Electromagnetic self-force as a cosmic censor
APA
Poisson, E. (2011). Electromagnetic self-force as a cosmic censor . Perimeter Institute. https://pirsa.org/11050063
MLA
Poisson, Eric. Electromagnetic self-force as a cosmic censor . Perimeter Institute, May. 25, 2011, https://pirsa.org/11050063
BibTex
@misc{ pirsa_PIRSA:11050063, doi = {10.48660/11050063}, url = {https://pirsa.org/11050063}, author = {Poisson, Eric}, keywords = {}, language = {en}, title = {Electromagnetic self-force as a cosmic censor }, publisher = {Perimeter Institute}, year = {2011}, month = {may}, note = {PIRSA:11050063 see, \url{https://pirsa.org}} }
University of Guelph
Collection
Talk Type
Abstract
Hubeny identified a scenario in which a charged particle falling toward a near-extreme Reissner-Nordstrom black hole can penetrate the black hole and drive it beyond the extremal limit, thereby giving rise to an apparent violation of cosmic censorship. A version of this scenario, relevant to a Kerr black hole and involving a particle with orbital and/or spin angular momentum, was recently examined by Jacobson and Sotiriou (following up on earlier work by Hod); here also the black hole is driven beyond the extremal limit. The Hubeny analysis was inconclusive, however, because in her scenario the particle crosses the horizon with a near-vanishing acceleration; the test-body acceleration is of the same order of magnitude as the acceleration produced by the particle's own electromagnetic self-force, which was not fully incorporated in the analysis. In this talk we report on our computation of the electromagnetic self-force acting on a charged particle falling radially toward a Reissner-Nordstrom black hole, and we reveal whether the self-force acts as a cosmic censor by preventing the particle from reaching the event horizon.