Thermal Hadron Production by QCD Hawking Radiation

Details Thermal Hadron Production by QCD Hawking Radiation Thermal Hadron Production by QCD Hawking Radiation

2006-12-12

arxiv.org/abs/hep-ph/0612151v1

PoSCPOD2006:039,2006

Physics

High Energy Physics

High Energy Physics - Phenomenology

17 pages, 12 figures; updated version of an invited talk at the workshop "Critical Point and Onset of Deconfinement", Firenze/

Scientific paper

10.1143/PTPS.168.338

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''.

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