Classical Effective Field Theory and Caged Black Holes
Barak Kol, Michael Smolkin

TL;DR
This paper connects matched asymptotic expansion with Classical Effective Field Theory to analyze caged black holes, simplifying calculations and revealing new insights into their thermodynamics and renormalization properties.
Contribution
It demonstrates the equivalence between matched asymptotic expansion and CLEFT, introduces diagrammatic methods, and computes higher-loop corrections for caged black holes.
Findings
Simplified the computation of thermodynamic quantities for caged black holes.
Replaced multiple two-loop diagrams with a single diagram, reducing complexity.
Found that angular momentum does not renormalize at leading order.
Abstract
Matched asymptotic expansion is a useful technique in General Relativity and other fields whenever interaction takes place between physics at two different length scales. Here matched asymptotic expansion is argued to be equivalent quite generally to Classical Effective Field Theory (CLEFT) where one (or more) of the zones is replaced by an effective theory whose terms are organized in order of increasing irrelevancy, as demonstrated by Goldberger and Rothstein in a certain gravitational context. The CLEFT perspective has advantages as the procedure is clearer, it allows a representation via Feynman diagrams, and divergences can be regularized and renormalized in standard field theoretic methods. As a side product we obtain a wide class of classical examples of regularization and renormalization, concepts which are usually associated with Quantum Field Theories. We demonstrate these…
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