Four-point amplitudes in N=8 supergravity and Wilson loops

被引:34
作者
Brandhuber, A. [1 ]
Heslop, P. [1 ]
Nasti, A. [1 ]
Spence, B. [1 ]
Travaglini, G. [1 ]
机构
[1] Univ London, Dept Phys, Ctr Res String Theory, London E1 4NS, England
基金
英国工程与自然科学研究理事会;
关键词
SUDAKOV FORM-FACTOR; YANG-MILLS; ASYMPTOTIC-BEHAVIOR; QUANTUM CHROMODYNAMICS; SCATTERING; GRAVITY; FIELD; QCD; RENORMALIZATION; DYNAMICS;
D O I
10.1016/j.nuclphysb.2008.09.010
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Prompted by recent progress in the study of N = 4 super Yang-Mills amplitudes, and evidence that similar approaches are relevant to N = 8 supergravity, we investigate possible iterative structures and applications of Wilson loop techniques in maximal supergravity. We first consider the two-loop, four-point MHV scattering amplitude in N = 8 supergravity, confirming that the infrared divergent parts exponentiate, and we give the explicit expression which represents the failure for this to occur for the finite part. We observe that each term in the expansion of the one- and two-loop amplitudes in the dimensional regularisation parameter E has a uniform degree of transcendentality. We then turn to consider Wilson loops in supergravity, showing that a natural definition of the loop, involving the Christoffel connection, fails to reproduce the one-loop amplitude. An alternative expression, which involves the metric explicitly, is shown to have a close relationship with the physical amplitude. We find that in a gauge in which the cusp diagrams vanish, the remaining diagrams for this Wilson loop correctly generate the full one-loop, four-point N = 8 supergravity amplitude. (C) 2008 Elsevier B.V. All rights reserved.
引用
收藏
页码:290 / 314
页数:25
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