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Searching for Kerr in string amplitudes
Stockholm University, Nordic Institute for Theoretical Physics (Nordita). The Niels Bohr Institute, Denmark.ORCID iD: 0000-0002-7672-9688
Number of Authors: 42026 (English)In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, Vol. 2026, no 7, article id 42Article in journal (Refereed) Published
Abstract [en]

We continue the approach of [JHEP06 (2023) 167] to attempt to reproduce the classical electromagnetic current of the Kerr solution from the infinite-spin limit of a three-point amplitude with two higher-spin string states and a massless vector. We review the infinite-spin limit of three-point amplitudes along the leading Regge trajectory, which differ from Kerr, and we provide evidence that any sub-leading trajectory parallel to the leading one give the same result. We extend the above investigation to the simplest sub-leading trajectory not parallel to the leading one, containing physical states with the first two harmonics. We compute all three-point amplitudes involving two such states and a massless vector, using both covariant and DDF formalism, and we extract the associated classical infinite-spin limit. Inspired by the leading Regge case, where this limit reproduces the classical electromagnetic current sourced by a rigid rotating string, we derive new classical string solutions containing the first two harmonics and compare the currents they source to the infinite-spin amplitude of the two-harmonic state. We do not see a matching between the two approaches, and we find that the classical behaviour is instead reproduced by the amplitude involving coherent string states. We conclude this paper by discussing common patterns between the different amplitudes we considered, and we conjecture how they can be generalised to reproduce Kerr.

Place, publisher, year, edition, pages
2026. Vol. 2026, no 7, article id 42
Keywords [en]
Black Holes in String Theory, Bosonic Strings, Higher Spin Symmetry, Scattering Amplitudes
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:su:diva-258430DOI: 10.1007/JHEP07(2026)042ISI: 001810883900005Scopus ID: 2-s2.0-105043962552OAI: oai:DiVA.org:su-258430DiVA, id: diva2:2095043
Available from: 2026-08-25 Created: 2026-08-25 Last updated: 2026-08-25Bibliographically approved

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Di Vecchia, Paolo

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