Lowering the Light Speed Isotropy Limit : European Synchrotron Radiation Facility Measurements

نویسندگان

  • V. G. Gurzadyan
  • A. Kashin
  • A. Margarian
  • O. Bartalini
  • V. Bellini
  • A. D ’ Angelo
  • J. - P. Didelez
  • A. Fantini
  • G. Gervino
  • F. Ghio
  • B. Girolami
  • A. Giusa
  • M. Guidal
  • E. Hourany
  • S. Knyazyan
  • V. Kouznetsov
  • R. Kunne
  • A. Lapik
  • P. Levi Sandri
  • A. Lleres
  • S. Mehrabyan
  • D. Moricciani
  • V. Nedorezov
  • C. Perrin
  • D. Rebreyend
  • G. Russo
  • N. Rudnev
  • C. Schaerf
  • M. - C. Sutera
  • A. Turinge
چکیده

— The measurement of the Compton edge of the scattered electrons in GRAAL facility in European Synchrotron Radiation Facility (ESRF) in Grenoble with respect to the Cosmic Microwave Background dipole reveals up to 10σ variations larger than the statistical errors. We now show that the variations are not due to the frequency variations of the accelerator. The nature of Compton edge variations remains unclear, thus outlining the imperative of dedicated studies. The inverse Compton scattered electron energy spectrum, as suggested in [1], provides a way to study the light speed anisotropy within the energy scales and monochromaticity reachable in existing synchrotrons. The study of such anisotropy vs the frame, when the dipole of the Cosmic Microwave Background (CMB) radiation is vanishing i.e. with respect to the apex of the CMB dipole, is of particular interest. It is due to the 'absolute' content of the CMB frame within the hierarchy of the motions of the Earth, of the Sun c Società Italiana di Fisica

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تاریخ انتشار 2008