University of Cambridge > > DAMTP Friday GR Seminar > Global structure of spherically symmetric charged scalar field spacetimes

Global structure of spherically symmetric charged scalar field spacetimes

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact David Kubiznak.

In this talk, we present recent results concerning the spherical collapse of self-gravitating charged scalar fields. The main result gives a complete characterization of the future boundary of spacetime, providing a starting point for studying the cosmic censorship conjectures. As a simple corollary, we show that scenarios of `naked singularity’ formation by means of `super-charging’ (near-)extremal Reissner-Nordstrom black holes are impossible. We will also discuss results on trapped surface formation, Cauchy horizon stability and spacetime extendibility. The main difficulty in delimiting the boundary is isolated in proving a suitable global extension principle which effectively excludes a broad class of singularity formation. This suggests a new notion of `strongly tame’ matter models which we introduce. The boundary characterization given extends to any such `strongly tame’ Einstein-matter system.

This talk is part of the DAMTP Friday GR Seminar series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.


© 2006-2023, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity