PIRSA:17030055

Sub-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

Talk numberPIRSA:17030055
Source RepositoryPIRSA
Collection

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.