Abstract
We present a calculation of at next-to-leading order including the effect of a finite top mass. Where possible we include the complete dependence on . This includes the leading order amplitude, the infrared poles of the two-loop amplitude and the real radiation amplitude. The remaining finite piece of the virtual correction is considered in an asymptotic expansion in , which is accurate to . By successively including more -exact pieces, the dependence on the asymptotic series diminishes and we find convergent behavior for for the first time. Our results justify rescaling by the -exact leading-order (LO) cross section to model top-mass effects in effective field theory results up to of 250 to 300 GeV. We show that the error made by using the LO rescaling becomes comparable to the next-to-next-to-leading-order scale uncertainty for such large energies. We implement our results into the Monte Carlo code mcfm.
3 More- Received 13 September 2016
DOI:https://doi.org/10.1103/PhysRevD.95.014004
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