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SUMMARY:Exploring the Sun's core with BabyIAXO
DTSTART;VALUE=DATE-TIME:20210830T154500Z
DTEND;VALUE=DATE-TIME:20210830T160000Z
DTSTAMP;VALUE=DATE-TIME:20260810T053127Z
UID:indico-contribution-15689@indico.ific.uv.es
DESCRIPTION:Speakers: Javier Galan (Universidad de Zaragoza)\nAxions are a
  natural consequence of the Peccei-Quinn mechanism\, the most compelling s
 olution to the strong-CP problem. Similar axion-like particles (ALPs) also
  appear in a number of possible extensions of the Standard Model\, notably
  in string theories. Both axions and ALPs are very well motivated candidat
 es for Dark Matter\, and in addition\, they would be copiously produced at
  the sun’s core. A relevant effort during the last decade has been the C
 AST experiment at CERN\, the most sensitive axion helioscope to-date. The 
 International Axion Observatory (IAXO) is a large-scale 4th generation hel
 ioscope. As its primary physics goal\, IAXO will look for solar axions or 
 ALPs with a signal to background ratio of about 5 orders of magnitude high
 er than CAST.\n\nIn this talk I will briefly review astrophysical hints an
 d models that we will be able to explore while searching for solar axions 
 within the context of the IAXO helioscope search program\, and in particul
 ar the physics under reach of BabyIAXO\, and intermediate helioscope stage
  towards the full IAXO.\n\nhttps://indico.ific.uv.es/event/6178/contributi
 ons/15689/
LOCATION:
URL:https://indico.ific.uv.es/event/6178/contributions/15689/
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