Página principal > CMS Collection > CMS Preprints > A search for light Higgs bosons from supersymmetric cascade decays in proton-proton collisions at 13 TeV |
CMS Physics Analysis Summaries | |
Report number | CMS-PAS-HIG-20-018 |
Title | A search for light Higgs bosons from supersymmetric cascade decays in proton-proton collisions at 13 TeV |
Corporate author(s) | CMS Collaboration |
Collaboration | CMS Collaboration |
Subject category | Particle Physics - Experiment |
Accelerator/Facility, Experiment | CERN LHC ; CMS |
Abstract | A search for pairs of boosted light Higgs bosons ($\mathrm{H}_1$) produced in supersymmetric cascade decays is performed in final states with small missing transverse momentum. The complete LHC Run II proton-proton collision data set is used, recorded with the CMS detector at a centre-of-mass energy of $13~\mathrm{TeV}$ and corresponding to an integrated luminosity of $137~\mathrm{fb}^{-1}$. The search targets events where both $\mathrm{H}_1$ bosons decay into $\mathrm{b}\bar{\mathrm{b}}$ pairs that are reconstructed as large-radius jets using substructure techniques. No evidence is found for any excess of events beyond the background expectations of the standard model (SM). Results from the search are interpreted in the next-to-minimal supersymmetric extension of the SM, where a low-mass singlino leads to multi-step squark and gluino decays that can predominantly end with a boosted singlet-like $\mathrm{H}_1$ boson and a low-momentum singlino-like neutralino. Upper limits are set on the product of the squark or gluino pair-production cross section and the $\mathrm{b}\bar{\mathrm{b}}$ branching ratio of the $\mathrm{H}_1$ for a benchmark model with almost mass-degenerate light flavour squarks and gluinos. Under the assumption of an SM-like $\mathrm{H}_1\to\mathrm{b}\bar{\mathrm{b}}$ branching ratio, $\mathrm{H}_1$ bosons with masses in the range 40--120 GeV, arising from the decays of squarks or gluinos with a mass from 1200--2500 GeV, are excluded at the $95\%$ confidence level. |
Other source | Inspire |
Related | superseded by: CERN-EP-2022-010 |
Email contact: [email protected] Fulltext in PDF Figure_010 Figure_009-b Figure_009-c Figure_009-a Figure_008 Figure_007 Figure_006 Figure_005-c Figure_005-b Figure_005-a Figure_004 Figure_003 Figure_002 Figure_001 Figure_005-d Additional information for the analysis (restricted access) |