Abstract
We consider the interesting “near-horizon test” reported in S. E. P. Bergliaffa and Y. E. C. de O. Nunes, Phys. Rev. D 84, 084006 (2011) for any static, spherically symmetric black hole solution admitted in gravity. Before adopting the necessary conditions for the test, however, revisions are needed as we point out in this Comment.
- Received 31 July 2012
DOI:https://doi.org/10.1103/PhysRevD.86.088501
© 2012 American Physical Society