Figure 3: Spacetime uncertainty (red, solid) vs uncertainty from spherical black holes (blue, dotted)
in 
dimensions, for 
(left) and 
(right). After [318], Figure 1. Below the
bound from spacetime uncertainty yet above the black-hole bound that hides short-distance physics
(shaded region), the concept of classical geometry becomes meaningless.
dimensions, for (left) and (right). After [318], Figure 1. Below the
bound from spacetime uncertainty yet above the black-hole bound that hides short-distance physics
(shaded region), the concept of classical geometry becomes meaningless.Sabine Hossenfelder, "Minimal Length Scale Scenarios for Quantum Gravity",
Living Rev. Relativity, 16 (2013), 2, doi:10.12942/lrr-2013-2, URL (accessed <date>): http://www.livingreviews.org/lrr-2013-2.
This work is licensed under a Creative Commons License.
© The author(s), except where otherwise noted.
Living Rev. Relativity, 16 (2013), 2, doi:10.12942/lrr-2013-2, URL (accessed <date>): http://www.livingreviews.org/lrr-2013-2.
This work is licensed under a Creative Commons License.
© The author(s), except where otherwise noted.