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Structure of Amplitudes in Gravity II Unitarity cuts, Loops, Inherited properties from Trees, Symmetries Playing with Gravity - 24 th Nordic Meeting Gronningen 2009. Niels Emil Jannik Bjerrum-Bohr Niels Bohr International Academy Niels Bohr Institute. TexPoint fonts used in EMF.
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Structure of Amplitudes in Gravity IIUnitarity cuts, Loops, Inherited properties fromTrees, Symmetries Playing with Gravity - 24th Nordic Meeting Gronningen 2009 Niels Emil Jannik Bjerrum-Bohr Niels Bohr International Academy Niels Bohr Institute TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: AAAAAAA
Outline of lecture II • Summery of lecture I • Tree amplitudes and Helicity formalism • How to compute and New Techniques • In this lecture we will consider loop amplitudes in gravity • Traditional methods vs. Unitarity • Supersymmetry and matter amplitudes • Organisation of amplitudes • Twistor Space and amplitudes beyond one-loop PlayingwithGravity
Simplicity… Twistors Trees SUSY N=4, N=1, QCD, Gravity.. (Witten) Hidden Beauty! New simple analytic expressions Trees simple and symmetric Cuts Loops simple and symmetric Unitarity PlayingwithGravity
Loop amplitudes in field theory • Standard way: • Choose gauge • ExpandLagrangian • Features: • 3pt vertex: approx 100 terms • 4pt vertex much worse • Propagator: 3 terms • Number of topologies grows as n! • Problems: off-shell formalism • Not directly usable with spinor-helicity • n Much worse than tree level – one have to do integrations • 1 In sums of contributions to loop amplitudes cancellations appear (but only after doing horrible integrals…) PlayingwithGravity
Unitarity cuts Unitarity methods are building on the cut equation Singlet Non-Singlet PlayingwithGravity
General 1-loop amplitudes n-pt amplitude (Maximal graph) Vertices carry factors of loop momentum p = 2n for gravity p=n for Yang-Mills Propagators (Passarino-Veltman)reduction Collapse of a propagator PlayingwithGravity
Passarino-Veltman Illustrative Passarino-Veltman Due to this generic loop amplitudes have the form: PlayingwithGravity
Unitarity cuts Generic one-loop amplitude (without R term): Relate kinematic discontinuity of the one loop amplitude. This imposes constraints on the coefficients Early problems in 60ties with cutting techniques isrelated to not having a integral basis(dimensionally regularised). PlayingwithGravity
Quadruple Cut Boxes only! Having complex momentum Crucial for mass-less corners In 4D an algebraic expression! (Britto, Cachazo and Feng) PlayingwithGravity
Triple Cut Scalar Boxes and Scalar Triangles In 4D still one integral left! PlayingwithGravity
Double Cut Scalar Boxes and Scalar Triangles and Bubbles In 4D still two integrals left! PlayingwithGravity
UnitarityCuts for differenttheories Sum over particles in multiplet (singlet) Sum over particles in multiplet (non-singlet states) • Have to sum over multiplet to compute supersymmetric amplitudes • Hence we need tree amplitudes with matter lines.. PlayingwithGravity
N=8 Supergravity Maximal theory of supergravity DeWit, Freedman; Cremmer, Julia, Scherk; Cremmer, Julia Features: 28 = 256 masslessstates (helicity) 1+1=2 graviton states (+2,-2) 8+8=16 gravitino states (+3/2, -3/2) 28+28 = 56 vector states (-1,1) 56+56 = 112 fermion states (-1/2,1/2) 70 scalars (0) Need to sum over multiplet of all 256 states… in cuts PlayingwithGravity
KLT and N=4 Yang-Mills Maximal theory of super Yang-Mills Features: 24 = 16 masslessstates (helicity) 1+1=2 vector states (+1,-1) 4+4=8 fermion states (+1/2, -1/2) 6 scalars (0) • Uses two things: • KLT writes N=8 amplitudes as products of N=4 amplitudes. • [Spectrum of N=8] = [Spectrum of N=4] x [Spectrum of N=4] PlayingwithGravity
Supersymmetric Ward Identities Sum over particles in multiplet (singlet) Sum over particles in multiplet (non-singlet states) • Need a method to sum over states in cut • Possibilities: • Use CSW, BCFW, other recursive techniques to generate amplitudes • Use SUSY ward identities to sum over terms in Cut. • Very useful for MHV amplitudes • Helps for NkMHV amplitudes but much more work... PlayingwithGravity
