2 WILLIAM DALLAWAY AND KAREN YEATS
An algebraic and combinatorial approach to the relationship between the cut
structure and subdivergence structure of Feynman diagrams was recently devel-
oped by one of us along with Dirk Kreimer [31]. The cut structure of a Feynman
diagram controls its monodromy around singularities and is related to its infrared
behaviour while the subdivergence structure controls its behaviour under renormal-
ization. However, the set up of [31] required fixing a spanning tree, as motivated by
connections to Cullen and Vogtmann’s Outerspace [16, 5, 29], something which is
unnecessary and at times cumbersome. We rectify this here with a tree-independent
formulation and then look at some of the combinatorial preliminaries necessary for
extending Klann’s calculations [26] on how the cut structure relates to the infrared
divergences.
The basis of all of this are the renormalization Hopf algebras first developed
by Connes and Kreimer and first we will give a brief account of this. We then
present the differential equations which will be the main focus of the analysis.
The remainder of the introduction considers extensions of the Hopf algebras and a
coaction studied in [31].
For a mathematical reader uninterested in the physics background, the key things
are the differential equations (1.1), (1.2) along with a general sense that there is
some motivation to studying them and especially to studying when solutions exist
for all xand all L, and the core and cut coproducts on graphs Definition 1.7 and
(1.3), and (1.4), along with a general sense that the relationship between them is
meaningful. Everything else in this introduction is motivation.
1.1. Feynman diagrams and renormalization Hopf algebras. Quantum field
theory is a framework in which we can understand arbitrary numbers of interacting
particles quantum mechanically. It is the standard way to unify quantum mechanics
and special relativity. In high energy physics, a prototypical experiment consists of
generating known particles, colliding them together at high energy, and investigat-
ing the particles that appear as a result. On the theoretical and mathematical side
of high energy physics, then, we want to better understand the mathematical struc-
tures in quantum field theory so as to be able to better calculate the probability
amplitudes of particle interactions as occur in such a collider experiment.
One longstanding but still important technique for computing these amplitudes
is the loop expansion in Feynman diagram. In this approach amplitudes are com-
puted and studied as given by an infinite series indexed by Feynman diagrams. Very
roughly Feynman diagrams are graphs where the edges represent particles propagat-
ing and the vertices represent particle interactions. Each graph contributes to the
amplitude via its Feynman integral, an integral which can be read off of the graph.
Particles entering or exiting are represented as unpaired half-edges in the graph.
The loop number of the graph is the dimension of the cycle space of the graph, and
in the loop expansion of an amplitude, the series is organized by increasing number
of loops.
Formally we will define graphs as follows.
Definition 1.1. Agraph Gconsists of
•a set H(G) of the half edges of the graph,
•a set partition, V(G), of H(G) into parts of size at least 3, the parts of
which are the vertices of the graph, and