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Overview of Solutions

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 $a$ in action.

\begin{displaymath}e^{\phi} F^2 \Rightarrow e^{a\phi} F^2 \end{displaymath}

Solvable E.O.M. only in the first and second case.
Solution generating symmetries in case three (Lorentz boost) and four ($SL(2,R)$).

Solution for vector field(s) in first three cases:

\begin{displaymath}F_{rt}=Q/r^2 \qquad F_{\theta\phi}=G\sin{\theta} \end{displaymath}

Class E.O.M. constraints Global structure
1 no $\Psi \rightarrow QG=0$ Ss
2 no $\Psi \rightarrow D=0$ RN
  no $\sigma \rightarrow Q_- ^2=G_- ^2$  
3 no $\Psi \rightarrow D=0$ Ss
4 class $1 \rightarrow a=1$ Ss
  class $2 \rightarrow Q_- ^2=G_- ^2$ RN
  class $3 \rightarrow Q_A G_A=Q_B G_B$ Ss
Where $D=Q_A G_B +Q_B G_A$ and $Q_{\pm}^2=Q_A ^2 \pm Q_B ^2$.
Table of Stringy Solutions
     
Class Scalars Metric
     
     
1 $e^\phi =\left( \frac{r-r_-}{r} \right)
^{\frac{-2a}{1+a^2}}$ $\lambda =\left( \frac{r-r_+}{r} \right) \left(
\frac{r-r_-}{r} \right) ^{\frac{1-a^2}{1+a^2}}$
    $R^2 =r^2 \left( \frac{r-r_-}{r} \right)
^{\frac{2a^2}{1+a^2}}$
     
     
2 $e^\phi =\frac{r+\Sigma}{r-\Sigma}$ $\lambda =\frac{(r-r_+)(r-r_-)}{(r-\Sigma)(r+\Sigma)}$
    $R^2=(r-\Sigma)(r+\Sigma)$
     
     
3 $e^\phi
=\frac{\sqrt{(r-\Sigma_1)(r+\Sigma_1)}}{r-\Sigma_2}$ $\lambda =\frac{r-r_+}{\sqrt{(r-\Sigma_1)(r+\Sigma_1)}}$
  $\sigma =\frac{r-\Sigma_1}{r+\Sigma_1}$ $R^2=\sqrt{(r-\Sigma_1)(r+\Sigma_1)}(r-\Sigma_2)$
     
Class 4: Axion Black Holes.
Solution generating symmetry which leaves the (Einstein) metric invariant.
$\displaystyle {e^\phi}'$ $\textstyle =$ $\displaystyle \frac{e^\phi}{a^2 +b^2 e^{2\phi}} \quad \Psi
'=\frac{ac+bd e^{2\phi}}{a^2+b^2 e^{2\phi}}$  
$\displaystyle F_A '$ $\textstyle =$ $\displaystyle a F_A -be^\phi \sigma^{-1} \tilde F_B$  

Area singularities are responsible for different properties w.r.t. General Relativity Black Holes.
Table of Parameter Relations
   
Class Parameter relations
   
   
1 $Q^2 =\frac{4 r_+ r_-}{1+a^2}$
  $2M=r_+ + \left( \frac{1-a^2}{1+a^2} \right) r_-$
   
   
2 $\Sigma (r_+ + r_-)={\textstyle{1\over 4}}\left( Q_+^2 -G_+^2
\right)$
  $\Sigma ^2 +r_+ r_- ={\textstyle{1\over 4}}\left( Q_+^2 +G_+^2
\right)$
  $2M=r_+ +r_- $
   
   
3 $Q_A ^2=(\Sigma_1 -\Sigma_2 )(\Sigma_1 -r_+)$
  $Q_B ^2=(\Sigma_1 +\Sigma_2 )(\Sigma_1 +r_+)$
  $r_+ =2M$
   

Note: Dilaton-Modulus Black Hole solutions have been obtained with electrical charge only.

Axion solutions lead to new parameter relations for every class.


next up previous contents
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