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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...
Autores principales: | , , , |
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Lenguaje: | eng |
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2015
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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. |
id | cern-2110525 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2015 |
record_format | invenio |
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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