Abstract
It is shown that in general the energy and the Hamiltonian of matter fields on the black hole exterior play different roles. is a generator of the time evolution along the Killing time while enters the first law of black hole thermodynamics. For nonminimally coupled fields the difference is not zero and is a Noether charge Q analogous to that introduced by Wald to define the black hole entropy. If fields vanish at the spatial boundary, Q is reduced to an integral over the horizon. The analysis is carried out and an explicit expression for Q is found for general diffeomorphism invariant theories. As an extension of the results by Wald and co-workers, the first law of black hole thermodynamics is derived for arbitrary weak matter fields.
- Received 8 September 1998
DOI:https://doi.org/10.1103/PhysRevD.59.064020
©1999 American Physical Society