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In the minimal supersymmetric standard model (MSSM) the lightestsuperparticle (LSP) can be a TeV neutralino (mainly dominated by higgsino orwino) which serves as a dark matter candidate with correct thermal relicdensity. In this work we confront the 1-2 TeV neutralino dark matter with thelatest direct and indirect detections from PandaX and AMS-02/DAMPE. Consideringvarious scenarios with decoupled sfermions, with \textit{A}-mediatedannihilation, with squark or stop coannihilation, we find that the parameterspace is stringently constrained by the direct detection limits. In the allowedparameter space, the TeV neutralino dark matter annihilation contribution tothe anti-proton flux is found to agree with the AMS-02 data while itscontribution to eletron/positron flux is too small to cause any visible excess.The current survived parameter space can be mostly covered by the future directdetection experiment LZ7.2T.

TeV SUSY dark matter confronted with the current direct and indirect detection data