Stream of dark matter as a possible cause of the opera clocks' synchronization signals delay
| Autor: | Mbelek, Jean Paul |
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| Rok vydání: | 2012 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| Popis: | 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. Comment: 5 pages, no figure |
| Databáze: | arXiv |
| Externí odkaz: |
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