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SUMMARY:Thermalization of dark atoms
DTSTART;VALUE=DATE-TIME:20261027T162500Z
DTEND;VALUE=DATE-TIME:20261027T163000Z
DTSTAMP;VALUE=DATE-TIME:20261021T015502Z
UID:indico-contribution-6493@cern.ch
DESCRIPTION:Speakers: Данила Сопин ()\nHeavy strongly interacti
 ng dark matter particles are excluded by data from several experiments (IM
 P-7/8\, XQC\, RRS\, CRESST\, CDMS\, and others) within scenarios which ass
 ume a velocity-independent nuclear elastic scattering cross section. Howev
 er\, taking into account the location of the detectors avoids some of the 
 constraints if energy loss leads to an increase in such cross section. Sce
 narios of the thermalization of 2-10 TeV particles were analyzed for sever
 al functions $\\sigma = \\sigma (v)$. The velocity and angular distributio
 ns for several penetration depths into the atmosphere and the upper layers
  of rock were calculated. The results are compared with existing constrain
 ts on SIMPs.\n\nhttps://indico.particle.mephi.ru/event/626/contributions/6
 493/
LOCATION:Sevastopol hotel Conference Hall 1
URL:https://indico.particle.mephi.ru/event/626/contributions/6493/
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