Local spacetime physics from the Grassmannian
A duality has recently been conjectured between all leading singularities of n-particle Nk-2MHV scattering amplitudes in N = 4 SYM and the residues of a contour integral with a natural measure over the Grassmannian G(k, n). In this note we show that a simple contour deformation converts the sum of Grassmannian residues associated with the BCFW expansion of NMHV tree amplitudes to the CSW expansion of the same amplitude. We propose that for general k the same deformation yields the (k-2) parameter Risager expansion. We establish this equivalence for all MHV amplitudes and show that the Risager degrees of freedom are non-trivially determined by the GL(k - 2) "gauge" degrees of freedom in the Grassmannian. The Risager expansion is known to recursively construct the CSW expansion for all tree amplitudes, and given that the CSW expansion follows directly from the (super) Yang-Mills Lagrangian in light-cone gauge, this contour deformation allows us to directly see the emergence of local space-time physics from the Grassmannian.
This version of the article has been accepted for publication, after peer review (when applicable) and is subject to Springer Nature’s AM terms of use, but is not the Version of Record and does not reflect post-acceptance improvements, or any corrections. The Version of Record is available online at: http://dx.doi.org/10.1007/JHEP01(2011)108
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Work Title | Local spacetime physics from the Grassmannian |
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License | In Copyright (Rights Reserved) |
Work Type | Article |
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Publication Date | January 24, 2011 |
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Deposited | January 10, 2024 |
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