activity
20162026
most citedKira - A Feynman Integral Reduction Program

417 citations · 1.3k across the 27 of their papers we have counts for

collaborators

29 papers

hep-ph2026

Third-order mixed electroweak-QCD corrections to the W-boson mass prediction from the muon lifetime

Ievgen Dubovyk, Ayres Freitas, Janusz Gluza +1

We present the calculation of the so far missing corrections to the quantity , which relates the Fermi constant to the W-boson mass, and enables pre…

hep-th2026★ 1 cited

Conservative Black Hole Scattering at Fifth Post-Minkowskian and Second Self-Force Order

Mathias Driesse, Gustav Uhre Jakobsen, Gustav Mogull +4

Using the worldline quantum field theory formalism, we compute conservative contributions to the scattering angle and impulse for classical black hole scattering at fifth post-Mink…

hep-ph2025

Kira 3: integral reduction with efficient seeding and optimized equation selection

Fabian Lange, Johann Usovitsch, Zihao Wu

We present version 3 of Kira, a Feynman integral reduction program for high-precision calculations in quantum field theory and gravitational-wave physics. Building on previous vers…

hep-ph2025

Performing integration-by-parts reductions using NeatIBP 1.1 + Kira

Zihao Wu, Janko Böhm, Rourou Ma +3

We introduce a new version v1.1 of NeatIBP. In this new version, a Kira interface is included. It allows the user to reduce the integration-by-parts (IBP) identity systems generate…

hep-ph2024

Planar Six-Point Feynman Integrals for Four-Dimensional Gauge Theories

Samuel Abreu, Pier Francesco Monni, Ben Page +1

We compute all planar two-loop six-point Feynman integrals entering scattering observables in massless gauge theories such as QCD. A central result of this paper is the formulation…

hep-th2024★ 72 cited

Emergence of Calabi-Yau manifolds in high-precision black hole scattering

Mathias Driesse, Gustav Uhre Jakobsen, Albrecht Klemm +5

Using the worldline quantum field theory formalism, we compute the radiation-reacted impulse, scattering angle, radiated energy and recoil of a classical black hole (or neutron sta…