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/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.