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VERSION:2.0
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BEGIN:VEVENT
SUMMARY:Microstates on a grid: a Numerical Relativity approach to the blac
 k-hole microstructure
DTSTART:20260618T143000Z
DTEND:20260618T160000Z
DTSTAMP:20260801T232209Z
UID:76185efb-630f-4a64-82d0-1e0e37f897e8
SEQUENCE:1
CREATED:20260616T081049Z
DESCRIPTION: Recent progress in the construction of more realistic (non-su
 persymmetric) black-hole microstates that could account for the Bekenstein
 -Hawking entropy has yielded novel families of regular and horizonless bla
 ck-hole mimickers. In this talk\, I will briefly review the known classica
 l phenomenology of these “topological solitons”. I will then report on
  the current effort to model the full nonlinear dynamics of these microsta
 te models with a Numerical Relativity approach. 
LAST-MODIFIED:20260616T081049Z
LOCATION:DF Seminar Room (2-8.3)\, 2nd floor of Physics Building
URL:http://df.vps.tecnico.ulisboa.pt/en/events/microstates-on-a-grid-a-num
 erical-relativity-approach-to-the-black-hole-microstructure/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="oy7my"> Recent progress in
  the construction of more realistic (non-supersymmetric) black-hole micros
 tates that could account for the Bekenstein-Hawking entropy has yielded no
 vel families of regular and horizonless black-hole mimickers. In this talk
 \, I will briefly review the known classical phenomenology of these “top
 ological solitons”. I will then report on the current effort to model th
 e full nonlinear dynamics of these microstate models with a Numerical Rela
 tivity approach.<br/> </p>
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