Wilson loops and amplitudes in N=4 Super Yang-Mills

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1 Wilson loops and amplitudes in N=4 Super Yang-Mills Vittorio Del Duca INFN LNF TH-LPCC CERN 8 August 2011

2 N=4 Super Yang-Mills maximal supersymmetric theory (without gravity) conformally invariant, β fn. = 0 spin 1 gluon 4 spin 1/2 gluinos 6 spin 0 real scalars

3 N=4 Super Yang-Mills maximal supersymmetric theory (without gravity) conformally invariant, β fn. = 0 spin 1 gluon 4 spin 1/2 gluinos 6 spin 0 real scalars t Hooft limit: Nc with λ = g 2 Nc fixed only planar diagrams

4 N=4 Super Yang-Mills maximal supersymmetric theory (without gravity) conformally invariant, β fn. = 0 spin 1 gluon 4 spin 1/2 gluinos 6 spin 0 real scalars t Hooft limit: Nc with λ = g 2 Nc fixed only planar diagrams AdS/CFT duality Maldacena 97 large-λ limit of 4dim CFT weakly-coupled string theory (aka weak-strong duality)

5 AdS/CFT duality, amplitudes & Wilson loops planar scattering amplitude at strong coupling Alday Maldacena 07 M exp [ i ] λ 2π (Area) cl area of string world-sheet ( classical solution ) neglect O(1/ λ) corrections

6 AdS/CFT duality, amplitudes & Wilson loops planar scattering amplitude at strong coupling Alday Maldacena 07 M exp [ i ] λ 2π (Area) cl area of string world-sheet ( classical solution ) neglect O(1/ λ) corrections amplitude has same form as ansatz for MHV amplitudes at weak coupling M n = M (0) n exp [ l=1 ( ) ] a l f (l) (ɛ) m (1) n (lɛ)+const (l) + E n (l) (ɛ)

7 AdS/CFT duality, amplitudes & Wilson loops planar scattering amplitude at strong coupling Alday Maldacena 07 M exp [ i ] λ 2π (Area) cl area of string world-sheet ( classical solution ) neglect O(1/ λ) corrections amplitude has same form as ansatz for MHV amplitudes at weak coupling M n = M (0) n exp [ l=1 ( ) ] a l f (l) (ɛ) m (1) n (lɛ)+const (l) + E n (l) (ɛ) computation ``formally the same as... the expectation value of a Wilson loop given by a sequence of light-like segments

8 MHV amplitudes in planar N=4 SYM at any order in the coupling, colour-ordered MHV amplitude in N=4 SYM can be written as tree-level amplitude times helicity-free loop coefficient M n (L) = M n (0) m (L) n

9 MHV amplitudes in planar N=4 SYM at any order in the coupling, colour-ordered MHV amplitude in N=4 SYM can be written as tree-level amplitude times helicity-free loop coefficient M n (L) = M n (0) m (L) n at 1 loop m (1) n = pq F 2me (p, q, P, Q) n 6

10 MHV amplitudes in planar N=4 SYM at any order in the coupling, colour-ordered MHV amplitude in N=4 SYM can be written as tree-level amplitude times helicity-free loop coefficient M n (L) = M n (0) m (L) n at 1 loop m (1) n = pq F 2me (p, q, P, Q) n 6 at 2 loops, iteration formula for the n-pt amplitude m (2) n (ɛ) = 1 2 [ m (1) n ] 2 (ɛ) + f (2) (ɛ) m (1) (2ɛ)+Const (2) + R n Anastasiou Bern Dixon Kosower 03

11 MHV amplitudes in planar N=4 SYM at any order in the coupling, colour-ordered MHV amplitude in N=4 SYM can be written as tree-level amplitude times helicity-free loop coefficient M n (L) = M n (0) m (L) n at 1 loop m (1) n = pq F 2me (p, q, P, Q) n 6 at 2 loops, iteration formula for the n-pt amplitude m (2) n (ɛ) = 1 2 [ m (1) n ] 2 (ɛ) + f (2) (ɛ) m (1) (2ɛ)+Const (2) + R at all loops, ansatz for a resummed exponent n Anastasiou Bern Dixon Kosower 03 m (L) n = exp [ l=1 ( a l f (l) (ɛ) m (1) n (lɛ)+const (l) + E n (ɛ)) ] (l) + R Bern Dixon Smirnov 05

12 MHV amplitudes in planar N=4 SYM at any order in the coupling, colour-ordered MHV amplitude in N=4 SYM can be written as tree-level amplitude times helicity-free loop coefficient M n (L) = M n (0) m (L) n at 1 loop m (1) n = pq F 2me (p, q, P, Q) n 6 at 2 loops, iteration formula for the n-pt amplitude m (2) n (ɛ) = 1 2 [ m (1) n ] 2 (ɛ) + f (2) (ɛ) m (1) (2ɛ)+Const (2) + R at all loops, ansatz for a resummed exponent n remainder function Anastasiou Bern Dixon Kosower 03 m (L) n = exp [ l=1 ( a l f (l) (ɛ) m (1) n (lɛ)+const (l) + E n (ɛ)) ] (l) + R Bern Dixon Smirnov 05

