Dark Higgs in Hidden Sector as a Probe for Dark Matter
Faeq Abed, Asmaa AlMellah, Gaber Faisel

TL;DR
This paper analyzes the potential of the FCC-ee collider to detect long-lived scalar particles from exotic Higgs decays, demonstrating sensitivity to decay lengths from millimeters to meters through displaced vertex reconstruction.
Contribution
It presents a detailed sensitivity analysis for detecting long-lived scalars in Higgs decays at FCC-ee, using advanced simulation and vertex reconstruction techniques.
Findings
FCC-ee can detect long-lived scalars with decay lengths from 1 mm to 10 m.
The analysis shows high sensitivity for scalar masses of 20 and 60 GeV.
Displaced vertex reconstruction effectively suppresses Standard Model backgrounds.
Abstract
This study presents a sensitivity analysis of exotic Higgs boson decays at the electron--positron stage of the Future Circular Collider (FCC-ee), performed within the FCCAnalyses framework. The analysis investigates Higgs boson production in association with a Z boson in electron--positron collisions at a center-of-mass energy of 240~GeV. The Higgs boson is assumed to decay into a pair of long-lived scalar particles, while the Z boson decays leptonically. A hadronic final state is considered, in which the long-lived scalars subsequently decay into bottom--antibottom quark pairs. The simulation chain is implemented using the FCCAnalyses framework, with event generation performed using \textsc{MadGraph} and \textsc{Pythia}, and detector effects modeled with \textsc{Delphes}. Displaced vertices arising from the decays of long-lived particles are reconstructed using the FCCAnalyses…
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 · Particle Detector Development and Performance · Dark Matter and Cosmic Phenomena
