Charting the Higgs self-coupling boundaries
Gauthier Durieux, Matthew McCullough, Ennio Salvioni

TL;DR
This paper explores the potential for Higgs self-coupling measurements at colliders to reveal new physics, even if other Higgs measurements align with the Standard Model, by deriving bounds on possible deviations.
Contribution
It provides theoretical bounds on Higgs self-coupling deviations in UV-complete models without fine-tuning, highlighting the discovery potential of future collider measurements.
Findings
Higgs self-coupling deviations can exceed 200% without fine-tuning.
Self-coupling measurements probe uncharted parameter space.
Potential for discovery even if other measurements show minimal deviations.
Abstract
Could new physics first manifest itself in Higgs self-coupling measurements? In other words, how large could deviations in the Higgs self-coupling be, if other Higgs and electroweak measurements are compatible with Standard Model predictions? Using theoretical arguments supported by concrete models we derive a bound on the ratio of self-coupling to single-Higgs coupling deviations in ultraviolet completions of the Standard Model where parameters are not fine-tuned. Broadly speaking, a one-loop hierarchy is allowed. We thus stress that self-coupling measurements at the LHC and future colliders probe uncharted parameter space, presenting discovery potential even in the absence of emerging hints in single-Higgs coupling measurements. For instance, if other observables show less than two-sigma deviations by the end of the LHC programme, the Higgs self-coupling deviations could still exceed…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsParticle physics theoretical and experimental studies · Distributed and Parallel Computing Systems · Dark Matter and Cosmic Phenomena
