View source for Talk:Bekenstein-Hawking entropy

== Reviewer B ==
Only two minor suggestions:

1- After equation (12) I would rather say that the content of the GSL is the area theorem in the classical limit. This is because it is not possible to avoid ordinary entropy in the quantum case due to Hawking radiation, and on the other hand the area theorem works also when there is external matter entropy if it satisfies the appropriate energy condition.  

2- I would repeat the citation to Bombelli et al in the section dedicated to entanglement entropy since their paper was written much earlier than the one by Srednicki.

There are some typos: "wodered" instead of wondered, and "an hole" and "an handle" which (I believe) should be replaced by "a hole" and "a handle". Also the numbers of the referred equations would have to be separated from the previous words.