The CMSSM survives Planck, the LHC, LUX-ZEPLIN, Fermi-LAT, H.E.S.S. and IceCube

Ellis, John; Olive, Keith A.; Spanos, Vassilis C.; Stamou, Ioanna D.

doi:10.1140/epjc/s10052-023-11405-1

Title: The CMSSM survives Planck, the LHC, LUX-ZEPLIN, Fermi-LAT, H.E.S.S. and IceCube

Journal Article · 22 March 2023 · European Physical Journal. C, Particles and Fields (Online)

DOI: https://doi.org/10.1140/epjc/s10052-023-11405-1 · OSTI ID:2234271

Ellis, John ^[1]; Olive, Keith A. ^[2]; Spanos, Vassilis C. ^[3]; Stamou, Ioanna D. ^[4]

King’s College London (United Kingdom); European Organization for Nuclear Research (CERN), Geneva (Switzerland); National Institute of Chemical Physics and Biophysics, Tallinn (Estonia); FTPI, University of Minnesota
University of Minnesota, Minneapolis, MN (United States)
National and Kapodistrian University of Athens (Greece)
Université Libre de Bruxelles, Brussels (Belgium)

We revisit the viability of the CMSSM, searching for regions of parameter space that yield a neutralino dark matter density compatible with Planck measurements, as well as LHC constraints including sparticle searches and the mass of the Higgs boson, recent direct limits on spin-independent and -dependent dark matter scattering from the LUX-ZEPLIN (LZ) experiment, the indirect constraints from Fermi-LAT and H.E.S.S. on dark matter annihilations to photons in dwarf spheroidal galaxies and the Galactic Centre, and the IceCube limits on muons from annihilations to neutrinos in the Sun. For representative values of tan β and A₀ we map in detail the Planck-compatible strips in CMSSM parameter planes, which exhibit multiple distinctive features for large tan β, A₀ = 0 and μ > 0, and identify portions of the strips that survive all the phenomenological constraints. We find that the most powerful constraint is that from m_h, followed by the LZ limit on spin-independent scattering, whereas sparticle searches at the LHC and indirect dark matter searches are less restrictive. Most of the surviving CMSSM parameter space features a Higgsino-like dark matter particle with a mass ~ 1000–1100 GeV, which could best be probed with future direct searches for dark matter scattering.

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Research Organization:: University of Minnesota, Minneapolis, MN (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: SC0011842

OSTI ID:: 2234271

Journal Information:: European Physical Journal. C, Particles and Fields (Online), Journal Name: European Physical Journal. C, Particles and Fields (Online) Journal Issue: 3 Vol. 83; ISSN 1434-6052

Publisher:: Springer NatureCopyright Statement

Country of Publication:: United States

Language:: English

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Cosmological dark matter annihilations into γ rays: A closer look Ullio, Piero; Bergström, Lars; Edsjö, Joakim Physical Review D, Vol. 66, Issue 12 https://doi.org/10.1103/PhysRevD.66.123502	journal	December 2002
Neutralino relic density including coannihilations Edsjö, Joakim; Gondolo, Paolo Physical Review D, Vol. 56, Issue 4 https://doi.org/10.1103/PhysRevD.56.1879	journal	August 1997

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