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Low-energy scattering of extremal black holes by neutral matter

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Low-energy scattering of extremal black holes by neutral matter

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dc.contributor.author Fabbri, Alessandro
dc.contributor.author Navarro Sanz, Diego José
dc.contributor.author Navarro Salas, José
dc.date.accessioned 2014-03-21T12:24:30Z
dc.date.available 2014-03-21T12:24:30Z
dc.date.issued 2002
dc.identifier.citation Fabbri, A. Navarro Sanz, Diego José Navarro Salas, José 2002 Low-energy scattering of extremal black holes by neutral matter Nuclear Physics B 628 1-2 361 374
dc.identifier.uri http://hdl.handle.net/10550/33651
dc.description.abstract We investigate the decay of a spherically symmetric near-extremal charged black hole, including back-reaction effects, in the near-horizon region. The non-locality of the effective action controlling this process allows and also forces us to introduce a complementary set of boundary conditions which permit to determine the asymptotic late time Hawking flux. The evaporation rate goes down exponentially and admits an infinite series expansion in Planck's constant. At leading order it is proportional to the total mass and the higher order terms involve higher order momenta of the classical stress-tensor. Moreover we use this late time behaviour to go beyond the near-horizon approximation and comment on the implications for the information loss paradox.
dc.relation.ispartof Nuclear Physics B, 2002, vol. 628, num. 1-2, p. 361-374
dc.subject Simetria (Física)
dc.subject Física nuclear
dc.title Low-energy scattering of extremal black holes by neutral matter
dc.type journal article es_ES
dc.date.updated 2014-03-21T12:24:30Z
dc.identifier.doi 10.1016/S0550-3213(02)00135-9
dc.identifier.idgrec 035531
dc.rights.accessRights open access es_ES
dc.identifier.url 10.1016/S0550-3213(02)00135-9

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