Large curvature and background scale independence in single-metric approximations to asymptotic safety
Large curvature and background scale independence in single-metric approximations to asymptotic safety
In single-metric approximations to the exact renormalization group (RG) for quantum gravity, it has been not been clear how to treat the large curvature domain beyond the point where the effective cutoff scale k is less than the lowest eigenvalue of the appropriate modified Laplacian. We explain why this puzzle arises from background dependence, resulting in Wilsonian RG concepts being inapplicable. We show that when properly formulated over an ensemble of backgrounds, the Wilsonian RG can be restored. This in turn implies that solutions should be smooth and well defined no matter how large the curvature is taken. Even for the standard single-metric type approximation schemes, this construction can be rigorously derived by imposing a modified Ward identity (mWI) corresponding to rescaling the background metric by a constant factor. However compatibility in this approximation requires the space-time dimension to be six. Solving the mWI and flow equation simultaneously, new variables are then derived that are independent of overall background scale.
Morris, Tim R.
a9927d31-7a12-4188-bc35-1c9d3a03a6a6
November 2016
Morris, Tim R.
a9927d31-7a12-4188-bc35-1c9d3a03a6a6
Morris, Tim R.
(2016)
Large curvature and background scale independence in single-metric approximations to asymptotic safety.
Journal of High Energy Physics, 2016 (11), [160].
(doi:10.1007/JHEP11(2016)160).
Abstract
In single-metric approximations to the exact renormalization group (RG) for quantum gravity, it has been not been clear how to treat the large curvature domain beyond the point where the effective cutoff scale k is less than the lowest eigenvalue of the appropriate modified Laplacian. We explain why this puzzle arises from background dependence, resulting in Wilsonian RG concepts being inapplicable. We show that when properly formulated over an ensemble of backgrounds, the Wilsonian RG can be restored. This in turn implies that solutions should be smooth and well defined no matter how large the curvature is taken. Even for the standard single-metric type approximation schemes, this construction can be rigorously derived by imposing a modified Ward identity (mWI) corresponding to rescaling the background metric by a constant factor. However compatibility in this approximation requires the space-time dimension to be six. Solving the mWI and flow equation simultaneously, new variables are then derived that are independent of overall background scale.
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Accepted/In Press date: 22 November 2016
e-pub ahead of print date: 25 November 2016
Published date: November 2016
Organisations:
Theoretical Partical Physics Group
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Local EPrints ID: 403359
URI: http://eprints.soton.ac.uk/id/eprint/403359
PURE UUID: 84cb776d-9e52-44c1-9f0a-9a7a67427791
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Date deposited: 30 Nov 2016 11:46
Last modified: 16 Mar 2024 02:36
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