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VERSION:2.0
PRODID:-//linuxsoftware.nz//NONSGML Joyous v1.4//EN
BEGIN:VEVENT
SUMMARY:Quasi-normal modes of rotating black holes beyond General Relativi
 ty
DTSTART:20250213T143000Z
DTEND:20250213T160000Z
DTSTAMP:20260916T134456Z
UID:f471e1b8-c7a3-4a05-aec8-f73fb7c44adc
SEQUENCE:2
CREATED:20250211T112546Z
DESCRIPTION:In this talk\, I will summarize the recent advancements of qua
 si-normal modes in alternative theories of gravity. I will explain the mai
 n issues in computing the characteristic frequencies of rotating black hol
 es and what are the most prominent strategies to tackle this problem. The 
 approaches covered include the slow-spin and small-coupling expansions. In
  particular\, I will present a beyond-Teukolsky approach for the computati
 on of quasi-normal modes using the continued fraction method\, and its app
 lication in several modified theories of gravity.
LAST-MODIFIED:20250211T112559Z
LOCATION:DF Seminar Room (2-8.3)\, 2nd floor of Physics Building
URL:http://df.vps.tecnico.ulisboa.pt/pt/eventos/quasi-normal-modes-of-rota
 ting-black-holes-beyond-general-relativity/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="m8w65">In this talk\, I wi
 ll summarize the recent advancements of quasi-normal modes in alternative 
 theories of gravity. I will explain the main issues in computing the chara
 cteristic frequencies of rotating black holes and what are the most promin
 ent strategies to tackle this problem.<br/><br/> The approaches covered in
 clude the slow-spin and small-coupling expansions. In particular\, I will 
 present a beyond-Teukolsky approach for the computation of quasi-normal mo
 des using the continued fraction method\, and its application in several m
 odified theories of gravity.<br/></p>
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