APA

Mureika, J. (2017). Sub-Planckian Black Holes. Perimeter Institute. https://pirsa.org/17030055

MLA

Mureika, Jonas. Sub-Planckian Black Holes. Perimeter Institute, Mar. 09, 2017, https://pirsa.org/17030055

BibTex

@misc{ pirsa_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},
  year = {2017},
  month = {mar},
  note = {PIRSA:17030055 see, \url{https://pirsa.org}}
}
            

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.