2018
DOI: 10.1007/s11005-018-1114-8
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Feynman integral relations from parametric annihilators

Abstract: We study shift relations between Feynman integrals via the Mellin transform through parametric annihilation operators. These contain the momentum space integration by parts relations, which are well-known in the physics literature. Applying a result of Loeser and Sabbah, we conclude that the number of master integrals is computed by the Euler characteristic of the Lee-Pomeransky polynomial. We illustrate techniques to compute this Euler characteristic in various examples and compare it with numbers of master i… Show more

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Cited by 84 publications
(104 citation statements)
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“…Proof. (A proof can be found also in [6]) Since U is homogeneous of degree L and F is homogeneous of degree L + 1, the integral in (1.5) as a function of d converges in the strip…”
Section: Remarkmentioning
confidence: 88%
“…Proof. (A proof can be found also in [6]) Since U is homogeneous of degree L and F is homogeneous of degree L + 1, the integral in (1.5) as a function of d converges in the strip…”
Section: Remarkmentioning
confidence: 88%
“…In some instances, we also found it useful to apply syzygy technology [59][60][61][62][63]. For the basis change to finite integrals, we made heavy use of first-and second-order annihilators [64,65] in the Lee-Pomeransky representation [66]. Instead of resorting to computer algebra systems, we compute syzygies with linear algebra [60,67] using Finred as a linear solver.…”
Section: Setup and Integral Reductionmentioning
confidence: 99%
“…where C × := C−{0}, in agreement with [31,78]. Physically it counts the number of linearlyindependent Feynman integrals that involve the set of propagators {D a } P a=1 over Q(K, ε, δ a ), where K in the set of kinematic variables appearing in Q, L, c. 4 It is the most convenient to compute |χ(M )| by invoking Morse-theory arguments, which for sufficiently generic W imply that it is equal to the number of critical points Crit(W ) determined by the condition dW = 0.…”
Section: )mentioning
confidence: 90%
“…The moduli space of metrics on the sunrise graph, M Gsun := (C × ) 3 − {G = 0}, has Euler characteristic |χ(M Gsun )| = 7 according to Macaulay2 [97], in agreement with [78,103].…”
Section: Example Ii: Two-loop Massive Sunrisementioning
confidence: 99%