13 ansatz for MHV amplitudes in planar N=4 SYM M n = M (0) n = M (0) n coupling a = [ 1+ exp L=1 [ l=1 λ 8π 2 (4πe γ ) ɛ a L m (L) n (ɛ) ] ( ) ] a l f (l) (ɛ)m (1) n (lɛ)+const (l) + E n (l) (ɛ) λ = g 2 N Bern Dixon Smirnov 05 t Hooft parameter f (l) (ɛ) = ˆγ(l) K 4 + ɛ l 2 Ĝ(l) + ɛ 2 f (l) 2 E (l) n (ɛ) =O(ɛ) ˆγ (l) K Ĝ (l) cusp anomalous dimension, known to all orders of a collinear anomalous dimension, known through O(a 4 ) Korchemsky Radyuskin 86 Beisert Eden Staudacher 06 Bern Dixon Smirnov 05 Cachazo Spradlin Volovich 07 ansatz generalises the iteration formula for the 2-loop n-pt amplitude mn (2) m (2) n (ɛ) = 1 2 [ m (1) n ] 2 (ɛ) + f (2) (ɛ) m (1) (2ɛ)+Const (2) + O(ɛ) n

14 Factorisation of a multi-leg amplitude in QCD Mueller 1981 Sen 1983 Botts Sterman 1987 Kidonakis Oderda Sterman 1998 Catani 1998 Tejeda-Yeomans Sterman 2002 Kosower 2003 Aybat Dixon Sterman 2006 Becher Neubert 2009 Gardi Magnea 2009 M N (p i /µ, ɛ) = L p i = β i Q 0 / 2 ( 2pi p j S NL (β i β j, ɛ) H L µ 2, (2p i n i ) 2 ) n 2 i µ2 i value of Q0 is immaterial in S, J J i ( (2pi n i ) 2 n 2 i µ2 J i ( 2(βi n i ) 2 n 2 i ), ɛ ), ɛ to avoid double counting of soft-collinear region (IR double poles), Ji removes eikonal part from Ji, which is already in S Ji/Ji contains only single collinear poles

15 N = 4 SYM in the planar limit colour-wise, the planar limit is trivial: can absorb S into Ji each slice is square root of Sudakov form factor M n = n i=1 [ ( )] 1/2 M [gg 1] si,i+1 µ 2, α s, ɛ h n ({p i },µ 2, α s, ɛ) β fn = 0 coupling runs only through dimension ᾱ s (µ 2 )µ 2ɛ =ᾱ s (λ 2 )λ 2ɛ Sudakov form factor has simple solution [ ( )] Q 2 ln Γ µ 2, α s(µ 2 ), ɛ = 1 2 ( αs (µ 2 ) n ( ) ) Q 2 nɛ [ ] γ (n) K π µ 2 2n 2 ɛ 2 + G(n) (ɛ) nɛ n=1 IR structure of N = 4 SUSY amplitudes Magnea Sterman 90 Bern Dixon Smirnov 05

16 Brief history of the ansatz the ansatz checked for the 3-loop 4-pt amplitude Bern Dixon Smirnov 05 2-loop 5-pt amplitude Cachazo Spradlin Volovich 06 Bern Czakon Kosower Roiban Smirnov 06

17 Brief history of the ansatz the ansatz checked for the 3-loop 4-pt amplitude Bern Dixon Smirnov 05 2-loop 5-pt amplitude Cachazo Spradlin Volovich 06 Bern Czakon Kosower Roiban Smirnov 06 the ansatz fails on 2-loop 6-pt amplitude Bern Dixon Kosower Roiban Spradlin Vergu Volovich 08 Alday Maldacena 07; Bartels Lipatov Sabio-Vera 08

18 Brief history of the ansatz the ansatz checked for the 3-loop 4-pt amplitude Bern Dixon Smirnov 05 2-loop 5-pt amplitude Cachazo Spradlin Volovich 06 Bern Czakon Kosower Roiban Smirnov 06 the ansatz fails on 2-loop 6-pt amplitude at 2 loops, the remainder function characterises the deviation from the ansatz R (2) n = m (2) n (ɛ) 1 2 [ m (1) n Bern Dixon Kosower Roiban Spradlin Vergu Volovich 08 Alday Maldacena 07; Bartels Lipatov Sabio-Vera 08 ] 2 (ɛ) f (2) (ɛ) m (1) n (2ɛ) Const (2) R (2) 6 known numerically Bern Dixon Kosower Roiban Spradlin Vergu Volovich 08 Drummond Henn Korchemsky Sokatchev 08 Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 analitically Duhr Smirnov VDD 09

19 W [C n ] = Tr P exp Wilson loops [ ig ] dτẋ µ (τ)a µ (x(τ)) closed contour C n made by light-like external momenta p i = x i x i+1 Alday Maldacena 07

20 W [C n ] = Tr P exp Wilson loops [ ig ] dτẋ µ (τ)a µ (x(τ)) closed contour C n made by light-like external momenta p i = x i x i+1 Alday Maldacena 07 non-abelian exponentiation theorem: vev of Wilson loop as an exponential, allows us to compute the log of W W [C n ] = 1 + L=1 a L W (L) n = exp L=1 a L w (L) n through 2 loops w (1) n = W (1) n w (2) n = W (2) n 1 2 ( W (1) n ) 2 Gatheral 83 Frenkel Taylor 84

