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Fields constant or absent: four classes.
1. One vector field Dilaton Black Holes [23]
2. Two vector fields dyonic Dilaton Black Holes
3. Dilaton-Modulus Black Holes
4. Axion Black Holes
Class 1: extra coupling parameter
in action.
Solvable E.O.M. only in the first and second case.
Solution generating symmetries in case three (Lorentz boost)
and four (
).
Solution for vector field(s) in first three cases:
| Class |
E.O.M. constraints |
Global
structure |
| 1 |
no
 |
Ss |
| 2 |
no
 |
RN |
| |
no
 |
|
| 3 |
no
 |
Ss |
| 4 |
class
 |
Ss |
| |
class
 |
RN |
| |
class
 |
Ss |
Where
and
.
Table of Stringy Solutions
| |
|
|
| Class |
Scalars |
Metric |
| |
|
|
| |
|
|
| 1 |
 |
 |
| |
|
 |
| |
|
|
| |
|
|
| 2 |
 |
 |
| |
|
 |
| |
|
|
| |
|
|
| 3 |
 |
 |
| |
 |
 |
| |
|
|
Class 4: Axion Black Holes.
Solution generating symmetry which leaves the (Einstein)
metric invariant.
Area singularities are responsible for different properties
w.r.t. General Relativity Black Holes.
Table of Parameter Relations
| |
|
| Class |
Parameter relations |
| |
|
| |
|
| 1 |
 |
| |
 |
| |
|
| |
|
| 2 |
 |
| |
 |
| |
 |
| |
|
| |
|
| 3 |
 |
| |
 |
| |
 |
| |
|
Note: Dilaton-Modulus Black Hole solutions have been obtained
with electrical charge only.
Axion solutions lead to new parameter relations for every
class.
Next: Overview of Extremal Solutions
Up: Stringy Black Holes
Previous: The Symmetry Group O(d,d')
  Contents
Jan Pieter van de Schaar
2005-09-09