Universality of highly damped quasinormal modes for single horizon black holes
Universality of highly damped quasinormal modes for single horizon black holes
It has been suggested that the highly damped quasinormal modes of black holes provide information about the microscopic quantum gravitational states underlying black-hole entropy. This interpretation requires the form of the highly damped quasinormal mode frequency to be universally of the form: [Formula: see text] = ln(l)kT BH , where …