21 W [C n ] = Tr P exp Wilson loops [ ig ] dτẋ µ (τ)a µ (x(τ)) closed contour C n made by light-like external momenta p i = x i x i+1 Alday Maldacena 07 non-abelian exponentiation theorem: vev of Wilson loop as an exponential, allows us to compute the log of W W [C n ] = 1 + L=1 a L W (L) n = exp L=1 a L w (L) n through 2 loops w (1) n = W (1) n w (2) n = W (2) n 1 2 ( W (1) n ) 2 Gatheral 83 Frenkel Taylor 84 relation between 1 loop amplitudes & Wilson loops w (1) n = Γ(1 2ɛ) Γ 2 (1 ɛ) m(1) n = m (1) n n ζ O(ɛ) Brandhuber Heslop Travaglini 07

22 MHV amplitudes Wilson loops agreement between n-edged Wilson loop and n-point MHV amplitude at weak coupling (aka weak-weak duality)

23 MHV amplitudes Wilson loops agreement between n-edged Wilson loop and n-point MHV amplitude at weak coupling (aka weak-weak duality) verified for n-edged 1-loop Wilson loop up to 6-edged 2-loop Wilson loop Brandhuber Heslop Travaglini 07 Drummond Henn Korchemsky Sokatchev 07 Bern Dixon Kosower Roiban Spradlin Vergu Volovich 08

24 MHV amplitudes Wilson loops agreement between n-edged Wilson loop and n-point MHV amplitude at weak coupling (aka weak-weak duality) verified for n-edged 1-loop Wilson loop up to 6-edged 2-loop Wilson loop Brandhuber Heslop Travaglini 07 Drummond Henn Korchemsky Sokatchev 07 Bern Dixon Kosower Roiban Spradlin Vergu Volovich 08 n-edged 2-loop Wilson loops also computed (numerically) Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09

25 MHV amplitudes Wilson loops agreement between n-edged Wilson loop and n-point MHV amplitude at weak coupling (aka weak-weak duality) verified for n-edged 1-loop Wilson loop up to 6-edged 2-loop Wilson loop Brandhuber Heslop Travaglini 07 Drummond Henn Korchemsky Sokatchev 07 Bern Dixon Kosower Roiban Spradlin Vergu Volovich 08 n-edged 2-loop Wilson loops also computed (numerically) Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 no amplitudes are known beyond the 6-point 2-loop amplitude

26 Wilson loops & Ward identities Drummond Henn Korchemsky Sokatchev 07 N=4 SYM is invariant under SO(2,4) conformal transformations

27 Wilson loops & Ward identities N=4 SYM is invariant under SO(2,4) conformal transformations the Wilson loops fulfill conformal Ward identities Drummond Henn Korchemsky Sokatchev 07

28 Wilson loops & Ward identities N=4 SYM is invariant under SO(2,4) conformal transformations the Wilson loops fulfill conformal Ward identities Drummond Henn Korchemsky Sokatchev 07 the solution of the Ward identity for special conformal boosts is given by the finite parts of the BDS ansatz + R

29 Wilson loops & Ward identities N=4 SYM is invariant under SO(2,4) conformal transformations the Wilson loops fulfill conformal Ward identities Drummond Henn Korchemsky Sokatchev 07 the solution of the Ward identity for special conformal boosts is given by the finite parts of the BDS ansatz + R for n = 4, 5, R is a constant for n 6, R is an unknown function of conformally invariant cross ratios

30 Wilson loops & Ward identities N=4 SYM is invariant under SO(2,4) conformal transformations the Wilson loops fulfill conformal Ward identities Drummond Henn Korchemsky Sokatchev 07 the solution of the Ward identity for special conformal boosts is given by the finite parts of the BDS ansatz + R for n = 4, 5, R is a constant for n 6, R is an unknown function of conformally invariant cross ratios for n = 6, the conformally invariant cross ratios are 2 u 1 = x2 13x 2 46 x 2 14 x2 36 u 2 = x2 24x 2 15 x 2 25 x2 14 u 3 = x2 35x 2 26 x 2 36 x xi are variables in a dual space s.t. p i = x i x i thus x 2 k,k+r =(p k p k+r 1 ) 2 5

31 Wilson loops Wilson loops fulfill a Ward identity for special conformal boosts the solution is the BDS ansatz + R

32 Wilson loops Wilson loops fulfill a Ward identity for special conformal boosts the solution is the BDS ansatz + R at 2 loops w n (2) (ɛ) =f (2) WL (ɛ) w(1) n (2ɛ)+C (2) WL + R(2) n,w L + O(ɛ) with f (2) WL (ɛ) = ζ 2 +7ζ 3 ɛ 5ζ 4 ɛ 2 (to be compared with f (2) (ɛ) = ζ 2 ζ 3 ɛ ζ 4 ɛ 2 for the amplitudes) R 4,W L = R 5,W L =0

33 Wilson loops Wilson loops fulfill a Ward identity for special conformal boosts the solution is the BDS ansatz + R at 2 loops w n (2) (ɛ) =f (2) WL (ɛ) w(1) n (2ɛ)+C (2) WL + R(2) n,w L + O(ɛ) with f (2) WL (ɛ) = ζ 2 +7ζ 3 ɛ 5ζ 4 ɛ 2 (to be compared with f (2) (ɛ) = ζ 2 ζ 3 ɛ ζ 4 ɛ 2 for the amplitudes) R 4,W L = R 5,W L =0 R (2) n,w L arbitrary function of conformally invariant cross ratios u ij = x2 ij+1 x2 i+1j x 2 ij x2 i+1j+1 with x 2 k,k+r =(p k p k+r 1 ) 2

