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SUMMARY:Analytical approximation of neutrino distribution function in core
 -collapse supernova
DTSTART;VALUE=DATE-TIME:20201005T164500Z
DTEND;VALUE=DATE-TIME:20201005T170000Z
DTSTAMP;VALUE=DATE-TIME:20260515T142107Z
UID:indico-contribution-2208@cern.ch
DESCRIPTION:Speakers: Eugenia Koptyaeva ()\nResults of the 1D numerical si
 mulations of the neutrino radiation in core-collapse supernova were analyz
 ed. Simple analytical approximation of local angular distribution of neutr
 ino momentum is suggested. The proposed approximation is verified on resul
 ts of numerical simulation in different parts of supernova and at some val
 ues of times after a bounce. With well-known analytical approximation of n
 eutrino energy distribution\, the local distribution function of neutrino 
 in supernova is constructed. Obtained results can be used for estimations 
 of significance of neutrino processes in core-collapse supernova. The work
  is supported by the Russian Science Foundation (Grant No. 18-72-10070).\n
 \nhttps://indico.particle.mephi.ru/event/35/contributions/2208/
LOCATION:Discord Poster Server
URL:https://indico.particle.mephi.ru/event/35/contributions/2208/
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