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Graviton Scattering and a Sum Rule for the c Anomaly in 4D CFT

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arxiv 1801.05807 v2 pith:DNSEROSC submitted 2018-01-17 hep-th

classification hep-th
keywords rulecoefficientstermsanomalyboundcftscoefficientcorrelation
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abstract

4D CFTs have a scale anomaly characterized by the coefficient $c$, which appears as the coefficient of logarithmic terms in momentum space correlation functions of the energy-momentum tensor. By studying the CFT contribution to 4-point graviton scattering amplitudes in Minkowski space we derive a sum rule for $c$ in terms of $TT\mathcal{O}$ OPE coefficients. The sum rule can be thought of as a version of the optical theorem, and its validity depends on the existence of the massless and forward limits of the $\langle TTTT \rangle$ correlation functions that contribute. The finiteness of these limits is checked explicitly for free scalar, fermion, and vector CFTs. The sum rule gives $c$ as a sum of positive terms, and therefore implies a lower bound on $c$ given any lower bound on $TT\mathcal{O}$ OPE coefficients. We compute the coefficients to the sum rule for arbitrary operators of spin 0 and 2, including the energy-momentum tensor.

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Cited by 2 Pith papers

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  1. Conformal 3-point functions and the Lorentzian OPE in momentum space

    hep-th 2019-09 conditional novelty 7.0 of 10

    The paper derives a closed Appell F4 expression for the Wightman 3-point function of scalar operators and for two scalars with one traceless symmetric tensor in Lorentzian momentum space.

  2. The Speed of Gravity

    hep-th 2019-09 conditional novelty 6.0 of 10

    In the standard effective field theory of gravity, gravitational waves on cosmological backgrounds propagate at a speed differing from unity, and analyticity arguments favor superluminal speed relative to matter.

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