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On the Theory of Continuous-Spin Particles: Helicity Correspondence in Radiation and Forces

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arxiv 1302.1577 v2 pith:E3BCFQK7 submitted 2013-02-06 hep-th hep-ph

classification hep-thhep-ph
keywords amplitudescspshelicityparticlescorrespondenceforcesconsistentcontinuous-spin
verification ladder T0 review T1 audit T2 compute T3 formal
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We have recently shown that continuous-spin particles (CSPs) have covariant single-emission amplitudes with the requisite properties to mediate long-range forces. CSPs, the most general massless particle type consistent with Lorentz symmetry, are characterized by a scale \rho. Here, we demonstrate a helicity correspondence at CSP energies larger than \rho, in which these amplitudes are well approximated by the familiar ones for particles of helicity 0, 1, or 2. These properties follow from Lorentz invariance. We also construct tree-level multi-emission and CSP-exchange amplitudes that are unitary, appropriately analytic, and consistent with helicity-0 correspondence. We propose sewing rules from which these amplitudes and others can be obtained. We also exhibit a candidate CSP-graviton matrix element, which shows that the Weinberg-Witten theorem does not apply to CSPs. These results raise the surprising possibility that the known long-range forces might be mediated by CSPs with very small \rho, rather than by helicity 1 and 2 particles.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Wigner continuous-spin equations in $\mathbf{AdS_D}$: bosonic and fermionic cases

    hep-th 2026-06 unverdicted novelty 6.0 of 10

    Construction of first-class constraint systems for bosonic and fermionic continuous-spin fields in AdS_D that realize the so(2,D-1) algebra via Lie-Lorentz derivative and match Metsaev's Casimir classification.

  2. Hydrogen 21 cm Constraints on the Photon's Spin Scale

    hep-ph 2025-05 conditional novelty 6.0 of 10

    A continuous-spin photon would suppress the hydrogen 21cm transition rate by 1 minus rho squared alpha squared over 6 omega squared, which turns existing in-beam hyperfine data into the bound rho below 1 meV.

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