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Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences
Evanescent operators such as the Gauss-Bonnet term have vanishing perturbative matrix elements in exactly D=4 dimensions. Similarly, evanescent fields do not propagate in D=4; a three-form field is in this class, since it is dual to a cosmological-constant contribution. In this Letter, we show that...
Autores principales: | , , , , , |
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Lenguaje: | eng |
Publicado: |
2015
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.115.211301 http://cds.cern.ch/record/2036928 |
_version_ | 1780947655134806016 |
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author | Bern, Zvi Cheung, Clifford Chi, Huan-Hang Davies, Scott Dixon, Lance Nohle, Josh |
author_facet | Bern, Zvi Cheung, Clifford Chi, Huan-Hang Davies, Scott Dixon, Lance Nohle, Josh |
author_sort | Bern, Zvi |
collection | CERN |
description | Evanescent operators such as the Gauss-Bonnet term have vanishing perturbative matrix elements in exactly D=4 dimensions. Similarly, evanescent fields do not propagate in D=4; a three-form field is in this class, since it is dual to a cosmological-constant contribution. In this Letter, we show that evanescent operators and fields modify the leading ultraviolet divergence in pure gravity. To analyze the divergence, we compute the two-loop identical-helicity four-graviton amplitude and determine the coefficient of the associated (non-evanescent) R^3 counterterm studied long ago by Goroff and Sagnotti. We compare two pairs of theories that are dual in D=4: gravity coupled to nothing or to three-form matter, and gravity coupled to zero-form or to two-form matter. Duff and van Nieuwenhuizen showed that, curiously, the one-loop conformal anomaly --- the coefficient of the Gauss-Bonnet operator --- changes under p-form duality transformations. We concur, and also find that the leading R^3 divergence changes under duality transformations. Nevertheless, in both cases the physical renormalized two-loop identical-helicity four-graviton amplitude can be chosen to respect duality. In particular, its renormalization-scale dependence is unaltered. |
id | cern-2036928 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2015 |
record_format | invenio |
spelling | cern-20369282022-08-10T13:02:29Zdoi:10.1103/PhysRevLett.115.211301http://cds.cern.ch/record/2036928engBern, ZviCheung, CliffordChi, Huan-HangDavies, ScottDixon, LanceNohle, JoshEvanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical ConsequencesParticle Physics - TheoryEvanescent operators such as the Gauss-Bonnet term have vanishing perturbative matrix elements in exactly D=4 dimensions. Similarly, evanescent fields do not propagate in D=4; a three-form field is in this class, since it is dual to a cosmological-constant contribution. In this Letter, we show that evanescent operators and fields modify the leading ultraviolet divergence in pure gravity. To analyze the divergence, we compute the two-loop identical-helicity four-graviton amplitude and determine the coefficient of the associated (non-evanescent) R^3 counterterm studied long ago by Goroff and Sagnotti. We compare two pairs of theories that are dual in D=4: gravity coupled to nothing or to three-form matter, and gravity coupled to zero-form or to two-form matter. Duff and van Nieuwenhuizen showed that, curiously, the one-loop conformal anomaly --- the coefficient of the Gauss-Bonnet operator --- changes under p-form duality transformations. We concur, and also find that the leading R^3 divergence changes under duality transformations. Nevertheless, in both cases the physical renormalized two-loop identical-helicity four-graviton amplitude can be chosen to respect duality. In particular, its renormalization-scale dependence is unaltered.arXiv:1507.06118SLAC-PUB-16332CERN-PH-TH-2015-162UCLA-15-TEP-101CALT-2015-036oai:cds.cern.ch:20369282015-07-22 |
spellingShingle | Particle Physics - Theory Bern, Zvi Cheung, Clifford Chi, Huan-Hang Davies, Scott Dixon, Lance Nohle, Josh Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences |
title | Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences |
title_full | Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences |
title_fullStr | Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences |
title_full_unstemmed | Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences |
title_short | Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences |
title_sort | evanescent effects can alter ultraviolet divergences in quantum gravity without physical consequences |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.1103/PhysRevLett.115.211301 http://cds.cern.ch/record/2036928 |
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