Review of NNLO and subtraction
Frank Petriello
Resummation and Parton Showers, IPPP July 17, 2013
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Review of NNLO and subtraction Frank Petriello Resummation and - - PowerPoint PPT Presentation
Review of NNLO and subtraction Frank Petriello Resummation and Parton Showers, IPPP July 17, 2013 1 Outline Will attempt to motivate the necessity of NNLO in the presence of advanced FO+PS and resummation tools The major bottleneck is
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Anastasiou, Dixon, Melnikov, FP 2004
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from de Florian, Higgs Magnificent Mile 2012
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H+1-jet
Banfi, Monni, Salam, Zanderighi 2012 Need NNLO H+jet! Need NNLO H+jet!
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SHERPA, 2011
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Acceptance
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counterterms but only after phase space integration for real radiations
differential observables
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1996), FKS subtraction (Frixione, Kunszt, Signer 1996)
Approximates real-emission matrix elements in all singular limits so this difference is numerically integrable Simple enough to integrate analytically so that 1/ε poles can be cancelled against virtual corrections
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Czakon, Fiedler, Mitov (2013) Gehrmann-de Ridder, Gehrmann, Glover, Pires (2013) Boughezal, Caola, Melnikov, FP , Schulze (2013)
dijet: gg-channel H+1j:gg-channel ttbar: all-channels
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Czakon, Fiedler, Mitov (2013) Gehrmann-de Ridder, Gehrmann, Glover, Pires (2013) Boughezal, Caola, Melnikov, FP , Schulze (2013)
dijet: gg-channel H+1j:gg-channel ttbar: all-channels
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from T. Gehrmann
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|M(. . . , p1, p1, p3)|2 ≈ 4g4
s
s2
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Mµ(. . . , p1 + p2 + p3)Mν∗(. . . , p1 + p2 + p3) P µν
g1g2g3 Catani, Grazzini 1999
zi=Ei/(∑Ej)
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|M(. . . , p1, p1, p3)|2 ≈ 4g4
s
s2
123
Mµ(. . . , p1 + p2 + p3)Mν∗(. . . , p1 + p2 + p3) P µν
g1g2g3
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x y x y
x y y x
Binoth, Heinrich; Anastasiou, Melnikov, FP 2003-2005
y−1−✏ = −(y) ✏ + 1 y
− ✏ ln y y
+ O(✏2)
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Melnikov, FP 2011). Retains the features of the QCD computation, but makes
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s-12 ~ ξ1(Aη1+Bξ2η2+Cξ1ξ2(η1-η2)2)
s-12 ~ ξ1η2(Aη1+Bξ2+Cξ1ξ2η2(1-η1)2)
Bracket is finite in all limits All singularities extracted as overall multiplicative factors
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regular functions of xi
with and Let’s look at some of the singularities that can occur
expandable in plus distributions
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E1 = E2 = 0 double soft limit the QED matrix element factorizes completely, use known singular limits with derive the following formula easy to calculate numerically
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E2 = 0 & p1 || p_ soft-collinear limit The matrix element factorizes in two steps: derive the following formula easy to calculate numerically collinear factorization of ϒ1 soft factorization of ϒ2
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from Czakon, 2010
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energy variable angular variable must keep track of the different fractional powers which can appear, to properly expand in plus distributions
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sL4 + α2 sL3 + α2 sL2 + α2 sL + α2 s
sL6 + α3 sL5 + α3 sL4 + α3 sL3 + α3 sL2 + . . .
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