Thermal Hadron Production by QCD Hawking Radiation

Abstract

The QCD counterpart of Hawking radiation from black holes leads to thermal hadron production in high energy collisions, from $e^{+}{e}^{-}$ annihilation to heavy ion interactions. This hadronic radiation is formed by tunnelling through the event horizon of colour confinement and is emitted at a universal temperature $T_H\simeq (\sigma /2\pi {)}^{1/2}$, where $\sigma$ denotes the string tension. Since the event horizon does not allow information transfer, the radiation is thermal ``at birth''.

Comments: 17 pages, 12 figures; updated version of an invited talk at the workshop "Critical Point and Onset of Deconfinement", Firenze/Italy, July 3-6, 2006