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dc.contributor.authorAmes, Ellery
dc.contributor.authorAndréasson, Håkan
dc.contributor.authorRinne, Oliver
dc.date.accessioned2020-12-15T12:59:44Z
dc.date.available2020-12-15T12:59:44Z
dc.date.issued2020-12-15
dc.identifier.urihttp://publications.mfo.de/handle/mfo/3820
dc.description.abstractWe numerically investigate the dynamcis near black hole formation of solutions to the Einstein-Vlasov system in axisymmetry. Our results are obtained using a particle-in-cell and finite difference code based on the (2+1)+1 formulation of the Einstein field equations in axisymmetry. Solutions are launched from generic type initial data and exhibit type I critical behaviour. In particular we find lifetime scaling in solutions containing black holes, and support that the critical solutions are stationary. Our results contain examples of solutions that form black holes, perform damped oscillations, and appear to disperse. We prove that complete dispersal of the solution implies that it has nonpositive binding energy.en_US
dc.language.isoen_USen_US
dc.publisherMathematisches Forschungsinstitut Oberwolfachen_US
dc.relation.ispartofseriesOberwolfach Preprints;2020-22
dc.titleDynamics of Gravitational Collapse in the Axisymmetric Einstein-Vlasov Systemen_US
dc.typePreprinten_US
dc.rights.licenseDieses Dokument darf im Rahmen von § 53 UrhG zum eigenen Gebrauch kostenfrei heruntergeladen, gelesen, gespeichert und ausgedruckt, aber nicht im Internet bereitgestellt oder an Außenstehende weitergegeben werden.de
dc.rights.licenseThis document may be downloaded, read, stored and printed for your own use within the limits of § 53 UrhG but it may not be distributed via the internet or passed on to external parties.en
dc.identifier.doi10.14760/OWP-2020-22
local.scientificprogramResearch in Pairs 2020en_US
local.series.idOWP-2020-22en_US
dc.identifier.urnurn:nbn:de:101:1-2021011210081898726445
dc.identifier.ppn1744533695


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