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SUMMARY:Detecting dark matter from Supernovae
DTSTART:20180621T140000
DTSTAMP:20260504T090548Z
UID:d855c022ec668d52b0c2599af0eaf8a41d3019256318e75739dd8e8c
CATEGORIES:Conferences - Seminars
DESCRIPTION:Gustavo Tavares\nThe central region of Supernovae are one of t
 he hottest and densest regions in the Universe. Due to the high temperatur
 es\, particles with sub-GeV masses can be copiously produced if they have 
 non-negligible couplings to the Standard Model. If dark matter has sub-GeV
  mass it will be produced in the hot Supernovae core and it will have suff
 iciently large momenta to be detectable in direct detection experiments. I
 n this work we investigate the sensitivity of current and future Xenon bas
 ed direct detection experiments to a simplified model of dark matter which
  interacts with the Standard Model via the dark photon portal
LOCATION:BSP 727 https://plan.epfl.ch/?room==BSP%20727
STATUS:CONFIRMED
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