34 Wilson loops Wilson loops fulfill a Ward identity for special conformal boosts the solution is the BDS ansatz + R at 2 loops w n (2) (ɛ) =f (2) WL (ɛ) w(1) n (2ɛ)+C (2) WL + R(2) n,w L + O(ɛ) with f (2) WL (ɛ) = ζ 2 +7ζ 3 ɛ 5ζ 4 ɛ 2 (to be compared with f (2) (ɛ) = ζ 2 ζ 3 ɛ ζ 4 ɛ 2 for the amplitudes) R 4,W L = R 5,W L =0 R (2) n,w L arbitrary function of conformally invariant cross ratios u ij = x2 ij+1 x2 i+1j x 2 ij x2 i+1j+1 with x 2 k,k+r =(p k p k+r 1 ) 2 duality Wilson loop MHV amplitude is expressed by R (2) n,w L = R(2) n

35 Collinear limits of Wilson loops collinear limit a b R6 0 R7 R6 Rn Rn-1 Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09

36 Collinear limits of Wilson loops collinear limit a b Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 R6 0 R7 R6 Rn Rn-1 triple collinear limit a b c R6 R6 R7 R6 R8 R6 + R6 Rn Rn-2 + R6

37 Collinear limits of Wilson loops collinear limit a b Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 R6 0 R7 R6 Rn Rn-1 triple collinear limit a b c R6 R6 R7 R6 R8 R6 + R6 Rn Rn-2 + R6 quadruple collinear limit a b c d R7 R7 R8 R7 R9 R6 + R7 Rn Rn-3 + R7

38 Collinear limits of Wilson loops collinear limit a b Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 R6 0 R7 R6 Rn Rn-1 triple collinear limit a b c R6 R6 R7 R6 R8 R6 + R6 Rn Rn-2 + R6 quadruple collinear limit a b c d R7 R7 R8 R7 R9 R6 + R7 Rn Rn-3 + R7 (k+1)-ple collinear limit i 1 i 2 i k+1 Rn Rn-k + Rk+4 (n-4)-ple collinear limit i 1 i 2 i n 4 Rn-1 Rn-1 Rn Rn-1 (n-3)-ple collinear limit Rn Rn i 1 i 2 i n 3

39 Collinear limits of Wilson loops collinear limit a b Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 R6 0 R7 R6 Rn Rn-1 triple collinear limit a b c R6 R6 R7 R6 R8 R6 + R6 Rn Rn-2 + R6 quadruple collinear limit a b c d R7 R7 R8 R7 R9 R6 + R7 Rn Rn-3 + R7 (k+1)-ple collinear limit i 1 i 2 i k+1 Rn Rn-k + Rk+4 (n-4)-ple collinear limit i 1 i 2 i n 4 Rn-1 Rn-1 Rn Rn-1 (n-3)-ple collinear limit Rn Rn i 1 i 2 i n 3 thus Rn is fixed by the (n-3)-ple collinear limit

40 Quasi-multi-Regge limit of hexagon Wilson loop 6-pt amplitude in the qmr limit of a pair along the ladder y 3 y 4 y 5 y 6 ; p 3 p 4 p 5 p 6 p 2 p 3 the conformally invariant cross ratios are q 2 u 36 = x2 13x 2 46 x 2 14 x2 36 = s 12s 45 s 123 s 345 p 4 p 5 u 14 = x2 24x 2 15 x 2 25 x2 14 = s 23s 56 s 234 s 123 p 1 q 1 p 6 u 25 = x2 35x 2 26 x 2 36 x2 25 = s 34s 61 s 234 s 345

41 Quasi-multi-Regge limit of hexagon Wilson loop 6-pt amplitude in the qmr limit of a pair along the ladder y 3 y 4 y 5 y 6 ; p 3 p 4 p 5 p 6 p 2 p 3 the conformally invariant cross ratios are q 2 u 36 = x2 13x 2 46 x 2 14 x2 36 = s 12s 45 s 123 s 345 p 4 p 5 u 14 = x2 24x 2 15 x 2 25 x2 14 = s 23s 56 s 234 s 123 p 1 q 1 p 6 u 25 = x2 35x 2 26 x 2 36 x2 25 = s 34s 61 s 234 s 345 the cross ratios are all O(1) R6 does not change its functional dependence on the u s

42 Quasi-multi-Regge limit of hexagon Wilson loop 6-pt amplitude in the qmr limit of a pair along the ladder y 3 y 4 y 5 y 6 ; p 3 p 4 p 5 p 6 p 2 p 3 the conformally invariant cross ratios are q 2 u 36 = x2 13x 2 46 x 2 14 x2 36 = s 12s 45 s 123 s 345 p 4 p 5 u 14 = x2 24x 2 15 x 2 25 x2 14 = s 23s 56 s 234 s 123 p 1 q 1 p 6 u 25 = x2 35x 2 26 x 2 36 x2 25 = s 34s 61 s 234 s 345 the cross ratios are all O(1) R6 does not change its functional dependence on the u s R6 is invariant under the qmr limit of a pair along the ladder Duhr Glover Smirnov VDD 08

