Abstract
Static black holes in two-dimensional string theory can carry tachyon hair. Configurations which are nonsingular at the event horizon have a nonvanishing asymptotic energy density. Such solutions can be smoothly extended through the event horizon and have a nonvanishing energy flux emerging from the past singularity. Dynamical processes will not change the amount of tachyon hair on a black hole. In particular, there will be no tachyon hair on a black hole formed in gravitational collapse if the initial geometry is the linear dilaton vacuum. There also exist static solutions with a finite total energy, which have singular event horizons. Simple dynamical arguments suggest that black holes formed in gravitational collapse will not have tachyon hair of this type.
| Original language | English |
|---|---|
| Pages (from-to) | 2415-2420 |
| Number of pages | 6 |
| Journal | Physical Review D |
| Volume | 48 |
| Issue number | 6 |
| DOIs | |
| Publication status | Published - 1993 |
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