The unequal mass sunrise integral expressed through iterated integrals on M1,3
Abstract
We solve the two-loop sunrise integral with unequal masses systematically to all orders in the dimensional regularisation parameter . In order to do so, we transform the system of differential equations for the master integrals to an -form. The sunrise integral with unequal masses depends on three kinematical variables. We perform a change of variables to standard coordinates on the moduli space M1,3 of a genus one Riemann surface with three marked points. This gives us the solution as iterated integrals on M1,3. On the hypersurface τ=const our result reduces to elliptic polylogarithms. In the equal mass case our result reduces to iterated integrals of modular forms.
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.