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Is Light Neutralino Thermal Dark Matter in the Phenomenological Minimal Supersymmetric Standard Model Ruled Out?

Rahool Kumar Barman, Geneviève Bélanger, Biplob Bhattacherjee, Rohini M. Godbole, and Rhitaja Sengupta
Phys. Rev. Lett. 131, 011802 – Published 6 July 2023
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Abstract

We explore the parameter space of the phenomenological minimal supersymmetric standard model with a light neutralino thermal dark matter (mχ˜10mh/2) that is consistent with current collider and astrophysical constraints. We consider both positive and negative values of the higgsino mass parameter (μ). Our investigation shows that the recent experimental results from the LHC as well as from direct detection searches for dark matter by the LUX-ZEPLIN Collaboration rule out the Z-funnel region for the μ>0 scenario. The same results severely restrict the h-funnel region for positive μ; however, the allowed points can be probed easily with few more days of data from the LUX-ZEPLIN experiment. In the μ<0 scenario, we find that very light higgsinos in both the Z and h funnels might survive the present constraints from the electroweakino searches at the LHC, and dedicated efforts from experimental collaborations are necessary to make conclusive statements about their present status.

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  • Received 26 July 2022
  • Revised 2 May 2023
  • Accepted 25 May 2023

DOI:https://doi.org/10.1103/PhysRevLett.131.011802

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Rahool Kumar Barman1,*, Geneviève Bélanger2,†, Biplob Bhattacherjee3,‡, Rohini M. Godbole3,§, and Rhitaja Sengupta3,∥

  • 1Department of Physical Sciences, Oklahoma State University, Stillwater, Oklahoma 74078, USA
  • 2LAPTh, Université Savoie Mont Blanc, CNRS, 9 Chemin de Bellevue, 74940 Annecy, France
  • 3Centre for High Energy Physics, Indian Institute of Science, Bangalore 560012, India

  • *Corresponding author. rahool.barman@okstate.edu
  • Corresponding author. belanger@lapth.cnrs.fr
  • Corresponding author. biplob@iisc.ac.in
  • §Corresponding author. rohini@iisc.ac.in
  • Corresponding author. rhitaja@iisc.ac.in

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Vol. 131, Iss. 1 — 7 July 2023

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  • Figure 1
    Figure 1

    Scaled SI DM-nucleon cross section (σSI×ξ) for μ>0 (upper) and μ<0 (center), along with scaled SD DM-neutron cross section (σSDn×ξ) for μ<0 (lower) as a function of the mass of the LSP neutralino DM in the region of parameter space satisfying LEP, flavor, Higgs constraints, relic density, DM DD constraints from the XENON-1T, PICO-60, and PandaX-4T experiments: “Before LZ” in yellow circles, “After LZ” in light green circles, overlayed with additional constraints from electroweakino searches at the LHC (in dark green circles). The current experimental limits from PandaX-4T and LZ are shown (solid lines) as well as projections for LZ 1000 days and XENON-nT (dashed lines).

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  • Figure 2
    Figure 2

    Allowed parameter space for μ>0 (top) and μ<0 (bottom) after satisfying the LEP, flavor, Higgs constraints, relic density DM DD constraints from the XENON-1T, PICO-60, and PandaX-4T experiments: “Before LZ” in yellow circles, “After LZ” in light green circles, overlayed with additional constraints from electroweakino searches at the LHC (in dark green circles) in the mχ˜10mχ˜20 plane.

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