Strings in Horizons, Dissipation and a Possible Interpretation of the Hagedorn Temperature

Simple item page
dc.creatorAbdalla, M. C. Batoni
dc.creatorCantcheff, M. Botta
dc.creatorNedel, D. L.
dc.date2007-03-07
dc.date2007-12-28
dc.date.accessioned2026-07-07T11:23:42Z
dc.date.available2026-07-07T11:23:42Z
dc.descriptionWe consider the entanglement of closed bosonic strings intersecting the event horizon of a Rindler spacetime and, by using some simplified (rather semiclassical) arguments and some elements of the string field theory, we show the existence of a critical temperature beyond which closed strings \emph{cannot be in thermal equilibrium}. The order of magnitude of this critical value coincides with the Hagedorn temperature, which suggests an interpretation consistent with the fact of having a partition function which is bad defined for temperatures higher than it. Possible implications of the present approach on the microscopical structure of stretched horizons are also pointed out.
dc.descriptionA detailed description of string boundary states in a Rindler horizon was added, and their relation with the stretched horizon microscopic structure was emphasized. References added. To appear in Eur. Phys. J. C
dc.identifierhttps://arxiv.org/abs/hep-th/0703064
dc.identifierhttp://arxiv.org/abs/hep-th/0703064
dc.identifierEur.Phys.J.C54:311-317,2008
dc.identifierdoi:10.1140/epjc/s10052-007-0513-2
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194983
dc.subjectHigh Energy Physics - Theory
dc.titleStrings in Horizons, Dissipation and a Possible Interpretation of the Hagedorn Temperature
dc.typetext

Files

Collections

arXiv