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- W4288705899 abstract "The framework of the so-called 3-3-1LHN model accommodates two different, but viable, scenarios of dark matter. In one case, the dark matter particle is a heavy Dirac neutrino ${N}_{1}$. In the other case, we have a scalar, $ensuremath{phi}$, as a dark matter candidate. In both cases, the dark matter phenomenology, relic abundance, and scattering cross section off of nuclei are controlled by exchange of ${Z}^{ensuremath{'}}$. We then investigate the impact on the parameter space $({M}_{{Z}^{ensuremath{'}}},{M}_{({N}_{1},ensuremath{phi})})$ due to the recent PandaX-4T experimental result in both scenarios. We obtain that the PandaX-4T experiment excludes scenarios with dark matter mass below 1.9 TeV. Concerning ${Z}^{ensuremath{'}}$, we find the lower bound ${M}_{{Z}^{ensuremath{'}}}>4.1text{ }text{ }mathrm{TeV}$ for the case where ${N}_{1}$ is the dark matter and ${M}_{{Z}^{ensuremath{'}}}>5.7text{ }text{ }mathrm{TeV}$ for the other case. This implies that the 3-3-1 symmetry is spontaneously broken above 10 TeV scale. We also comment on the contributions to the relic abundance of processes involving flavor-changing neutral current mediated by ${Z}^{ensuremath{'}}$." @default.
- W4288705899 created "2022-07-30" @default.
- W4288705899 creator A5012418676 @default.
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- W4288705899 date "2022-07-29" @default.
- W4288705899 modified "2023-09-27" @default.
- W4288705899 title "PandaX-4T limits on <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mrow><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math> mass in 3-3-1LHN model" @default.
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- W4288705899 doi "https://doi.org/10.1103/physrevd.106.015031" @default.
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