Amplitudes in Gravity and Yang- Mills Theories University of Sussex

Download Report

Transcript Amplitudes in Gravity and Yang- Mills Theories University of Sussex

Amplitudes in Gravity and YangMills Theories
Workshop on Continuum and Lattice
Approaches to Quantum Gravity
University of Sussex
Niels Emil Jannik Bjerrum-Bohr
Includes work in collaboration with
Z. Bern, D.C. Dunbar, H. Ita, W. Perkins, K. Risager and P. Vanhove
Introduction
2
Twistor space / New insights
Amplitudes N=4,
N=1, QCD
at NLO, Gravity..
Trees
Twistors
(Witten)
Hidden Beauty!
Loop amplitudes
Simple expressions
for amplitudes
Unitarity
Cuts
3
Yang-Mills vs Gravity
Yang-Mills
Gravity
• Twistor space
structure??!
• Yang-Mills provide Inspiration
•Twistor theory for gravity?
• Much progress
•SUSY theories
•QCD
• Progress
•SUSY theories esp N = 8 SUGRA
•Less for pure gravity
• Many new results both
•Trees
•One-loop
•n-Loops
•Planar theories
•Conformal invariance
•New results
•Trees
•One-loop (SUGRA)
•n-Loop (3-loop counterterms)
4
pp ! jets
Motivation QCD / SUSY
Signals of new physics
The LHC collider approaching
Smaller scales / higher energies..
New physics?? Supersymmetry?
Theory
versus
Experiment
Higgs?…
Precision calculations:
QCD background at NLO
5
Motivation gravity
• Spinor – Helicity / Twistor space methods
– Analytic structure of amplitudes
– MHV rules for gravity
Witten
(Witten)
• Gravity from (Yang-Mills)2
– KLT / String based rules
– Recursion / MHV rules
• Extra cancellations in gravity / finiteness of N=8???
– Amplitudes at multi-loop level
– Factorisation of amplitudes
6
Calculation of perturbative
amplitudes
# Feynman diagrams:
Factorial Growth!
Momentum vectors :
(pi ¢ pj)
Generic Feynman amplitudes
Sum over topological
different diagrams
External polarisation
tensors :
(pi ¢ εj) (ε i ¢ ε j) 7
Amplitudes
Specifying external
polarisation tensors (ε i , ε j)
Colour ordering
Simplifications
Tr(T1 T2 .. Tn)
Recursion
Spinor-helicity
formalism
Loop amplitudes
(Unitarity,
Supersymmetric
decomposition)
8
Gravity Trees
9
Quantum theory for gravity
• Gravity as a theory of point-like interactions
• Non-renormalisable theory!
Dimensionful
GN=1/M2planck
• Traditional belief : – no known symmetry can remove higher
derivative divergences.. String theory can by introducing new length scale
• Focus: N=8 supergravity – maximal supersymmetry
(Cremmer,Julia, Scherk;
Cremmer, Julia)
– Also cancellations in pure gravity as well..
10
Gravity Amplitudes
Expand Einstein-Hilbert Lagrangian :
Infinitely
many
vertices
Vertices: 3pt, 4pt, 5pt,..n-pt
Feynman diagrams:
Complicated expressions for vertices!
not attractive...!
45 terms
+ sym
(Sannan)
11
Gravity Amplitudes
KLT relationship (Kawai, Lewellen and Tye)
The KLT relationship relates open and
closed strings
Not manifest
crossing symmetry
(Bern, Carrasco,
Johansson
Better understanding
of KLT /
organisation of
amplitudes
KLT not manifestly crossing symmetric – explicit representation :
KLT not the simplest
form but better
than
Feynman diagrams
Momentum prefactors cancel double poles
Simplicity of YM amplitudes!!12
Helicity states formalism
Spinor products :
Different representations of
the Lorentz group
Momentum parts of amplitudes:
Spin-2 polarisation tensors in terms of helicities,
(squares of those of YM):
(Xu, Zhang,
Chang) 13
Scattering amplitudes in D=4

Amplitudes in gravity theories as well as
YM can hence be expressed completely
specifying
–
The external helicies
e.g. : A(1+,2-,3+,4+, .. )
–
The spinor variables
Spinor Helicity formalism
14
Yang-Mills
Trees
15
Yang-Mills MHV-amplitudes
(n) same helicities vanishes
Atree(1+,2+,3+,4+,..) = 0
(n-1) same helicities vanishes
Atree(1+,2+,..,j-,..) = 0
Tree amplitudes
First non-trivial
example,
(M)aximally
(H)elicity (V)iolating
(MHV) amplitudes
(n-2) same helicities:
Atree(1+,2+,..,j-,..,k-,..)  0
One single term!!