SUSY Ward identities N=4 MHV PlayingwithGravity
Ward identities NMHV Needed to work out For N=8 6pt SUGRA amplitudes PlayingwithGravity
Recipe for computations in N=8 SUGRA • Write down 1-loop amplitude • Write down all helicity configurations • Write down all possible cuts (consider various cut channels) • Write down cut trees (including all trees with internal SUSY particles) • Fix box coefficients from quadruple cuts • Fix triangles and bubbles from triple and double cuts • Finally check that amplitudedoes not have rational parts: • If rational partsexist either compute using cuts in • Or use new recursive techniques (will be discussed in lecture III) PlayingwithGravity
Example of quadruple cut Have to solve… If corners is massive we can just solve constraints If one corner is massless we have to assume complex momenta of say Thereby we can write Where either Playing with Gravity
Examples of cuts Lets consider 5pt 1-loop amplitude in N=8 Supergravity (singlet cut) We have PlayingwithGravity
Examples of cuts In this example we have 4 terms (after some algebra…) PlayingwithGravity
Examples of cuts Using that We have PlayingwithGravity
Supergravityboxes KLT N=4 YM results can be recycled into results for N=8 supergravity (Bern, NEJBB, Dunbar) PlayingwithGravity
Supergravity amplitudes Box Coefficients (Bern, NEJBB, Dunbar) PlayingwithGravity
Supergravity amplitudes • A way to organise cuts is through use the scaling behaviour of shifts Playing with Gravity
Supergravity amplitudes This can serve as a way to organise the amplitude. Especially if the large-z limit is zero then bubbles will be vanishing Terms corresponding to box terms will go as While triangles goes as We will discuss this in more details in Lecture III Playing with Gravity
Singularitystructure of amplitude Tree amplitude has factorisations: Loop amplitudes has the followinggenericfactorisationstructure: (Bern and Chalmers) Playing with Gravity
IR singularities of gravity Gravity amplitudes have IR singularities of the form IR singularities can arise from both box and triangle integral functions PlayingwithGravity
Singularitystructure of amplitude • Singularitystructurecanbeused to check validity of amplitude expressions • Looking at IR singularitiescanbeused to determineifcertain terms are in amplitude • Completecontrol of singularitystructurecanbeused to do recursivecomputations • Will discuss more in Lecture III… Playing with Gravity
Twistor space properties of gravity loop amplitudes • Unitarity : loop behaviour from trees • Cuts of the MHV box • Consider the cut C123, where the gravity tree amplitude is Mtree(l5, 1, 2, 3, l3). • This tree is annihilated by F3(123) • Hence F3(123)cN=8(45)123 = 0 • Similarly F3(145)cN=8(45)123 = F3(345)cN=8(45)123 = 0. • Remaining choices of Fijk : consider more generalised cuts, e.g., C(4512) and hence F4(124)cN=8(45)123 = 0. • Summarising: PlayingwithGravity
Twistor space properties of gravity loop amplitudes • Inspecting the general n-point case, we can now predict • Similarly we can deduce that (consistent with the YM picture), Topology : As N=4 super-Yang-Mills) Pointslie on three intersecting lines(Bern, Dixon and Kosower) PlayingwithGravity
Multi-loop amplitude • Most of the cut techniques we have discussed can be applied also at multi-loop level • Difficulties: more difficult factorisations + no set basis of integral functions PlayingwithGravity
Conclusions • We have seen how it possible to deal with loop amplitudes in new and efficient ways • On-shell tree amplitudes can be used as input for cuts. • Calculating all cuts we can compute the amplitude • Feature: Symmetries for tree amplitudes leads to symmetries for loop amplitudes PlayingwithGravity
Outline af III • In Lecture III • we will discuss how new techniques for gravity amplitudes can be used learn new aspects of gravity amplitudes • Among other things we will discuss • Additional symmetry for gravity • No-triangle Property of N=8 Supergravity • Possible Finiteness of N=8 Supergravity PlayingwithGravity