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SUMMARY:Kyriakos Destounis (Tubingen U.)
DTSTART:20210608T133000Z
DTEND:20210608T143000Z
DTSTAMP:20260423T035748Z
UID:CENTRA/48
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CENTRA/48/">
 Gravitational-wave imprints of non-integrable extreme-mass-ratio inspirals
 </a>\nby Kyriakos Destounis (Tubingen U.) as part of CENTRA Seminar\n\n\nA
 bstract\nThe detection of gravitational waves from extreme-mass-ratio insp
 irals (EMRIs) with upcoming space-borne detectors will allow for unprecede
 nted tests of general relativity in the strong-field regime. Aside from as
 sessing whether black holes are unequivocally described by the Kerr metric
 \, they may place constraints on the degree of spacetime symmetry. Dependi
 ng on exactly how a hypothetical departure from the Kerr metric manifests\
 , the Carter symmetry\, which implies the integrability of the geodesic eq
 uations\, may be broken. In this talk\, I will discuss the impact of non-i
 ntegrability in EMRIs which involve a supermassive compact object with ano
 malous multipolar structure. After reviewing the features of chaotic pheno
 mena in EMRIs\, I will argue that non-integrability is precisely imprinted
  in the gravitational waveform. Explicit examples of non-integrable EMRIs 
 will be discussed\, as well as their role in LISA data analysis.\n\nThis t
 alk will be based on the following articles:\n\nPhys.Rev.D 102 (2020) 6\, 
 064041\nPhys.Rev.Lett. 126 (2021) 14\, 141102\n
LOCATION:https://researchseminars.org/talk/CENTRA/48/
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