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SUMMARY:Nuclear reactions in stars far below the Coulomb barrier
DTSTART;VALUE=DATE-TIME:20081120T110000Z
DTEND;VALUE=DATE-TIME:20081120T120000Z
DTSTAMP;VALUE=DATE-TIME:20260618T201928Z
UID:indico-event-821@indico.ific.uv.es
DESCRIPTION:It is in the nature of astrophysics that many of the processes
  and objects one tries to understand are physically inaccessible. Thus\, i
 t is important that those aspects that can be studied in the laboratory be
  rather well understood. One such aspect are nuclear fusion reactions\, wh
 ich are at the heart of nuclear astrophysics: they influence sensitively t
 he nucleosynthesis of the elements in the earliest stages of the universe 
 and in all the objects formed thereafter\, and control the associated ener
 gy generation\, neutrino luminosity\, and evolution of stars. A good knowl
 edge of the rates of these reactions is thus essential for understanding t
 his broad picture.\n\nhttps://indico.ific.uv.es/event/821/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/821/
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