A bstract We describe the formalism to compute gravitational-wave observables for compact
binaries via the effective field theory framework in combination with modern tools from …

We find that all Feynman integrals (FIs), having any number of loops, can be completely
determined once linear relations between FIs are provided. Therefore, FI computation is …

We compute the three-loop nonsinglet corrections to the photon-quark form factors taking
into account the full dependence on the virtuality of the photon and the quark mass. We …

We consider quantum chromodynamics with external vector, axial-vector, scalar, and
pseudoscalar currents and compute three-loop corrections to the corresponding vertex …

Working within the post-Newtonian (PN) approximation to general relativity, we use the
effective field theory (EFT) framework to study the conservative dynamics of the two-body …

A recently introduced approach to the classical gravitational dynamics of binary systems
involves intricate integrals (linked to a combination of nonlocal-in-time interactions with …

A recently introduced approach to the gravitational dynamics of binary systems involves
intricate integrals, linked to nonlocal-in-time interactions arising at the 5-loop level of …

We present the bare one-, two-, and three-loop form factors in massless quantum
chromodynamics as linear combinations of finite master integrals. Using symbolic …

We revisit several aspects of the interaction of self-gravitating, slowly varying sources with
their own emitted radiation within the context of post-Newtonian approximation to General …

A bstract Extending an argument of [1] for the case of 5-loop massless propagators we prove
a host of new exact model-independent relations between contributions proportional to odd …