Content area
Abstract
Functional Renormalization Group Equations constitute a powerful tool to encode the perturbative and non-perturbative properties of a physical system. We present an algorithm to systematically compute the expansion of such flow equations in a given background quantity specified by the approximation scheme. The method is based on off-diagonal heat-kernel techniques and can be implemented on a computer algebra system, opening access to complex computations in, e.g., Gravity or Yang-Mills theory. In a first illustrative example, we re-derive the gravitational β-functions of the Einstein-Hilbert truncation, demonstrating their background-independence. As an additional result, the heat-kernel coefficients for transverse vectors and transverse-traceless symmetric matrices are computed to second order in the curvature.
Details
1 Albert Einstein Institute, Max Planck Institute for Gravitational Physics, Potsdam, Germany (GRID:grid.450243.4) (ISNI:0000000107904262)
2 University of Mainz, Institute of Physics, Mainz, Germany (GRID:grid.5802.f) (ISNI:0000000119417111)
3 University of Cambridge, Department of Genetics, Cambridge, U.K. (GRID:grid.5335.0) (ISNI:0000000121885934)




