Authors: Christian Corda
It is an intuitive but general conviction that black holes (BHs) result in highly excited states representing both the “hydrogen atom” and the “quasi-thermal emission” in quantum gravity. Here we show that such an intuitive picture is more than a picture, discussing a model of quantum BH somewhat similar to the historical semi-classical model of the structure of a hydrogen atom introduced by Bohr in 1913. Our model has important implications on the BH information puzzle and on the non-strictly random character of Hawking radiation. It is also in perfect agreement with existing results in the literature, starting from the famous result of Bekenstein on the area quantization. This paper improves, clarifies and finalizes some recent results that, also together with collaborators, we published in various peer reviewed journals. Preliminary results on the model in this paper have been recently discussed in an Invited Lecture at the 12th International Conference of Numerical Analysis and Applied Mathematics.
Comments: 17 Pages.
Download: PDF
[v1] 2014-10-30 13:17:08
Unique-IP document downloads: 168 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.