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Twistors and Pertubative Gravity including work (2005) with Z Bern, S Bidder, E Bjerrum-Bohr, H Ita, W Perkins, K Risager From Twistors to Amplitudes 2005.

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Presentation on theme: "Twistors and Pertubative Gravity including work (2005) with Z Bern, S Bidder, E Bjerrum-Bohr, H Ita, W Perkins, K Risager From Twistors to Amplitudes 2005."— Presentation transcript:

1 Twistors and Pertubative Gravity including work (2005) with Z Bern, S Bidder, E Bjerrum-Bohr, H Ita, W Perkins, K Risager From Twistors to Amplitudes 2005

2 Dave Dunbar QMUL, Nov 05 2/36 Summary Review of Perturbative Gravity KLT approach Recursive approach MHV vertex approach Loops N=8, 1-loop comparison with gravity beyond one-loop Conclusions

3 Dave Dunbar QMUL, Nov 05 3/36 Perturbative Quantum Gravity

4 Dave Dunbar QMUL, Nov 05 4/36 Feynman diagram approach to quantum gravity is extremely complicated Gravity = (Yang-Mills) 2 Feynman diagrams for Yang-Mills = horrible mess How do we deal with (horrible mess) 2 Using traditional techniques even the four-point tree amplitude is very difficult Sannan,86

5 Dave Dunbar QMUL, Nov 05 5/36 Kawai-Lewellen-Tye Relations -pre-twistors one of few useful techniques -derived from string theory relations -become complicated with increasing number of legs -contains unneccessary info -MHV amplitudes calculated using this KLT,86 Berends,Giele, Kuijf

6 Dave Dunbar QMUL, Nov 05 6/36 Double-Poles Naively, products of Yang-Mills amplitudes would contain double poles A(1,2,3,4,5)xA(2,1,3,4,5) Cancelled by momentum prefactors s 34 s 12 Factorisation structure not manifest Crossing Symmetric although not manifest

7 Dave Dunbar QMUL, Nov 05 7/36 Twistor Structure Of Gravity Amplitudes Look for Twistor inspired formalism Not obvious such formalism exist (conformal gravity..) Can we examine twistor structure by action of differential operators?

8 Dave Dunbar QMUL, Nov 05 8/36 Collinearity of MHV amplitudes For Yang-Mills F ijk A n =0 trivially This implies MHV amplitudes have collinear support when transforming to a function in twistor space Independence upon implies has a  function

9 Dave Dunbar QMUL, Nov 05 9/36 Gravity MHV amplitudes For Gravity M n is polynomial in with degree (2n-6), eg Consequently In fact….. Upon transforming M has a derivative of  function support

10 Dave Dunbar QMUL, Nov 05 10/36 MHV amplitudes have suppport on line only -For Yang-Mills there is  function -For Gravity it is a derivative of a  function

11 Dave Dunbar QMUL, Nov 05 11/36 Coplanarity NMHV amplitudes in Yang-Mills have coplanar support For Gravity we have verified n=5 by Giombi, Ricci, Robles-Llana Trancanelli n=6,7,8 Bern, Bjerrum-Bohr,Dunbar

12 Dave Dunbar QMUL, Nov 05 12/36 Coplanarity-MHV vertices Two intersecting lines in twistor space define the plane -Points on one MHV vertex

13 Dave Dunbar QMUL, Nov 05 13/36 Recursion Relations Return of the analytic S-matrix! Shift amplitude so it is a complex function of z Amplitude becomes an analytic function of z, A(z) Full amplitude can be reconstructed from analytic properties Britto,Cachazo,Feng (and Witten) Within the amplitude momenta containing only one of the pair are z-dependant P(z)

14 Dave Dunbar QMUL, Nov 05 14/36 Recursion for Gravity Gravity, seems to satisfy the conditions to use recursion relations Allows (re)calculation of MHV gravity tree amps Expression for six-point NMHV tree Bedford, Brandhuber, Spence, Travaglini Cachazo,Svrcek Bedford, Brandhuber, Spence, Travaglini Cachazo,Svrcek

15 Dave Dunbar QMUL, Nov 05 15/36 MHV-vertex construction Works for gluon scattering tree amplitudes Works for (massless) quarks Works for Higgs and W’s Works for photons Works for gravity……. Bjerrum-Bohr,DCD,Ita,Perkins, Risager Ozeren+Stirling Badger, Dixon, Glover, Forde, Khoze, Kosower Mastrolia Wu,Zhu; Su,Wu; Georgiou Khoze Cachazo Svrcek Witten++ Promotes MHV amplitude to fundamental object by off-shell continuation

16 Dave Dunbar QMUL, Nov 05 16/36 + _ _ _ _ _ + + + + + + _ _ _ -three point vertices allowed -number of vertices = (number of -) -1

17 Dave Dunbar QMUL, Nov 05 17/36 -problem for gravity Need the correct off-shell continuation Proved to be difficult Resolution involves continuing the of the negative helicity legs The r i are chosen so that a) momentum is conserved b) multi-particle poles P(z) are on-shell -this fixes them uniquely Shift is the same as that used by Risager to derive MHV rules using analytic structure

