Bootstrapping extremal scalar amplitudes with and without supersymmetry

A bstract We re-examine positivity bounds on the 2 → 2 scattering of identical massless real scalars with a novel perspective on how these bounds can be used to constrain the spectrum of UV theories. We propose that the entire space of consistent weakly-coupled (and generically non-supersymmetric) UV amplitudes is determined as a convex hull of the massive scalar amplitude and a one-parameter family of scalarless “extremal amplitudes” parameterized by the ratio of the masses of the two lightest massive states. Further, we propose that the extremal amplitudes can be constructed from a similar one-parameter set of maximally supersymmetric amplitudes, leading to the surprising possibility that the S-matrix bootstrap with maximal supersymmetry may be sufficient to determine the entire allowed space of four-point amplitudes! Finally, we show that minimal spectrum input reduces the allowed space of Wilson coefficients to small islands around the open string Dirac-Born-Infeld tree amplitude and the closed string Virasoro-Shapiro amplitude.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-05-13
DOI
https://doi.org/10.1007/jhep05(2026)149
Primary Topic
Black Holes and Theoretical Physics
Type
preprint
Field-Weighted Citation Impact
0.00

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preprint

Bootstrapping extremal scalar amplitudes with and without supersymmetry

Loki L. Lin, Nicholas Geiser, Henriette Elvang, J D Berman
Journal of High Energy Physics
Black Holes and Theoretical Physics
preprint

Bootstrapping extremal scalar amplitudes with and without supersymmetry

Loki L. Lin, Nicholas Geiser, Henriette Elvang, J D Berman
preprint en

Abstract

A bstract We re-examine positivity bounds on the 2 → 2 scattering of identical massless real scalars with a novel perspective on how these bounds can be used to constrain the spectrum of UV theories. We propose that the entire space of consistent weakly-coupled (and generically non-supersymmetric) UV amplitudes is determined as a convex hull of the massive scalar amplitude and a one-parameter family of scalarless “extremal amplitudes” parameterized by the ratio of the masses of the two lightest massive states. Further, we propose that the extremal amplitudes can be constructed from a similar one-parameter set of maximally supersymmetric amplitudes, leading to the surprising possibility that the S-matrix bootstrap with maximal supersymmetry may be sufficient to determine the entire allowed space of four-point amplitudes! Finally, we show that minimal spectrum input reduces the allowed space of Wilson coefficients to small islands around the open string Dirac-Born-Infeld tree amplitude and the closed string Virasoro-Shapiro amplitude.

Journal of High Energy PhysicsVol. 2026(5)
University of Copenhagen (DK), University of Michigan (US)
National Science Foundation, U.S. Department of Energy, Research Corporation for Science Advancement, University of Michigan
Openalex Percentile: Top 99%
Black Holes and Theoretical Physics
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