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SUMMARY:Gravitational Wave Models and Post-Minkowskian Contributions
DTSTART:20250324T130000Z
DTEND:20250324T140000Z
DTSTAMP:20260511T112900Z
UID:indico-event-46326@agenda.infn.it
DESCRIPTION:Speakers: Piero Rettegno (Università di Perugia)\n\nGravitati
 onal wave (GW) emission from compact binaries hastraditionally been modele
 d using post-Newtonian (PN) methods.In recent years\, the post-Minkowskian
  (PM) framework hasgained significant traction for two main reasons. First
 \, thePM approximation is better suited for describing non-circularbinarie
 s\, which are expected to be detected more frequentlyby future generations
  of GW detectors. Second\, computationaltechniques from quantum mechanics 
 have been increasinglyapplied to derive higher-order PM contributions. Thi
 s talkwill present recent developments in GW modeling using PMresults\, as
  well as the prospects for accurately describingbinaries on generic orbits
 \, meeting the precision requiredby future GW observatories.\n\nhttps://ag
 enda.infn.it/event/46326/
LOCATION:Aula Galileo
URL:https://agenda.infn.it/event/46326/
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