study of optical degradation monitoring in the SNO+

Radioactivity
Radioactivity

... The electron in beta decay is not an orbital electron; it is created in the decay. The fundamental process is a neutron decaying to a proton, electron, and neutrino: ...
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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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