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摘要
En 中文
We discuss the structure of Dyson-Schwinger equations in quantum gravity and conclude in particular that all relevant skeletons are of first order in the loop number. There is an accompanying sub-Hopf algebra on gravity amplitudes equivalent to identities between n-graviton scattering amplitudes which generalize the Slavnov-Taylor identities. These identities map the infinite number of charges and finite numbers of skeletons in gravity to an infinite number of skeletons and a finite number of charges needing renormalization. Our analysis suggests that gravity, regarded as a probability conserving but perturbatively non-renormalizable theory, is renormalizable after all, thanks to the structure of its Dyson-Schwinger equations. (C) 2007 Elsevier Inc. All rights reserved.
Keyword:
gravity
renormalization
Dyson-Schwinger equations
Hopf algebra
Hochschild cohomology
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期刊
IF:
3
论文数:
5.5K
被引数:
1.8W

