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Holography for the Trace Anomaly Action
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abstract
A recently proposed effective action for the trace anomaly describes a tensor-scalar theory that is weakly coupled up to a certain high energy scale, where it becomes strongly interacting. Its ultraviolet completion is obtained by coupling to gravity a quantum field theory in which conformal invariance is spontaneously broken. In this paper, we show that if the field theory that gives rise to the trace anomaly is a large $N_c$ conformal field theory, then the trace anomaly action has a completion above the strong scale in a holographic Randall-Sundrum two-brane theory, with the radion as a low energy remnant of the spontaneously broken conformal symmetry. Furthermore, we note that the sub-leading $N_c$ terms can be derived by adding localized fields to the UV brane, so that the theory remains weakly coupled. The sub-leading terms are also obtained by introducing the Weyl squared terms in the 5D bulk. These, however, exhibit strongly coupled behavior at the respective sub-Planckian energy scales.
Forward citations
Cited by 3 Pith papers
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Inflation with the Trace Anomaly Action and Primordial Black Holes
In the trace anomaly effective theory, the anomalyon's curvature perturbation has a power spectrum growing as k^2, which can seed primordial black holes on short scales.
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Weakly-Coupled Trace Anomaly Action for Gravity
The trace anomaly effective action for gravity is not a valid low-energy EFT unless a new sector with spontaneously broken scale invariance adds a kinetic term for the anomalyon scalar.
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Massive Gravity @ 15
A status review arguing that ghost-free massive gravity remains a theoretically consistent and phenomenologically viable infrared modification of General Relativity, with open UV questions.
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