Atree MHV Given by the formula
(Parke and Taylor) and proven
by (Berends and Giele)
16
Gravity MHV amplitudes
• Can be generated from KLT via YM
MHV amplitudes.
Anti holomorphic
Contributions
– feature in gravity
• (Berends-Giele-Kuijf) recursion formula
17
Simplifications from SpinorHelicity
Huge simplifications
45 terms
+ sym
Vanish in spinor helicity formalism
Gravity:
Contractions
18
Twistor space
• Transformation of amplitudes
into twistor space (Penrose)
• Tree amplitudes in YM on
degenerate algebraic curves
Degree : N-1+L
• In metric signature ( + + - - ) :
2D Fourier transform
• In twistor space : plane wave
function is a line:
(Witten)
Degree : number of negative
helicities
19
Review: CSW expansion of YM
amplitudes
• In the CSW-construction : off-shell MHV-amplitudes building
blocks for more complicated amplitude expressions
(Cachazo, Svrcek and Witten) Vertex construction !
spin off of twistor support properties
• MHV vertices:
20
CSW expansion of amplitudes
• Example of A6(1-,2-,3-,4+,5+,6+)
21
Twistor space properties for gravity
• Twistor-space properties N=8 Supergravity:
More complicated!
N=4
-functions
Anti-holomorphic
pieces in gravity
amplitudes
Signature of non-locality ! typical in gravity
Derivatives of - functions
N=8
22
Twistor space properties
• For gravity : Guaranteed that
Acting with differential operators F and K
• Five-point amplitude. (Giombi, Ricci, Rables-Llana and
Trancanelli; Bern, NEJBB and Dunbar)
• Tree amplitudes :
Gravity
(Bern, NEJBB and Dunbar)
23
BCFW
Recursion
24
BCFW Recursion for trees
Complex
momentum
space!!
Shift of the spinors :
a and b will remain on-shell even after shift
Amplitude transforms as
(Britto, Cachazo, Feng, Witten)
We can now evaluate the contour integral over A(z)
25
BCWF Recursion for trees
Given that
• A(z) vanish for z ! 1
• A(z) is a rational function
• A(z) has simple poles
(C1 = 0)
(Britto, Cachazo, Feng, Witten)
Residues : Determined by factorization properties
Tree amplitude : Factorise in product of tree amplitudes
• in z
26
Recursion for tree amplitudes
• Tree-level : No other factorizations in complex plane
Interesting Fact
Only 3pt
amplitudes
needed
Generating gravity amplitudes from IR and recursion
(Bedford, Brandhuber, Spence and Travaglini; Cachazo and Svrcek;
NEJBB, Dunbar, Ita; Arkani-Hamed, Cachazo, Kaplan)
27
MHV vertex
construction
gravity
28
MHV vertex expansion for
gravity tree amplitudes
• CSW expansion in gravity
(NEJBB, Dunbar, Ita, Perkins, Risager;
• Shift (Risager)
Bianchi ,Elvang, Friedman)
Shift : Correct factorisation
CSW vertex
Reproduce CSW for Yang-Mills
29
MHV vertex expansion for
gravity tree amplitudes
• Negative legs shifted in the following way
• Analytic continuation of amplitude into the complex plane.
