Please use this identifier to cite or link to this item: https://scholarbank.nus.edu.sg/handle/10635/171914
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dc.titleA scale-critical trapped surface formation criterion for the Einstein-Maxwell system
dc.contributor.authorAN XINLIANG
dc.contributor.authorAthanasiou, Nikolaos
dc.date.accessioned2020-08-05T07:59:55Z
dc.date.available2020-08-05T07:59:55Z
dc.date.issued2020-05-25
dc.identifier.citationAN XINLIANG, Athanasiou, Nikolaos (2020-05-25). A scale-critical trapped surface formation criterion for the Einstein-Maxwell system. https://arxiv.org/abs/2005.12699. ScholarBank@NUS Repository.
dc.identifier.urihttps://scholarbank.nus.edu.sg/handle/10635/171914
dc.description.abstractInthisstudyweshowthat, fromarbitrarilydispersedinitialdata, boththefocusingofelectromagnetic fields and the concentration of gravitational waves could lead to the formation of trapped surfaces. We establish a scale–critical semi–global existence result from past null infinity for the Einstein–Maxwell system by assigning the signature for decay rates to geometric quantities and Maxwell components. This result generalizes an approach of the first author on studying the Einstein vacuum equations by employing additional elliptic estimates and geometric renormalizations and it also extends a result of Yu to the scale–critical regime.
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dc.typeArticle
dc.date.updated2020-08-02T07:35:32Z
dc.contributor.departmentMATHEMATICS
dc.description.sourcetitlehttps://arxiv.org/abs/2005.12699
dc.published.stateUnpublished
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