Abstract
The controversy over whether the particles scatter from each other after being emitted is reviewed. It is shown that a self-consistent description is afforded by the application of relativistic viscous fluid equations, at least towards the end of the black hole's existence and under some assumptions.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1670-1673 |
| Number of pages | 4 |
| Journal | Physical review letters |
| Volume | 86 |
| Issue number | 9 |
| DOIs | |
| State | Published - Feb 26 2001 |