TY  - JOUR
AU  - Carrasco, J.
AU  - Zurita, J.
PY  - 2024
DA  - 2024//
TI  - Emerging jet probes of strongly interacting dark sectors
T2  - J. High Energy Phys.
JO  - Journal of High Energy Physics
SP  - 034
EP  - 23pp
VL  - 01
IS  - 1
PB  - Springer
KW  - Dark Matter at Colliders
KW  - New Gauge Interactions
KW  - New Light Particles
KW  - Higgs Properties
AB  - A strongly interacting dark sector can give rise to a class of signatures dubbed dark showers, where in analogy to the strong sector in the Standard Model, the dark sector undergoes its own showering and hadronization, before decaying into Standard Model final states. When the typical decay lengths of the dark sector mesons are larger than a few centimeters (and no larger than a few meters) they give rise to the striking signature of emerging jets, characterized by a large multiplicity of displaced vertices.In this article we consider the general reinterpretation of the CMS search for emerging jets plus prompt jets into arbitrary new physics scenarios giving rise to emerging jets. More concretely, we consider the cases where the SM Higgs mediates between the dark sector and the SM, for several benchmark decay scenarios. Our procedure is validated employing the same model than the CMS emerging jet search. We find that emerging jets can be the leading probe in regions of parameter space, in particular when considering the so-called gluon portal and dark photon portal decay benchmarks. With the current 16.1 fb-1 of luminosity this search can exclude down to O\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{O} $$\end{document}(20)% exotic branching ratio of the SM Higgs, but a naive extrapolation to the 139 fb-1 luminosity employed in the current model-independent, indirect bound of 16 % would probe exotic branching ratios into dark quarks down to below 10 %. Further extrapolating these results to the HL-LHC, we find that one can pin down exotic branching ratio values of 1%, which is below the HL-LHC expectations of 2.5-4 %. We make our recasting code publicly available, as part of the LLP Recasting Repository.
SN  - 1029-8479
UR  - https://arxiv.org/abs/2307.04847
UR  - https://doi.org/10.1007/JHEP01(2024)034
DO  - 10.1007/JHEP01(2024)034
LA  - English
N1  - WOS:001137951900009
ID  - Carrasco+Zurita2024
ER  -