43 Quasi-multi-Regge limit of n-sided Wilson loop 7-pt amplitude in the qmr limit of a triple along the ladder y 3 y 4 y 5 y 6 y 7 ; p 3 p 4 p 5 p 6 p 7 p 2 p 3 q 2 p 4 p 6 p 5 7 cross ratios, which are all O(1) R7 is invariant under the qmr limit of a triple along the ladder q 1 p 1 p 7

44 Quasi-multi-Regge limit of n-sided Wilson loop 7-pt amplitude in the qmr limit of a triple along the ladder y 3 y 4 y 5 y 6 y 7 ; p 3 p 4 p 5 p 6 p 7 p 2 p 3 q 2 p 4 p 6 p 5 7 cross ratios, which are all O(1) R7 is invariant under the qmr limit of a triple along the ladder q 1 p 1 p 7 can be generalised to the n-pt amplitude in the qmr limit of a (n-4)-ple along the ladder y 3 y 4... y n 1 y n ; p 3... p n Duhr Smirnov VDD 09

45 Quasi-multi-Regge limit of Wilson loops L-loop Wilson loops are Regge exact w n (L) (ɛ) =f (L) WL (ɛ) w(1) n (Lɛ)+C (L) WL + R(L) n,w L (u ij)+o(ɛ) Drummond Korchemsky Sokatchev 07 Duhr Smirnov VDD 09

46 Quasi-multi-Regge limit of Wilson loops L-loop Wilson loops are Regge exact w n (L) (ɛ) =f (L) WL (ɛ) w(1) n (Lɛ)+C (L) WL + R(L) n,w L (u ij)+o(ɛ) Drummond Korchemsky Sokatchev 07 Duhr Smirnov VDD 09 w (1) n = Γ(1 2ɛ) Γ 2 (1 ɛ) m(1) n

47 Quasi-multi-Regge limit of Wilson loops L-loop Wilson loops are Regge exact w n (L) (ɛ) =f (L) WL (ɛ) w(1) n (Lɛ)+C (L) WL + R(L) n,w L (u ij)+o(ɛ) Drummond Korchemsky Sokatchev 07 Duhr Smirnov VDD 09 w (1) n = Γ(1 2ɛ) Γ 2 (1 ɛ) m(1) n ln(s ij ) + Li 2 (1 u ij )

48 Quasi-multi-Regge limit of Wilson loops L-loop Wilson loops are Regge exact w n (L) (ɛ) =f (L) WL (ɛ) w(1) n (Lɛ)+C (L) WL + R(L) n,w L (u ij)+o(ɛ) Drummond Korchemsky Sokatchev 07 Duhr Smirnov VDD 09 w (1) n = Γ(1 2ɛ) Γ 2 (1 ɛ) m(1) n u s are invariant in the qmrk ln(s ij ) + Li 2 (1 u ij )

49 Quasi-multi-Regge limit of Wilson loops L-loop Wilson loops are Regge exact w n (L) (ɛ) =f (L) WL (ɛ) w(1) n (Lɛ)+C (L) WL + R(L) n,w L (u ij)+o(ɛ) Drummond Korchemsky Sokatchev 07 Duhr Smirnov VDD 09 w (1) n = Γ(1 2ɛ) Γ 2 (1 ɛ) m(1) n u s are invariant in the qmrk ln(s ij ) + Li 2 (1 u ij ) log s are not power suppressed

50 Quasi-multi-Regge limit of Wilson loops L-loop Wilson loops are Regge exact w n (L) (ɛ) =f (L) WL (ɛ) w(1) n (Lɛ)+C (L) WL + R(L) n,w L (u ij)+o(ɛ) Drummond Korchemsky Sokatchev 07 Duhr Smirnov VDD 09 w (1) n = Γ(1 2ɛ) Γ 2 (1 ɛ) m(1) n u s are invariant in the qmrk ln(s ij ) + Li 2 (1 u ij ) log s are not power suppressed we may compute the Wilson loop in qmrk the result will be correct in general kinematics!!!

51 hard diagram Diagrams of 2-loop Wilson loops curtain diagram cross diagram Y diagram Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 factorised cross diagram each diagram yields an integral, similar to a Feynman-parameter integral

52 Wilson loops: analytic calc 1. Use Mellin-Barnes (MB) representation of the Feynman-parameter integrals: replace each denominator by a contour integral 1 (A + B) λ = 1 Γ(λ) 1 2πi +i i dz Γ( z) Γ(λ + z) A z B λ+z integral turns into a sum of residues Res z= n Γ(z) = ( 1)n n!

