2013
DOI: 10.1063/1.4776234
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On the non-local heat kernel expansion

Abstract: We propose a novel derivation of the non-local heat kernel expansion, first studied by Barvinsky, Vilkovisky and Avramidi, based on simple diagrammatic equations satisfied by the heat kernel. For Laplace-type differential operators we obtain the explicit form of the non-local heat kernel form factors to second order in the curvature. Our method can be generalized easily to the derivation of the non-local heat kernel expansion of a wide class of differential operators.Comment: 23 pages, 1 figure, 31 diagrams; r… Show more

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Cited by 68 publications
(104 citation statements)
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“…In two dimensions the Ricci tensor is proportional to the Ricci scalar R µν = 1 2 g µν R so there is only one non-local heat kernel structure function at the order curvature square [10] and this is given by the following linear combination:…”
Section: λmentioning
confidence: 99%
See 2 more Smart Citations
“…In two dimensions the Ricci tensor is proportional to the Ricci scalar R µν = 1 2 g µν R so there is only one non-local heat kernel structure function at the order curvature square [10] and this is given by the following linear combination:…”
Section: λmentioning
confidence: 99%
“…the beta functions are the coefficients of the expansion of the functional trace on the rhs of the flow equation. In the context of quantum gravity, the expansion of the functional trace is performed with the fundamental aid of the heat kernel expansion, in both its local and non-local realizations [10]. These techniques allow us to work covariantly at any step of the computations.…”
Section: Flow Equationsmentioning
confidence: 99%
See 1 more Smart Citation
“…Comparing (10) with the stand expansion of g µν used in perturbation theory, g µν = δ µν + √ 16πG N h µν with G N being Newton's constant, identifies the natural scale for Λ as the Planck mass m Pl = (8πG N ) −1/2 (also see [64] for a related discussion). A lengthy but in principle straightforward calculation [31,32,[60][61][62] then yields the expression for the inverse propagators of the physical fields including the full-momentum dependence…”
Section: The Spectral Action and Its Bosonic Propagatorsmentioning
confidence: 99%
“…For an alternative derivation see [25]. Keeping terms up to second order in the fields strengths, the non-local heat kernel expansion reads as follows:…”
Section: The Non-local Heat Kernel Expansionmentioning
confidence: 99%