Celestial superamplitude in $$ \mathcal{N} $$ = 4 SYM theory
نویسندگان
چکیده
A bstract Celestial amplitude is a new reformulation of momentum space scattering amplitudes and offers promising way for flat holography. In this paper, we study the celestial in $$ \mathcal{N} N = 4 Super-Yang-Mills (SYM) theory aiming at understanding role superconformal symmetry We first construct generators acting on superfield which assembles all on-shell fields multiplet together terms variables Grassmann parameters. These satisfy algebra SYM theory. also compute three-point four-point super-amplitudes explicitly. They can be identified as conformal correlation functions superfields living sphere. further soft collinear limits give rise to super-Ward identity super-OPE sphere, respectively. Our results initiate perspective well-studied via 2D field
منابع مشابه
SL ( 2 , Z ) multiplets in N = 4 SYM theory
We discuss the action of SL(2, Z) on local operators in D = 4, N = 4 SYM theory in the superconformal phase. The modular property of the operator’s scaling dimension determines whether the operator transforms as a singlet, or covariantly, as part of a finite or infinite dimensional multiplet under the SL(2, Z) action. As an example, we argue that operators in the Konishi multiplet transform as ...
متن کاملNew results in the deformed N = 4 SYM theory
We investigate various perturbative properties of the deformed N = 4 SYM theory. We carry out a three-loops calculation of the chiral matter superfield propagator and derive the condition on the couplings for maintaining finiteness at this order. We compute the 2-, 3-and 4-point functions of composite operators of dimension 2 at two loops. We identify all the scalar operators (chiral and non-ch...
متن کاملNon-renormalisation of extremal correlators in N=4 SYM theory
We show that extremal correlators of chiral primary operators in N=4 supersymmetric Yang–Mills theory with SU(N) gauge group are neither renormalised at first (g2) order in perturbation theory nor receive contribution from any instanton sector at leading order in the semiclassical expansion. This lends support to the strongest version of a new prediction recently put forward on the basis of the...
متن کاملPerturbation Theory in Celestial Mechanics
4 Classical perturbation theory 4 4.1 The classical theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 4.2 The precession of the perihelion of Mercury . . . . . . . . . . . . . . . . . . . . 6 4.2.1 Delaunay action–angle variables . . . . . . . . . . . . . . . . . . . . . . 6 4.2.2 The restricted, planar, circular, three–body problem . . . . . . . . . . . 7 4.2.3 Expansi...
متن کاملA super MHV vertex expansion for N = 4 SYM theory
We present a supersymmetric generalization of the MHV vertex expansion for all tree amplitudes in N = 4 SYM theory. In addition to the choice of a reference spinor, this super MHV vertex expansion also depends on four reference Grassmann parameters. We demonstrate that a significant fraction of diagrams in the expansion vanishes for a judicious choice of these Grassmann parameters, which simpli...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of High Energy Physics
سال: 2021
ISSN: ['1127-2236', '1126-6708', '1029-8479']
DOI: https://doi.org/10.1007/jhep08(2021)031