53 Wilson loops: analytic calc 1. Use Mellin-Barnes (MB) representation of the Feynman-parameter integrals: replace each denominator by a contour integral 1 (A + B) λ = 1 Γ(λ) 1 2πi +i i dz Γ( z) Γ(λ + z) A z B λ+z integral turns into a sum of residues Res z= n Γ(z) = ( 1)n n! 2. Use Regge exactness in the qmr limit: retain only leading behaviour (i.e. leading residues) of the integral leading residue

54 Wilson loops: analytic calc 3. Use Regge exactness again: iterate the qmr limit n times, by taking the n cyclic permutations of the external legs

55 Wilson loops: analytic calc 3. Use Regge exactness again: iterate the qmr limit n times, by taking the n cyclic permutations of the external legs leading residue in step 2 leading residue in step 3

56 Wilson loops: analytic calc 3. Use Regge exactness again: iterate the qmr limit n times, by taking the n cyclic permutations of the external legs 4. Sum remaining towers of residues n=1 n=1 u n n = ln(1 u) u n n k = Li k(u) leading residue in step 2 leading residue in step 3

57 Wilson loops: analytic calc 3. Use Regge exactness again: iterate the qmr limit n times, by taking the n cyclic permutations of the external legs 4. Sum remaining towers of residues n=1 n=1 u n n = ln(1 u) u n n k = Li k(u) leading residue in step 2 leading residue in step 3 in general, get nested harmonic sums Goncharov polylogarithms n 1 =1 u n 1 1 n m 1 1 n 1 1 n 2 =1... n k 1 1 n k =1 u n k k n m k k =( 1) k G 0,..., 0, 1,..., 0,..., 0, }{{} u 1 }{{} m 1 1 m k 1 1 ;1 u 1... u k

58 Analytic 2-loop 6-edged Wilson loop compute 2-loop 6-edged Wilson loop in MB representation of the integrals in general kinematics, get up to 8-fold integrals

59 Analytic 2-loop 6-edged Wilson loop compute 2-loop 6-edged Wilson loop in MB representation of the integrals in general kinematics, get up to 8-fold integrals after procedure in qmr limit, at most 3-fold integrals in fact, only one 3-fold integral, which comes from f H (p 1,p 3,p 5 ; p 4,p 6,p 2 ) +i +i +i i i i dz 1 2πi dz 2 2πi dz 3 2πi (z 1 z 2 + z 2 z 3 + z 3 z 1 ) u z 1 1 uz 2 2 uz 3 3 Γ ( z 1 ) 2 Γ ( z 2 ) 2 Γ ( z 3 ) 2 Γ (z 1 + z 2 ) Γ (z 2 + z 3 ) Γ (z 3 + z 1 ) the result is in terms of Goncharov polylogarithms G(a, w; z) = z 0 dt (1 t a G( w; t), G(a; z) = ln z ) a

60 Analytic 2-loop 6-edged Wilson loop compute 2-loop 6-edged Wilson loop in MB representation of the integrals in general kinematics, get up to 8-fold integrals after procedure in qmr limit, at most 3-fold integrals in fact, only one 3-fold integral, which comes from f H (p 1,p 3,p 5 ; p 4,p 6,p 2 ) +i +i +i i i i dz 1 2πi dz 2 2πi dz 3 2πi (z 1 z 2 + z 2 z 3 + z 3 z 1 ) u z 1 1 uz 2 2 uz 3 3 Γ ( z 1 ) 2 Γ ( z 2 ) 2 Γ ( z 3 ) 2 Γ (z 1 + z 2 ) Γ (z 2 + z 3 ) Γ (z 3 + z 1 ) the result is in terms of Goncharov polylogarithms G(a, w; z) = z 0 dt (1 t a G( w; t), G(a; z) = ln z ) a the remainder function R6 (2) is given in terms of O(10 3 ) Goncharov polylogarithms G(u1, u2, u3) Duhr Smirnov VDD 09

61 2-loop 6-edged remainder function R6 (2) the remainder function R6 (2) is explicitly dependent on the cross ratios u1, u2, u3 Duhr Smirnov VDD 09

62 2-loop 6-edged remainder function R6 (2) the remainder function R6 (2) is explicitly dependent on the cross ratios u1, u2, u3 it is symmetric in all its arguments (in general it s symmetric under cyclic permutations and reflections) Duhr Smirnov VDD 09

63 2-loop 6-edged remainder function R6 (2) the remainder function R6 (2) is explicitly dependent on the cross ratios u1, u2, u3 it is symmetric in all its arguments (in general it s symmetric under cyclic permutations and reflections) it is of uniform, and irreducible, transcendental weight 4 Duhr Smirnov VDD 09 transcendental weights: w(ln x) = w(π) = 1 w(li2(x)) = w(π 2 ) = 2

64 2-loop 6-edged remainder function R6 (2) the remainder function R6 (2) is explicitly dependent on the cross ratios u1, u2, u3 it is symmetric in all its arguments (in general it s symmetric under cyclic permutations and reflections) it is of uniform, and irreducible, transcendental weight 4 Duhr Smirnov VDD 09 transcendental weights: w(ln x) = w(π) = 1 w(li2(x)) = w(π 2 ) = 2 it vanishes under collinear and multi-regge limits (in Euclidean space)

65 2-loop 6-edged remainder function R6 (2) the remainder function R6 (2) is explicitly dependent on the cross ratios u1, u2, u3 it is symmetric in all its arguments (in general it s symmetric under cyclic permutations and reflections) it is of uniform, and irreducible, transcendental weight 4 Duhr Smirnov VDD 09 transcendental weights: w(ln x) = w(π) = 1 w(li2(x)) = w(π 2 ) = 2 it vanishes under collinear and multi-regge limits (in Euclidean space) it is in agreement with the numeric calculation by Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09

