Video URL
https://pirsa.org/17030055Sub-Planckian Black Holes
APA
Mureika, J. (2017). Sub-Planckian Black Holes. Perimeter Institute for Theoretical Physics. https://pirsa.org/17030055
MLA
Mureika, Jonas. Sub-Planckian Black Holes. Perimeter Institute for Theoretical Physics, Mar. 09, 2017, https://pirsa.org/17030055
BibTex
@misc{ scivideos_PIRSA:17030055, doi = {10.48660/17030055}, url = {https://pirsa.org/17030055}, author = {Mureika, Jonas}, keywords = {Strong Gravity}, language = {en}, title = {Sub-Planckian Black Holes}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2017}, month = {mar}, note = {PIRSA:17030055 see, \url{https://scivideos.org/index.php/pirsa/17030055}} }
Jonas Mureika Loyola Marymount University
Abstract
The characteristics of black holes smaller than the Planck scale are addressed. These result from a modified metric that reproduces desirable aspects of a variety of disparate models in the sub-Planckian limit, while remaining Schwarzschild in the large mass limit. The self-dual nature of this solution has two interesting features: first, it naturally implies the Generalized Uncertainty Principle. Secondly, this metric exhibits an effective dimensional reduction feature, indicating that the gravitational physics of the sub-Planckian regime is effectively (1+1)-D.