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A Dispersive Bootstrap for the Virasoro-Shapiro Amplitude

Abstract

We study the closed-string tree-level Virasoro-Shapiro amplitude using the dispersive S-matrix bootstrap. For the ten-dimensional maximally supersymmetric four-point amplitude, we impose analyticity, crossing symmetry, partial-wave unitarity, and Regge boundedness. With the massless graviton pole kept explicitly, the resulting dispersion relations and crossing null constraints give numerical bounds on the leading low-energy coefficients normalized by the gravitational coupling, which agree at our reference truncation with earlier bounds from smeared functionals. We then introduce a Virasoro-inspired ansatz, which becomes a set of nonlinear relations among Wilson coefficients and shrinks the allowed region toward the Virasoro-Shapiro trajectory. Finally, we study a gravity-pole-subtracted setup, where the regular part of the amplitude has a well-defined forward limit. In this stripped problem, on the slice of the leading coefficient that places the first Virasoro-Shapiro resonance at the cutoff, the nonlinear constraints reduce the allowed region to a small island containing the Virasoro-Shapiro point. Imposing the ansatz to all orders, together with spectral assumptions not used in the numerics, we show analytically that positivity selects the Virasoro-Shapiro spectrum.

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BibTeX
@misc{xu2026dispersive,
  title = {{A Dispersive Bootstrap for the Virasoro-Shapiro Amplitude}},
  author = {Yongjun Xu},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2606.19283},
  eprint = {2606.19283},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2606.19283},
}
RIS
TY  - UNPB
TI  - A Dispersive Bootstrap for the Virasoro-Shapiro Amplitude
AU  - Yongjun Xu
PY  - 2026
DA  - 2026/10/16
PB  - arXiv
DO  - 10.48550/arxiv.2606.19283
UR  - https://arxiv.org/abs/2606.19283
AB  - We study the closed-string tree-level Virasoro-Shapiro amplitude using the dispersive S-matrix bootstrap. For the ten-dimensional maximally supersymmetric four-point amplitude, we impose analyticity, crossing symmetry, partial-wave unitarity, and Regge boundedness. With the massless graviton pole kept explicitly, the resulting dispersion relations and crossing null constraints give numerical bounds on the leading low-energy coefficients normalized by the gravitational coupling, which agree at our reference truncation with earlier bounds from smeared functionals. We then introduce a Virasoro-inspired ansatz, which becomes a set of nonlinear relations among Wilson coefficients and shrinks the allowed region toward the Virasoro-Shapiro trajectory. Finally, we study a gravity-pole-subtracted setup, where the regular part of the amplitude has a well-defined forward limit. In this stripped problem, on the slice of the leading coefficient that places the first Virasoro-Shapiro resonance at the cutoff, the nonlinear constraints reduce the allowed region to a small island containing the Virasoro-Shapiro point. Imposing the ansatz to all orders, together with spectral assumptions not used in the numerics, we show analytically that positivity selects the Virasoro-Shapiro spectrum.
ER  -