66 2-loop 6-edged remainder function R6 (2) the remainder function R6 (2) is explicitly dependent on the cross ratios u1, u2, u3 it is symmetric in all its arguments (in general it s symmetric under cyclic permutations and reflections) it is of uniform, and irreducible, transcendental weight 4 Duhr Smirnov VDD 09 transcendental weights: w(ln x) = w(π) = 1 w(li2(x)) = w(π 2 ) = 2 it vanishes under collinear and multi-regge limits (in Euclidean space) it is in agreement with the numeric calculation by Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 straightforward computation qmr kinematics make it technically feasible

67 2-loop 6-edged remainder function R6 (2) the remainder function R6 (2) is explicitly dependent on the cross ratios u1, u2, u3 it is symmetric in all its arguments (in general it s symmetric under cyclic permutations and reflections) it is of uniform, and irreducible, transcendental weight 4 Duhr Smirnov VDD 09 transcendental weights: w(ln x) = w(π) = 1 w(li2(x)) = w(π 2 ) = 2 it vanishes under collinear and multi-regge limits (in Euclidean space) it is in agreement with the numeric calculation by Anastasiou Brandhuber Heslop Khoze Spence Travaglini 09 straightforward computation qmr kinematics make it technically feasible finite answer, but in intermediate steps many divergences output is punishingly long

68 our result has been simplified and given in terms of polylogarithms R (2) 6,W L (u 1,u 2,u 3 ) = 1 8 Goncharov Spradlin Vergu Volovich 10 3 ( L 4 (x + i,x i ) 1 ) 2 Li 4(1 1/u i ) i=1 ( 3 ) 2 Li 2 (1 1/u i ) + J π2 12 J 2 + π4 72 i=1

69 where our result has been simplified and given in terms of polylogarithms x ± i = u i x ± R (2) 6,W L (u 1,u 2,u 3 ) = L 4 (x +,x )= Goncharov Spradlin Vergu Volovich 10 3 ( L 4 (x + i,x i ) 1 ) 2 Li 4(1 1/u i ) x ± = u 1 + u 2 + u 3 1 ± 2u 1 u 2 u 3 =( u 1 + u 2 + u 3 1) 2 4u 1 u 2 u 3 3 m=0 1 8 i=1 ( 3 ) 2 Li 2 (1 1/u i ) + J π2 12 J 2 + π4 72 i=1 ( 1) m (2m)!! log(x+ x ) m (l 4 m (x + )+l 4 m (x )) + 1 8!! log(x+ x ) 4 l n (x) = 1 2 (Li n(x) ( 1) n Li n (1/x)) J = 3 (l 1 (x + i ) l 1(x i )) i=1

70 where our result has been simplified and given in terms of polylogarithms x ± i = u i x ± R (2) 6,W L (u 1,u 2,u 3 ) = L 4 (x +,x )= Goncharov Spradlin Vergu Volovich 10 3 ( L 4 (x + i,x i ) 1 ) 2 Li 4(1 1/u i ) x ± = u 1 + u 2 + u 3 1 ± 2u 1 u 2 u 3 =( u 1 + u 2 + u 3 1) 2 4u 1 u 2 u 3 3 m=0 1 8 i=1 ( 3 ) 2 Li 2 (1 1/u i ) + J π2 12 J 2 + π4 72 i=1 ( 1) m (2m)!! log(x+ x ) m (l 4 m (x + )+l 4 m (x )) + 1 8!! log(x+ x ) 4 l n (x) = 1 2 (Li n(x) ( 1) n Li n (1/x)) J = 3 (l 1 (x + i ) l 1(x i )) i=1 not a new, independent, computation just a manipulation of our result

71 where our result has been simplified and given in terms of polylogarithms x ± i = u i x ± R (2) 6,W L (u 1,u 2,u 3 ) = L 4 (x +,x )= Goncharov Spradlin Vergu Volovich 10 3 ( L 4 (x + i,x i ) 1 ) 2 Li 4(1 1/u i ) x ± = u 1 + u 2 + u 3 1 ± 2u 1 u 2 u 3 =( u 1 + u 2 + u 3 1) 2 4u 1 u 2 u 3 3 m=0 1 8 i=1 ( 3 ) 2 Li 2 (1 1/u i ) + J π2 12 J 2 + π4 72 i=1 ( 1) m (2m)!! log(x+ x ) m (l 4 m (x + )+l 4 m (x )) + 1 8!! log(x+ x ) 4 l n (x) = 1 2 (Li n(x) ( 1) n Li n (1/x)) J = 3 (l 1 (x + i ) l 1(x i )) i=1 not a new, independent, computation just a manipulation of our result answer is short and simple introduces symbols in TH physics

72 Symbols Fn. F of deg(f) = n : fn. with log cuts, s.t. Disc = 2πi f, with deg(f) = n-1

73 Symbols Fn. F of deg(f) = n : fn. with log cuts, s.t. Disc = 2πi f, with deg(f) = n-1 deg(const) = 0 deg(π) = 0 ln x : cut along [-, 0] with Disc = 2πi deg(ln x) = 1 Li2(x) : cut along [1, ] with Disc = -2πi ln x deg(li2(x)) = 2

