Category Archives: Muons

G-2 Experiment

Posted on October 11, 2012 by PlatoHagel

See: Muon Dialogos of Eide

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The Bolshoi simulation

Posted on July 6, 2012 by PlatoHagel

A virtual world?  The more complex the data base the more accurate one’s simulation is achieved. The point is though that you have to capture scientific processes through calorimeter examinations just as you do in the LHC. So these backdrops … Continue reading →

Posted in Calorimeters, Fermi, Muons, SNO, SuperKamiokande, Tscan, Virtual Reality, Xenon | Tagged , , , , , , , , | Leave a comment

first tau-neutrino “appearing” out of several billion of billions muon neutrinos

Posted on November 22, 2011 by PlatoHagel

Layout of the CNGS beam line. The OPERA neutrino experiment [1] at the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in direct appearance mode in the νμ→ντ channel, the signature being the … Continue reading →

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Energy Boost From Shock Front

Posted on November 20, 2011 by PlatoHagel

Main Components of CNGS A 400 GeV/c proton beam is extracted from the SPS in 10.5 microsecond short pulses of 2.4×1013 protons per pulse. The proton beam is transported through the transfer line TT41 to the CNGS target T40. The … Continue reading →

Posted in Faster Than Light, General Relativity, Gran Sasso, Hulse, Muons, Relativistic Muons, Taylor | Tagged , , , , , , | Leave a comment

Seeing Underlying Structures

Posted on October 12, 2011 by PlatoHagel

 There is  gap between,  “Proton Collision ->Decay to Muons and Muon Neutrinos ->Tau Neutrino ->[gap] tau lepton may travel some tens of microns before decaying back into neutrino and charged tracks.” Use the case of Relativistic Muons?  An analysis of … Continue reading →

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Cohen-Glashow Argument

Posted on October 7, 2011 by PlatoHagel

Bee:And for all I know you need a charge for Cherenkov radiation and neutrinos don’t have one. Fig. 1: Cerenkov radiation involves the nearly continuous emission of photons by a charged particle moving faster than the speed of light in … Continue reading →

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Proton Collision ->Decay to Muons and Muon Neutrinos ->Tau Neutrino ->

Posted on October 5, 2011 by PlatoHagel

…..tau lepton may travel some tens of microns before decaying back into neutrino and charged tracks  Before I comment on the result, let me give you a little background on the whole thing. Opera is a very innovative concept in … Continue reading →

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Cherenkov radiation

Posted on October 4, 2011 by PlatoHagel

Taking the formalisms of electromagnetic radiation and supposing a tachyon had an electric charge—as there is no reason to suppose a priori that tachyons must be either neutral or charged—then a charged tachyon must lose energy as Cherenkov radiation[15]—just as … Continue reading →

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P.I. Chats: Faster-than-light neutrinos?

Posted on October 4, 2011 by PlatoHagel

Measurements by GPS confirm that the neutrinos identified by the Super-Kamiokande detector were indeed produced on the east coast of Japan. The physicists therefore estimate that the results obtained point to a 99.3% probability that electron neutrino appearance was detected.Neutrino … Continue reading →

Posted in Cerenkov Radiation, Faster Than Light, Gran Sasso, Muons, Neutrinos, Opera, Relativistic Muons, Sterile Neutrinos | Tagged , , , , , , , | Leave a comment

Measurement of the neutrino velocity with the OPERA detector

Posted on September 23, 2011 by PlatoHagel

Scanning results tau decays New results from OPERA on neutrino propertieslive from Main Amphitheatre. “This result comes as a complete surprise,” said OPERA spokesperson, Antonio Ereditato of the University of Bern. “After many months of studies and cross checks we … Continue reading →

Posted in Calorimeters, Cdms, Cerenkov Radiation, Faster Than Light, Gran Sasso, Muons, Neutrinos, Opera, Relativistic Muons | Tagged , , , , , , , , | 8 Comments