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- W1810367240 abstract "A stream of weakly interacting massive particles (WIMPs) gravitationally scattered outwards within the Earth yields a delay, delta t simeq 60 ns, in good agreement with the results of the OPERA experiment. Conversely, the OPERA experiment may be seen as the unveiling of the first hint of a dark matter particle probed with the photons of the GPS communication signals and using the neutrino beam of the CNGS as a velocity standard. Our analysis yields the true neutrino velocity, V_{nu}, less than the speed of light in vacuum, one finds (V_{nu} - c)/c = - (1.8 pm 0.4) x 10^{-9}. A new experimental test still predicting delta t sim 60 ns instead of delta t sim 600 ns is suggested, based on the use of the long baseline of the order 7 800 km between either the Fermilab neutrino production site and the OPERA detector or the CERN neutrino production site and the MINOS detector." @default.
- W1810367240 created "2016-06-24" @default.
- W1810367240 creator A5088040650 @default.
- W1810367240 date "2012-01-12" @default.
- W1810367240 modified "2023-09-27" @default.
- W1810367240 title "Stream of dark matter as a possible cause of the opera clocks' synchronization signals delay" @default.
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