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SUMMARY:“Search for sub-microsecond bursts of Cherenkov radio emission c
 aused  by the interaction of high-energy neutrinos with lunar regolith”
DTSTART;VALUE=DATE-TIME:20241022T140500Z
DTEND;VALUE=DATE-TIME:20241022T160000Z
DTSTAMP;VALUE=DATE-TIME:20260718T032733Z
UID:indico-contribution-4107@cern.ch
DESCRIPTION:Speakers: Sergei Shavkovich (PUShGU)\nG.A. Askaryan had shown 
 in 1960s [1\,2] that the interaction of high-energy particles with the rat
 her dense dielectric medium should form the negative charged cascades  mov
 ing with superluminal velocity in the medium.  This Askaryan’s effect is
  laid on the basis of the radio-astronomical method for detecting ultra-hi
 gh-energy neutrinos\, proposed later by R.D.Dagkesamansky and I.M. Zhelezn
 ykh [3].  This report provides a brief overview of the application of this
  radio astronomy method to search for Cherenkov radio bursts from the Moon
 .  Some results of the search for such radio bursts on the meter wave radi
 o telescope BSA FIAN are presented.\n\nhttps://indico.particle.mephi.ru/ev
 ent/436/contributions/4107/
LOCATION: Alexeevskiy hall
URL:https://indico.particle.mephi.ru/event/436/contributions/4107/
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