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SUMMARY:Non-singular black holes without quantum gravity nor exotic physic
 s
DTSTART:20260330T120000Z
DTEND:20260330T140000Z
DTSTAMP:20260419T021900Z
UID:indico-event-13523@indico.ijclab.in2p3.fr
CONTACT:jacopo.mazza@ijclab.in2p3.fr
DESCRIPTION:Speakers: Francesco Di Filippo (Goethe U.)\n\nSingularity theo
 rems suggest that spacetime singularities are unavoidable in general relat
 ivity when matter satisfies standard energy conditions. Although Hawking r
 adiation provides a well-understood mechanism for violating these conditio
 ns\, the resulting violation is commonly regarded as too weak to remove si
 ngularities\, reinforcing the view that exotic physics or full quantum gra
 vity is required. In this talk\,we challenge this view by analyzing a char
 ged spherically symmetric black hole formed through gravitational collapse
  and evaporating via Hawking radiation. We show that the electromagnetic r
 epulsion and the mild violation of energy conditions due to the presence o
 f Hawking radiation can be sufficient to avoid the formation of both a sin
 gularity and a Cauchy horizon.\n\nhttps://indico.ijclab.in2p3.fr/event/135
 23/
LOCATION:210/1-114 - Salle des Séminaires (IJCLab)
URL:https://indico.ijclab.in2p3.fr/event/13523/
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