• If Mn(z), 1) rational, 2) simple poles at points z,
and 3) C1 vanishes (justified assumption) :
Mn(0) = sum of residues,
30
MHV vertex expansion for
gravity tree amplitudes
• All poles : Factorise as :
•
vanishes linearly in z :
• Spinor products : not z dependent (normal
CSW)
31
MHV vertex expansion for
gravity tree amplitudes
• For gravity : Substitutions
non-locality
MHV amplitudes on the pole -> MHV vertices
– MHV vertex expansion for gravity
Contact term!
Some issue for amplitudes beyond 12pt .. Unresolved (Bianchi, Elvang, Friedman)
32
Gravity
Trees
Gravity
tree properties
MHV rules for gravity
Recursion
(Bedford,
Brandhuber,Spence,
Travaglini; Cachazo,
Svrtec; NEJBB, Dunbar,
Ita; Arkani-Hamed,
Kaplan; Hall; Cheung,
Arkani-Hamed, Cachazo,
Kaplan)
MHV
(NEJBB,Dunbar,Ita,Perkins,Risager;
Bianchi, Elvang, Freedman; Mason,
Skinner; Boels, Larsen, Obers, Vonk)
Gravity scaling behaviour: Unexpected!!
A(z) » 1/z2
33
One Loop
34
Unitarity cuts
• Unitarity methods are building on the
cut equation
Singlet
Non-Singlet
35
General 1-loop amplitudes
n-pt amplitude
Vertices
carry factors
of loop
momentum
p = 2n for gravity
p=n for YM
Propagators
(Passarino-Veltman) reduction
Collapse of a propagator
36
Supersymmetric decomposition
The three types of multiplets are:
• Linked by :
• QCD amplitudes for gluons :
Combine:
N=4 : vector multiplet
N=1 : chiral multiplet
+ extra A[0] contribution
(that may contain rational non cut contributions)
37
Supersymmetric
decomposition in YM
• Super-symmetry imposes a simplicity of the expressions for loop
amplitudes.
– For N=4 YM only scalar boxes appear.
– For N=1 YM scalar boxes, triangles and bubbles appear.
• One-loop amplitudes are built up from a linear combination of
terms (Bern, Dixon, Dunbar, Kosower).
38
Quadruple cuts in complex
momenta
• Observation : Quadruple cuts of N = 4 box coefficients
) Coefficients of box functions by algebra
(Britto, Cachazo and Feng)
Solving the on-shell conditions
39
One-loop YM
• Many new results
(Britto, Cachazo, Feng)
N=4 SYM
N=1 SYM
• Many new techniques
– Recursion
(Berger, Bern, NEJBB, Dixon, Dunbar
Forde, Ita, Kosower, Su, Xiao, Yang, Zhu)
– Direct extraction in complex plane (Forde)
– Improved cutting techniques / better results for trees
• Phenomelogically interesting amplitudes
2p ! (Z,W..) + · 4 jets
– NLO is needed for precision at LHC
A key research task!!
Issues:
Rational pieces
Bulky results
40
No-Triangle Hypothesis
Justified suggestion…….
Factorisation suggests this is true for all
one-loop amplitudes
Consequence: N=8 supergravity same one-loop
structure as N=4 SYM
Evidence?
True for 4pt
Direct
evaluation
of cuts
(Green,Schwarz,Brink)
n-point MHV
(Bern,Dixon,Perelstein,Rozowsky)
6pt NMHV (IR)
(Bern, NEJBB, Dunbar,Ita)
6pt Proof
7pt evidence
n-pt proof
(NEJBB, Dunbar,Ita, Perkins, Risager;
Bern, Carrasco, Forde, Ita, Johansson)
(NEJBB, Vanhove; Arkani-Hamed,
Cachazo, Kaplan)
41
No-Triangle Hypothesis by
Cuts
Attack different parts of amplitudes 1) .. 2) .. 3) ..
(1)
Look at soft divergences (IR)
! 1m and 2m triangles
Check that boxes gives the correct IR divergences
(2)
Explicit unitary cuts
! bubble and 3m triangles
(3)
Factorisation
! rational terms.
