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Probing triple Higgs coupling with machine learning at the LHC

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arxiv 2005.11086 v4 pith:3M5Z46H7 submitted 2020-05-22 hep-ph hep-ex

classification hep-phhep-ex
keywords higgscouplingtriplecrossmpnnpairprocessproduction
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

Measuring the triple Higgs coupling is a crucial task in the LHC and future collider experiments. We apply the Message Passing Neural Network (MPNN) to the study of the non-resonant Higgs pair production process $pp \to hh$ in the final state with $2b + 2\ell + E_{\rm T}^{\rm miss}$ at the LHC. Although the MPNN can improve the signal significance, it is still challenging to observe such a process at the LHC. We find that a $2\sigma$ upper bound (including a 10\% systematic uncertainty) on the production cross section of the Higgs pair is 3.7 times the predicted SM cross section at the LHC with the luminosity of 3000 fb$^{-1}$, which will limit the triple Higgs coupling to the range of $[-3,11.5]$.

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Cited by 4 Pith papers

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  1. Tagging fully hadronic exotic decays of the vectorlike $\mathbf{B}$ quark using a graph neural network

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  2. Deep Learning to Improve the Sensitivity of Higgs Pair Searches in the $4b$ Channel at the LHC

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    An attention-based full-event classifier constrains the Higgs self-coupling to (-0.53, 6.01) at 68% CL in the HH to 4b channel, a projected improvement over cut-based analyses.

  3. Triple Higgs Boson Production with Two Heavy Scalars at the LHC via a Simplified Approach

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    Double-resonant triple Higgs boson production at the LHC can be described by a single rescaling factor rho2, and projected 95% CL limits on rho2 over the (m2,m3) plane make the analysis applicable to any two-narrow-sc...

  4. The LHC sensitivity to weak gauginos in light of the latest muon $g-2$ and dark matter results

    hep-ph 2025-05 conditional novelty 4.0 of 10

    In the MSSM, after muon g-2 and dark matter constraints, only bino-like LSPs with wino or slepton coannihilation survive, and a 27 TeV HE-LHC could probe most of the remaining mass range.

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