The Exact String Black-Hole behind the hadronic Rindler horizon?

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dc.creatorCastorina, P.
dc.creatorGrumiller, D.
dc.creatorIorio, A.
dc.date2008-02-18
dc.date.accessioned2026-07-07T11:56:05Z
dc.date.available2026-07-07T11:56:05Z
dc.descriptionThe recently suggested interpretation of the universal hadronic freeze-out temperature T_f ~ 170 Mev - found for all high energy scattering processes that produce hadrons: e+ e-, p p, p anti-p, pi p, etc. and N N' (heavy-ion collisions) - as a Unruh temperature triggers here the search for the gravitational black-hole that in its near-horizon approximation better simulates this hadronic phenomenon. To identify such a black-hole we begin our gravity-gauge theory phenomenologies matching by asking the question: which black-hole behind that Rindler horizon could reproduce the experimental behavior of T_f (\sqrt{s}) in N N', where \sqrt{s} is the collision energy. Provided certain natural assumptions hold, we show that the exact string black-hole turns out to be the best candidate (as it fits the available data on T_f (\sqrt{s})) and that its limiting case, the Witten black-hole, is the unique candidate to explain the constant T_f for all elementary scattering processes at large energy. We also are able to propose an effective description of the screening of the hadronic string tension sigma(mu_b) due to the baryon density effects on T_f.
dc.description15 pages, 2 eps figures
dc.identifierhttps://arxiv.org/abs/0802.2286
dc.identifierhttp://arxiv.org/abs/0802.2286
dc.identifierPhys.Rev.D77:124034,2008
dc.identifierdoi:10.1103/PhysRevD.77.124034
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205466
dc.subjectHigh Energy Physics - Theory
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe Exact String Black-Hole behind the hadronic Rindler horizon?
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