Extending the Black Hole Uniqueness Theorems I. Accelerating Black Holes: The Ernst Solution and C-Metric
نویسنده
چکیده
We present black hole uniqueness theorems for the C-metric and Ernst solution. The proof follows a similar strategy as that used to prove the uniqueness of the Kerr-Newman solution, however the presence of an acceleration horizon provides some critical differences. We also show how to derive the Bunting/Mazur result (on the positivity of a suitable divergence required in the proof) using new methods. We briefly explain the importance of the uniqueness of the Ernst solution in relation to the proposed black hole monopole pair creation mediated by the related instanton. Typeset using REVTEX ∗Electronic address: [email protected] 1
منابع مشابه
Extending the Black Hole Uniqueness Theorems II. Superstring Black Holes
We make use of an internal symmetry of a truncation of the bosonic sector of the superstring and N = 4 supergravity theories to write down an analogue of Robinson’s identity for the black holes of this theory. This allows us to prove the uniqueness of a restricted class of black hole solutions. In particular, we can apply the methods of the preceding paper to prove the uniqueness of a class of ...
متن کاملGlobal aspects of accelerating and rotating black hole space-times
The complete family of exact solutions representing accelerating and rotating black holes with possible electromagnetic charges and a NUT parameter is known in terms of a modified Plebański–Demiański metric. This demonstrates the singularity and horizon structure of the sources but not that the complete space-time describes two causally separated black holes. To demonstrate this property, the m...
متن کاملPair creation of extremal black holes and Kaluza-Klein monopoles.
Classical solutions describing charged dilaton black holes accelerating in a background magnetic field have recently been found. They include the Ernst metric of the EinsteinMaxwell theory as a special case. We study the extremal limit of these solutions in detail, both at the classical and quantum levels. It is shown that near the event horizon, the extremal solutions reduce precisely to the s...
متن کاملBlack holes: Classical properties, thermodynamics, and heuristic quantization, in
I start with a discussion of the no-hair principle. The hairy black hole solutions of recent vintage do not deprive it of value because they are often unstable. Generic properties of spherical static black holes with nonvacuum exteriors are derived. These form the basis for the discussion of the new no scalar hair theorems. I discuss the generic phenomenon of superradiance for its own sake, as ...
متن کاملar X iv : g r - qc / 9 60 50 59 v 1 2 8 M ay 1 99 6 Black hole hair : twenty – five years after
Originally regarded as forbidden, black hole “hair” are fields associated with a stationary black hole apart from the gravitational and electromagnetic ones. Several stable stationary black hole solutions with gauge or Skyrme field hair are known today within general relativity. We formulate here a “no scalar– hair” conjecture, and adduce some new theorems that almost establish it by ruling out...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008