On the quest for a holographic interpretation of the black hole evaporation process

TL;DR

This paper discusses the challenges of interpreting black hole evaporation holographically, but was withdrawn and recommends more recent work for general results on black hole formation and evolution.

Contribution

The paper attempted to explore a holographic interpretation of black hole evaporation but was withdrawn, indicating ongoing challenges in this research area.

Findings

Hawking radiation was derived for a specific tail model

The model used was considered somewhat unphysical

More general results are available in hep-th/0407191

Abstract

This paper has been withdrawn by the authors because the Hawking radiation outside the core was just obtained for a specific (and somewhat unphysical) model of the tail. Interested readers should instead look at the more recent hep-th/0407191 where more general results are given for the formation and evolution of black-holes on the brane.