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SUMMARY:Nuclear and astrophysics aspects for the rapid neutron capture pro
 cess in the era of multi-messenger observations. (May 1\, 2019. Trento\, I
 taly)
DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20190501T090000
DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20190501T170000
DTSTAMP;VALUE=DATE-TIME:20201230T131446Z
UID:1d46c9ee820041a9b37c0c73b0ffce14
ATTENDEE;CN="Dr Laetitia Canete; Dr Benoit Cote; Dr Marius Eichler; Dr Tob
 ias Fischer; Mr Stylianos Nikas; Mr Ante Ravlic";ROLE=REQ-PARTICIPANT:Dr L
 aetitia Canete; Dr Benoit Cote; Dr Marius Eichler; Dr Tobias Fischer; Mr S
 tylianos Nikas; Mr Ante Ravlic
CREATED;VALUE=DATE-TIME:20200120T151926Z
DESCRIPTION:The rapid-neutron capture process (r-process) is responsible f
 or producing around half of all nuclides heavier than iron. One site for t
 he r-process was recently confirmed: the advanced LIGO and Virgo detectors
  observed two neutron stars merging and immediate follow-up observations w
 ere fully compatible with a kilonova\, a thermal “afterglow” powered b
 y radioactive decay of newly synthesized r-process material. Moreover\, th
 e observations indicated that neutron-star mergers produce a blue lanthani
 de-free signal followed by a red lanthanide-rich component\, contrary to e
 xpectations. Although neutron-star mergers are now known to be r-process e
 lement factories\, this might not be the only r-process site\, and a compr
 ehensive understanding and description of the r-process is still lacking. 
 This workshop will bring together theorists and experimentalists to addres
 s the many aspects of nuclear physics and astrophysics that must be consid
 ered and properly understood in order to model the r-process.
LAST-MODIFIED;VALUE=DATE-TIME:20200128T165028Z
LOCATION:ECT* (European Centre for Theoretical Studies in Nuclear Physics 
 and Related Areas). Trento\, Italy
URL:http://www.chetec.eu/events/nuclear-and-astrophysics-aspects-for-the-r
 apid-neutron-capture-process-in-the-era-of-multi-messenger-observations
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TZID:Europe/Paris
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