(NEJBB, Dunbar,Ita, Perkins, Risager;
Arkani-Hamed, Cachazo, Kaplan) 42
Boxes or Quadruple cuts in
complex momenta
• Observation : Quadruple cuts of N = 4 box coefficients
) Coefficients of box functions by algebra
(Britto, Cachazo and Feng)
Solving the on-shell conditions
(l1)2=0, (l2)2=0, (l3)2=0, (l4)2=0
43
Supergravity boxes / amplitudes
KLT
N=4 YM results can be recycled
into results for N=8 supergravity
(Bern, NEJBB, Dunbar)
44
Supergravity boxes /
amplitudes
Box Coefficients
(Bern, NEJBB, Dunbar)
45
String based
analysis
46
No-triangle hypothesis
(NEJBB, Vanhove)
Generic loop amplitude
Passarino-Veltman
Naïve counting!!
Tensor integrals derivatives in Qn
47
No-triangle hypothesis
String based formalism natural basis of integrals is
Amplitude takes the form
Constraint from SUSY
48
No-triangle hypothesis
Now if we look at integrals
Typical expressions
Use
+ integration by parts
49
No-triangle hypothesis
N=8 Maximal Supergravity
(r = 2 (n – 4), s = 0)
(NEJBB, Vanhove)
(r = 2 (n – 4) - s, s >0)
Higher dimensional contributions
– vanish by amplitude gauge
invariance
Proof of No-triangle hypothesis
50
No-triangle hypothesis
Generic gravity theories:
N · 3 theories
constructable from
cuts
• Prediction N=4 SUGRA
• Prediction pure gravity
51
Gravity Multiloop
52
No-triangle for multiloops
•
No-triangle hypothesis 1-loop
• Consequences for powercounting
arguments above one-loop..
Possible to obtain YM bound??
D < 6/L + 4 for gravity???
D < 10/L + 2
Two-particle cut might miss certain cancellations
Bound might be too conservative!!
Iterated two-particle cut
Three/N-particle cut
Explicitly possible to
see extra cancellations!
(Bern, Dixon, Perelstein, Rozowsky; Bern, Dixon,
Roiban)
53
Two-Loop SYM/ Supergravity
Explicit at two loops :
‘No-triangle hypothesis’ holds at two-loops 4pt
Two-loop 5pt would be
interesting to know
(Bern,Rozowsky,Yan)
(Bern,Dixon,Dunbar,Perelstein,Rozowsky)
54
Three-Loop SYM/ Supergravity
• Three-loop four-point amplitude of N=8 supergravity
directly constructed via unitarity.
• The amplitude is ultraviolet finite in four dimensions.
• Degree of divergence in D dimensions at three loop
to be no worse than that of N=4 super-Yang-Mills
theory. Confirms ‘no-triangle hypothesis’ for three
loops.
– Remark: Surprising extra cancellations between diagrams
which are not just ‘triangle-type’..
(Bern, Carrasco, Dixon,
Johansson, Kosower, Roiban)
55
Outlook
• Wittens conjecture ! very inspiring time
– Further investigations needed to fully grasp..1-loop??
• Trees solved by
– MHV rules
– BCFW recursion
• Analytic properties of amplitudes
– Complex analysis methods
– Recursion results extended (double shifts etc)
– Development of new techniques
56
Conclusions YM
Important further investigations..
SYM theories with massless particles : Almost a closed
chapter at one-loop
Multi-loop N=4 SYM:
– real phenomenology at NLO a challenge!!
•
•
–
Further push for phenomenological results
Automatisation
(Bern et al)
1. Methods are well-developed
2. Possible to construct automatic computer code
More investigations in analytic results
Key: Simplicity / Twistor support..
57
Conclusions Gravity
• Graviton amplitudes $ much benefit from recent progress
(..twistor / helicity structure, hidden simplicity,
string based formalism..)
• Gravity $ much simpler – than Lagrangian / power counting
indicate (no-triangle property $ extra simplicity..)
• Unordered amplitudes might be even simpler than
ordered amplitudes (due to lack of boundary terms..)
Consequences at higher loop order
Finiteness??!
• String based / helicity formalism is very helpful
– however better ways to deal with gravity amplitudes
still important to focus on..
58