Psychosocial and Sociodemographic Characteristics of DWI Offenders

A bound on the effective gravitational coupling from semiclassical black holes

“…Supposedly in string theory there are no BHs smaller than l s , since at that point BHs turn into ordinary, non collapsed, "large" objects [15]. More exotic possibilities can be considered, however, where BHs smaller than l s and with temperature higher than the Hagedorn temperature M s might exist.…”

“…Here we wish to emphasize that weakly coupled string theory is an example of a theory that contains semiclassical BH with sizes all the way down to the cutoff scale l s but where, at the same time, BHs remain as classical as one wishes for all length scales since MR S = g −2 s > N. Then, supposedly, they stop existing as BHs and turn into ordinary weakly-coupled strings . Supposedly in string theory there are no BHs smaller than l s , since at that point BHs turn into ordinary, non collapsed, "large" objects [15]. More exotic possibilities can be considered, however, where BHs smaller than l s and with temperature higher than the Hagedorn temperature M s might exist.…”