18 Dave Dunbar QMUL, Nov 05 18/36 Eg NMHV amplitudes 3-3- 1-1- k+k+ 2-2- k+1 + + -+

19 Dave Dunbar QMUL, Nov 05 19/36 applying momentum conservation gives -this a combination of three BCF shifts -demanding P(z) 2 =0 gives the condition on z -which fixes z and so determines prescription

20 Dave Dunbar QMUL, Nov 05 20/36 Makes MHV apparent as a analytic shift Has interpretation as contact terms since and the P 2 can cancel pole between MHV vertices Construction ``expands’’ contact terms in a consistent manner

21 Dave Dunbar QMUL, Nov 05 21/36 Loop Amplitudes Loop amplitudes perhaps the most interesting aspect of gravity calculations UV structure always interesting Chance to prove/disprove our prejudices Studying Amplitudes may uncover symmetries not obvious in Lagrangian

22 Dave Dunbar QMUL, Nov 05 22/36 Supersymmetric Decomposition Supersymmetric decomposition important for QCD amplitudes -this can be inverted

23 Dave Dunbar QMUL, Nov 05 23/36 Decomposition of Graviton One- Loop Scattering Amplitude Known for Four-Point only -N=8 Green Schwarz & Brink  ’ ! 0 limit of string theory, 1985 -N=0 Grisaru & Zak, 1980 -remainder Dunbar & Norridge, 1996 -focus upon N=8 for rest of talk

24 Dave Dunbar QMUL, Nov 05 24/36 General Decomposition of One- loop n-point Amplitude Vertices involve loop momentum propagators p degree p in l p=n : Yang-Mills p=2n Gravity

25 Dave Dunbar QMUL, Nov 05 25/36 Passarino-Veltman reduction Decomposes a n-point integral into a sum of (n-1) integral functions obtained by collapsing a propagator k l l-kl-k

26 Dave Dunbar QMUL, Nov 05 26/36 -process continues until we reach four-point integral functions with (in yang-mills up to quartic numerators) -similarly 3 -> 2 also gives scalar triangles. At bubbles process ends. Quadratic bubbles can be rational functions involving no logarithms. -so in general, for massless particles

27 Dave Dunbar QMUL, Nov 05 27/36 N=4 Susy Yang-Mills In N=4 Susy there are cancellations between the states of different spin circulating in the loop. Leading four powers of loop momentum cancel (in well chosen gauges..) N=4 lie in a subspace of the allowed amplitudes (BDDK) Determining rational c i determines amplitude -4pt…. Green, Schwarz, Brink -MHV,6pt 7pt,gluinos Bern, Dixon, Del Duca Dunbar, Kosower Britto, Cachazo, Feng; Roiban Spradlin Volovich Bidder, Perkins, Risager UV finiteness of one-loop amplitudes trivial

28 Dave Dunbar QMUL, Nov 05 28/36 Basis in N=4 Theory ‘easy’ two-mass box ‘hard’ two-mass box

29 Dave Dunbar QMUL, Nov 05 29/36 N=8 Supergravity Loop polynomial of n-point amplitude of degree 2n. Leading eight-powers of loop momentum cancel (in well chosen gauges..) leaving (2n-8) Beyond 4-point amplitude contains triangles..bubbles Beyond 6-point amplitude is not cut-constructible

30 Dave Dunbar QMUL, Nov 05 30/36 No-Triangle Hypothesis -against this expectation, it might be the case that……. Evidence? true for 4pt n-point MHV 6pt NMHV -factorisation suggests this is true for all one-loop amplitudes Bern,Dixon,Perelstein,Rozowsky Bern, Bjerrum-Bohr, Dunbar,Ita Green,Schwarz,Brink

31 Dave Dunbar QMUL, Nov 05 31/36 consequences? One-Loop amplitudes look just like N=4 SYM UV finiteness obvious …..as it is from field theory analysis..but no so for N<8 Dunbar,Julia,Seminara,Trigiante, 00

32 Dave Dunbar QMUL, Nov 05 32/36 Two-Loop SYM/ Supergravity Bern,Rozowsky,Yan Bern,Dixon,Dunbar,Perelstein,Rozowsky -N=8 amplitudes very close to N=4 I P planar double box integral

33 Dave Dunbar QMUL, Nov 05 33/36 Beyond 2-loops: UV pattern D=110 #/  D=100(!) #/  D=90 #/  D=8 #/  #’/  2 +#”/  D=70 #/  D=600 D=5000 D=40000 L=1L=2L=3L=4L=5L=6 N=4 Yang-Mills Honest calculation/ conjecture (BDDPR) N=8 Sugra

34 Dave Dunbar QMUL, Nov 05 34/36 Does ``no-triangle hypothesis imply perturbative expansion of N=8 SUGRA more similar to that of N=4 SYM than power counting/ field theory arguments suggest???? If factorisation is the key then perhaps yes.

35 Dave Dunbar QMUL, Nov 05 35/36 Conclusions Gravity calculations amenable to many of the new techniques Both recursion and MHV– vertex formulations exist Perturbative expansion of N=8 seems to be surprisingly simple. This may have consequences Consequences for the duality?


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