Motic-descendant degree conjecture for Feynman amplitudes

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Let GG be a Feynman graph with hh loops in d∈2Nd\in 2\mathbb{N} space-time dimensions, and suppose that GG satisfies the weight bound conjecture for momentum-space Feynman amplitudes. A motic descendant of GG is a descendant graph in the motic graph construction, and its degree is measured in that construction.

Motic-descendant degree conjecture. The amplitude of GG is a regularised period of motic descendants of GG of degree at most dhdh.

The source presents this as a consequence expected from the weight bound conjecture combined with the stability conjecture. Its status is not resolved in the supplied text.

References

Primary source

Francis Brown, “Feynman Amplitudes and Cosmic Galois group”, arXiv:1512.06409 (2017).

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