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Unified limiting form of graviton radiation at extreme energies

We derive the limiting form of graviton radiation in gravitational scattering at transplanckian energies ($E\gg M_P$) and small deflection angles. We show that --- owing to the graviton's spin 2 --- such limiting form unifies the soft- and Regge- regimes of emission, by covering a broad angular...

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Autores principales: Ciafaloni, Marcello, Colferai, Dimitri, Coradeschi, Francesco, Veneziano, Gabriele
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.93.044052
http://cds.cern.ch/record/2110525
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author Ciafaloni, Marcello
Colferai, Dimitri
Coradeschi, Francesco
Veneziano, Gabriele
author_facet Ciafaloni, Marcello
Colferai, Dimitri
Coradeschi, Francesco
Veneziano, Gabriele
author_sort Ciafaloni, Marcello
collection CERN
description We derive the limiting form of graviton radiation in gravitational scattering at transplanckian energies ($E\gg M_P$) and small deflection angles. We show that --- owing to the graviton's spin 2 --- such limiting form unifies the soft- and Regge- regimes of emission, by covering a broad angular range, from forward fragmentation to deeply central region. The single-exchange emission amplitudes have a nice expression in terms of the transformation phases of helicity amplitudes under rotations. As a result, the multiple-exchange emission amplitudes can be resummed via an impact parameter $b$-space factorization theorem that takes into account all coherence effects. We then see the emergence of an energy spectrum of the emitted radiation which, being tuned on $\hbar/R \sim M_P^2/E \ll M_P$, is reminiscent of Hawking's radiation. Such a spectrum is much softer than the one na\"ively expected for increasing input energies and neatly solves a potential energy crisis. Furthermore, by including rescattering corrections in the (quantum) factorization formula, we are able to recover the classical limit and to find the corresponding quantum corrections. Perspectives for the extrapolation of such limiting radiation towards the classical collapse regime (where $b$ is of the order of the gravitational radius $R$) are also discussed.
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institution Organización Europea para la Investigación Nuclear
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publishDate 2015
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spelling cern-21105252023-03-14T17:20:21Zdoi:10.1103/PhysRevD.93.044052http://cds.cern.ch/record/2110525engCiafaloni, MarcelloColferai, DimitriCoradeschi, FrancescoVeneziano, GabrieleUnified limiting form of graviton radiation at extreme energiesParticle Physics - TheoryWe derive the limiting form of graviton radiation in gravitational scattering at transplanckian energies ($E\gg M_P$) and small deflection angles. We show that --- owing to the graviton's spin 2 --- such limiting form unifies the soft- and Regge- regimes of emission, by covering a broad angular range, from forward fragmentation to deeply central region. The single-exchange emission amplitudes have a nice expression in terms of the transformation phases of helicity amplitudes under rotations. As a result, the multiple-exchange emission amplitudes can be resummed via an impact parameter $b$-space factorization theorem that takes into account all coherence effects. We then see the emergence of an energy spectrum of the emitted radiation which, being tuned on $\hbar/R \sim M_P^2/E \ll M_P$, is reminiscent of Hawking's radiation. Such a spectrum is much softer than the one na\"ively expected for increasing input energies and neatly solves a potential energy crisis. Furthermore, by including rescattering corrections in the (quantum) factorization formula, we are able to recover the classical limit and to find the corresponding quantum corrections. Perspectives for the extrapolation of such limiting radiation towards the classical collapse regime (where $b$ is of the order of the gravitational radius $R$) are also discussed.We derive the limiting form of graviton radiation in gravitational scattering at trans-Planckian energies (E≫MP) and small deflection angles. We show that—owing to the graviton’s spin 2—such a limiting form unifies the soft and Regge regimes of emission, by covering a broad angular range, from forward fragmentation to the deeply central region. The single-exchange emission amplitudes have a nice expression in terms of the transformation phases of helicity amplitudes under rotations. As a result, the multiple-exchange emission amplitudes can be resummed via an impact parameter b-space factorization theorem that takes into account all coherence effects. We then see the emergence of an energy spectrum of the emitted radiation which, being tuned on ℏ/R∼MP2/E≪MP, is reminiscent of Hawking’s radiation. Such a spectrum is much softer than the one naïvely expected for increasing input energies and neatly solves a potential energy crisis. Furthermore, by including rescattering corrections in the (quantum) factorization formula, we are able to recover the classical limit and find the corresponding quantum corrections. Perspectives for the extrapolation of such limiting radiation towards the classical collapse regime (where b is of the order of the gravitational radius R) are also discussed.We derive the limiting form of graviton radiation in gravitational scattering at transplanckian energies ($E\gg M_P$) and small deflection angles. We show that --- owing to the graviton's spin 2 --- such limiting form unifies the soft- and Regge- regimes of emission, by covering a broad angular range, from forward fragmentation to deeply central region. The single-exchange emission amplitudes have a nice expression in terms of the transformation phases of helicity amplitudes under rotations. As a result, the multiple-exchange emission amplitudes can be resummed via an impact parameter $b$-space factorization theorem that takes into account all coherence effects. We then see the emergence of an energy spectrum of the emitted radiation which, being tuned on $\hbar/R \sim M_P^2/E \ll M_P$, is reminiscent of Hawking's radiation. Such a spectrum is much softer than the one na\"ively expected for increasing input energies and neatly solves a potential energy crisis. Furthermore, by including rescattering corrections in the (quantum) factorization formula, we are able to recover the classical limit and to find the corresponding quantum corrections. Perspectives for the extrapolation of such limiting radiation towards the classical collapse regime (where $b$ is of the order of the gravitational radius $R$) are also discussed.arXiv:1512.00281CERN-PH-TH-2015-272CERN-PH-TH-2015-272oai:cds.cern.ch:21105252015-12-01
spellingShingle Particle Physics - Theory
Ciafaloni, Marcello
Colferai, Dimitri
Coradeschi, Francesco
Veneziano, Gabriele
Unified limiting form of graviton radiation at extreme energies
title Unified limiting form of graviton radiation at extreme energies
title_full Unified limiting form of graviton radiation at extreme energies
title_fullStr Unified limiting form of graviton radiation at extreme energies
title_full_unstemmed Unified limiting form of graviton radiation at extreme energies
title_short Unified limiting form of graviton radiation at extreme energies
title_sort unified limiting form of graviton radiation at extreme energies
topic Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.93.044052
http://cds.cern.ch/record/2110525
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AT venezianogabriele unifiedlimitingformofgravitonradiationatextremeenergies