Abstract:In search of natural building blocks for supergravity amplitudes, a tentative
criteria is term-by-term bonus z^-2 large momentum scaling. For a given choice
of deformation legs, we present such an expansion in the form of a BCFW
representation in N=7 supergravity based on a special shift. We will show that
this improved scaling behavior, with respect to the fully N=8 representation,
is due to its automatic incorporation of the so called bonus relations.Comment: 16 pages, 2 figure
“…instead of (n − 2)! terms so it appears that the N = 7 recursion encodes bonus relations [27], as was previously observed in [28]. In [30], the bonus relations were used to write non-MHV amplitudes in N = 8 sugra as a sum over (n − 3)!…”
Section: Jhep01(2021)181mentioning
confidence: 85%
“…For example, for MHV amplitudes there are (n−3)! diagrams rather than (n−2)!, so the N = 7 recursion incorporates a property of sugra amplitudes known as the bonus relations [27] (this property of N = 7 recursion was first observed in [28]). The price to pay for having fewer diagrams is that they generally contain more closed cycles which can become tedious to evaluate at high multiplicity using conventional methods, so we develop a new technique which avoids summing over closed cycles.…”
We derive an on-shell diagram recursion for tree-level scattering amplitudes in $$ \mathcal{N} $$
N
= 7 supergravity. The diagrams are evaluated in terms of Grassmannian integrals and momentum twistors, generalising previous results of Hodges in momentum twistor space to non-MHV amplitudes. In particular, we recast five and six-point NMHV amplitudes in terms of $$ \mathcal{N} $$
N
= 7 R-invariants analogous to those of $$ \mathcal{N} $$
N
= 4 super-Yang-Mills, which makes cancellation of spurious poles more transparent. Above 5-points, this requires defining momentum twistors with respect to different orderings of the external momenta.
“…instead of (n − 2)! terms so it appears that the N = 7 recursion encodes bonus relations [27], as was previously observed in [28]. In [30], the bonus relations were used to write non-MHV amplitudes in N = 8 sugra as a sum over (n − 3)!…”
Section: Jhep01(2021)181mentioning
confidence: 85%
“…For example, for MHV amplitudes there are (n−3)! diagrams rather than (n−2)!, so the N = 7 recursion incorporates a property of sugra amplitudes known as the bonus relations [27] (this property of N = 7 recursion was first observed in [28]). The price to pay for having fewer diagrams is that they generally contain more closed cycles which can become tedious to evaluate at high multiplicity using conventional methods, so we develop a new technique which avoids summing over closed cycles.…”
We derive an on-shell diagram recursion for tree-level scattering amplitudes in $$ \mathcal{N} $$
N
= 7 supergravity. The diagrams are evaluated in terms of Grassmannian integrals and momentum twistors, generalising previous results of Hodges in momentum twistor space to non-MHV amplitudes. In particular, we recast five and six-point NMHV amplitudes in terms of $$ \mathcal{N} $$
N
= 7 R-invariants analogous to those of $$ \mathcal{N} $$
N
= 4 super-Yang-Mills, which makes cancellation of spurious poles more transparent. Above 5-points, this requires defining momentum twistors with respect to different orderings of the external momenta.
Modern on-shell S-matrix methods may dramatically improve our understanding of perturbative quantum gravity, but current foundations of on-shell techniques for General Relativity still rely on off-shell Feynman diagram analysis. Here, we complete the fully on-shell proof of Ref.[1] that the recursion relations of Britto, Cachazo, Feng, and Witten (BCFW) apply to General Relativity tree amplitudes. We do so by showing that the surprising requirement of "bonus" z −2 scaling under a BCFW shift directly follows from Bose-symmetry. Moreover, we show that amplitudes in generic theories subjected to BCFW deformations of identical particles necessarily scale as z even . When applied to the color ordered expansions of Yang-Mills, this directly implies the improved behavior under non-adjacent gluon shifts. Using the same analysis, three-dimensional gravity amplitudes scale as z −4 , compared to the z −1 behavior for conformal Chern-Simons matter theory.
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