LZ reports no WIMP detection in 60 live days with 5.5 t exposure and sets a new spin-independent limit of 9.2×10^{-48} cm² at 36 GeV/c².
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LZ reports a null result from 4.2 tonne-year exposure and sets new world-leading upper limits on spin-independent WIMP-nucleon cross sections reaching 2.2e-48 cm2 at 40 GeV.
In f(R,Σ,T) gravity with logarithmic Om(z) parameterization, the model produces quintessence dark energy that drives acceleration without phantom crossing but exhibits classical instability.
citing papers explorer
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First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
LZ reports no WIMP detection in 60 live days with 5.5 t exposure and sets a new spin-independent limit of 9.2×10^{-48} cm² at 36 GeV/c².
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Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment
LZ reports a null result from 4.2 tonne-year exposure and sets new world-leading upper limits on spin-independent WIMP-nucleon cross sections reaching 2.2e-48 cm2 at 40 GeV.
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Dark Energy Phenomenology in a $f(R,\Sigma,T)$ Gravity Framework: $O_m(z)$ Parameterization Approach
In f(R,Σ,T) gravity with logarithmic Om(z) parameterization, the model produces quintessence dark energy that drives acceleration without phantom crossing but exhibits classical instability.