74 Symbols Fn. F of deg(f) = n : fn. with log cuts, s.t. Disc = 2πi f, with deg(f) = n-1 deg(const) = 0 deg(π) = 0 ln x : cut along [-, 0] with Disc = 2πi deg(ln x) = 1 Li2(x) : cut along [1, ] with Disc = -2πi ln x deg(li2(x)) = 2 take a fn. defined as an iterated integral Ri rational functions T k = b a d lnr 1 d lnr k the symbol is Sym[T k ]=R 1 R k defined on the tensor product of the group of rational functions, modulo constants R 1 R 2 = R 1 + R 2

75 Symbols Fn. F of deg(f) = n : fn. with log cuts, s.t. Disc = 2πi f, with deg(f) = n-1 deg(const) = 0 deg(π) = 0 ln x : cut along [-, 0] with Disc = 2πi deg(ln x) = 1 Li2(x) : cut along [1, ] with Disc = -2πi ln x deg(li2(x)) = 2 take a fn. defined as an iterated integral Ri rational functions T k = b a d lnr 1 d lnr k the symbol is Sym[T k ]=R 1 R k defined on the tensor product of the group of rational functions, modulo constants R 1 R 2 = R 1 + R 2 Sym[ln x] =x Sym[Li 2 (x)] = (x 1) x

76 Symbols Fn. F of deg(f) = n : fn. with log cuts, s.t. Disc = 2πi f, with deg(f) = n-1 deg(const) = 0 deg(π) = 0 ln x : cut along [-, 0] with Disc = 2πi deg(ln x) = 1 Li2(x) : cut along [1, ] with Disc = -2πi ln x deg(li2(x)) = 2 take a fn. defined as an iterated integral Ri rational functions T k = b a d lnr 1 d lnr k the symbol is Sym[T k ]=R 1 R k defined on the tensor product of the group of rational functions, modulo constants R 1 R 2 = R 1 + R 2 Sym[ln x] =x Sym[Li 2 (x)] = (x 1) x take f, g with deg(f) = deg(g) = n and Sym[f] = Sym[g] then f-g = h with deg(h) = n -1

77 Symbols Fn. F of deg(f) = n : fn. with log cuts, s.t. Disc = 2πi f, with deg(f) = n-1 deg(const) = 0 deg(π) = 0 ln x : cut along [-, 0] with Disc = 2πi deg(ln x) = 1 Li2(x) : cut along [1, ] with Disc = -2πi ln x deg(li2(x)) = 2 take a fn. defined as an iterated integral Ri rational functions T k = b a d lnr 1 d lnr k the symbol is Sym[T k ]=R 1 R k defined on the tensor product of the group of rational functions, modulo constants R 1 R 2 = R 1 + R 2 Sym[ln x] =x Sym[Li 2 (x)] = (x 1) x take f, g with deg(f) = deg(g) = n and Sym[f] = Sym[g] then f-g = h with deg(h) = n -1 a symbol determines a polynomial of uniform degree up to a constant

78 2-loop 6-edged Wilson loop integral function differential equations Drummond Henn Trnka 10 discontinuities Caron-Huot 11 ideally integral symbol algorithm Duhr Gangl Rhodes (in progress) symbol (simpler) function simpler function

79 Symbols find suitable variables such that arguments of polylogarithms become rational functions (in N=4 SYM it helps to use twistors, but it s not mandatory) through some symbol-processing procedure (e.g. DGR algorithm) find simpler form of the integral in terms of polylogarithms

80 Amplitudes in twistor space twistors live in the fundamental irrep of SO(2,4) any point in dual space corresponds to a line in twistor space x a (Z a,z a+1 )

81 Amplitudes in twistor space twistors live in the fundamental irrep of SO(2,4) any point in dual space corresponds to a line in twistor space x a (Z a,z a+1 ) null separations in dual space correspond to intersections in twistor space

82 Amplitudes in twistor space twistors live in the fundamental irrep of SO(2,4) any point in dual space corresponds to a line in twistor space x a (Z a,z a+1 ) null separations in dual space correspond to intersections in twistor space 2-loop n-pt MHV amplitudes can be written as sum of pentaboxes in twistor space m (2) n = 1 2 i<j<k<l<i Arkani-Hamed Bourjaily Cachazo Trnka10

83 Recent results on symbols/integrals symbol of n-edged 2-loop Wilson loops Caron-Huot 11 (in principle one could get the n-edged 2-loop Wilson loop, but symbol is very complicated) symbols (and explicit expressions) of the 6-dimensional massless, 1-mass & 3-mass 1-loop 6-pt integrals Dixon Drummond Duhr Henn Smirnov VDD 11 explicit expression of massless 1-loop 6-pt integral is reminiscent of 6-edged 2-loop Wilson loop, but it has weight 3 I 6 (u 1,u 2,u 3 )= 1 [ L 3 (x + i,x i ) i=1 ( 3 ) 3 ] 3 l 1 (x + i ) l 1(x i ) + π2 3 χ (l 1 (x + i ) l 1(x i )) i=1 i=1 L 3 (x +,x )= 2 k = 0 ( 1) k (2k)!! lnk (x + x ) ( l 3 k (x + ) l 3 k (x ) )

84 In October 7-11, we shall have a School of Analytic Computing in Atrani, Italy lectures on amplitudes & Wilson loops by Fernando Alday Simon Caron-Huot Claude Duhr Johannes Henn Henrik Johansson Vladimir Smirnov

85

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