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VERSION:2.0
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BEGIN:VEVENT
SUMMARY:Black hole ringing in General Relativity and beyond
DTSTART:20251127T143000Z
DTEND:20251127T160000Z
DTSTAMP:20260627T173739Z
UID:8e5e47c7-37c1-49f8-a0cc-779dc5f8db49
SEQUENCE:2
CREATED:20251124T093430Z
DESCRIPTION:The black hole ringdown offers a powerful window into both ast
 ro- and fundamental physics. However\, the construction of an accurate and
  reliable theoretical template for the interpretation of real data is cruc
 ial. In this seminar\, I will discuss how ringdown modes respond to some d
 itinct physical key-effects.First\, I will talk about the impact of a dyna
 mical evolution of the black hole mass due to accretion or radiation. Then
 \, I will present a parametrized framework to describe possible deviations
  from General Relativity in the ringdown spectrum of spinning black holes.
  Finally\, I will explore how incomplete ringdown modeling can bias parame
 ter estimation for massive black hole binaries observed by LISA\, and asse
 ss the optimal degree of accuracy of the template that is required across 
 parameter space.
LAST-MODIFIED:20251124T093447Z
LOCATION:DF Seminar Room (2-8.3)\, 2nd floor of Physics Building
URL:http://df.vps.tecnico.ulisboa.pt/pt/eventos/black-hole-ringing-in-gene
 ral-relativity-and-beyond/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="8iinc">The black hole ring
 down offers a powerful window into both astro- and fundamental physics. Ho
 wever\, the construction of an accurate and reliable theoretical template 
 for the interpretation of real data is crucial. In this seminar\, I will d
 iscuss how ringdown modes respond to some ditinct physical key-effects.</p
 ><p data-block-key="ck1l1"></p><p data-block-key="6ko22">First\, I will ta
 lk about the impact of a dynamical evolution of the black hole mass due to
  accretion or radiation. Then\, I will present a parametrized framework to
  describe possible deviations from General Relativity in the ringdown spec
 trum of spinning black holes. Finally\, I will explore how incomplete ring
 down modeling can bias parameter estimation for massive black hole binarie
 s observed by LISA\, and assess the optimal degree of accuracy of the temp
 late that is required across parameter space.</p>
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