Ultraviolet Properties of N = 8 Supergravity at Five Loops
Zvi Bern, John Joseph Carrasco, Wei-Ming Chen, Alex Edison, Henrik Johansson, Julio Parra-Martinez, Radu Roiban, Mao Zeng
TL;DR
The paper determines the five-loop ultraviolet behavior of N=8 supergravity, showing that the first divergence occurs in D_c = 24/5 and corresponds to a D^8 R^4 counterterm, with no evidence of enhanced cancellations at this order. It achieves this by constructing an improved five-loop integrand through a generalized double-copy, performing a vacuum-expansion of the integrand, and executing a full IBP reduction organized by an SL(5) symmetry to extract the UV pole. A striking outcome is that the leading UV contributions can be expressed entirely in terms of a small set of vacuum master integrals with coefficients dictated by diagram automorphisms, and that cross-loop consistency relations tie higher-loop divergences to lower-loop vacuum structures. These patterns not only validate the five-loop result but also suggest powerful avenues for simplifying higher-loop calculations and understanding the ultraviolet structure of maximal supergravity in four dimensions.
Abstract
We use the recently developed generalized double-copy construction to obtain an improved representation of the five-loop four-point integrand of $N = 8$ supergravity whose leading ultraviolet behavior we analyze using state of the art loop-integral expansion and reduction methods. We find that the five-loop critical dimension where ultraviolet divergences first occur is $D_c=24/5$, corresponding to a $D^8 R^4$ counterterm. This ultraviolet behavior stands in contrast to the cases of four-dimensional $N = 4$ supergravity at three loops and $N = 5$ supergravity at four loops whose improved ultraviolet behavior demonstrates enhanced cancellations beyond implications from standard-symmetry considerations. We express this $D_c=24/5$ divergence in terms of two relatively simple positive-definite integrals reminiscent of vacuum integrals, excluding any additional ultraviolet cancellations at this loop-order. We note nontrivial relations between the integrals describing this leading ultraviolet behavior and integrals describing lower-loop behavior. This observation suggests not only a path towards greatly simplifying future calculations at higher loops, but may even allow us to directly investigate ultraviolet behavior in terms of simplified integrals, avoiding the construction of complete integrands.
