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The recently sharpened H_0 tension is argued not to be a result of datacalibration or other systematic but an indication for the common nature of darkmatter and dark energy. This conclusion is devised within modified weak-fieldGeneral Relativity where the accelerated expansion of the Universe and thedynamics of galaxy groups and clusters are described by the same parameter, thecosmological constant. The common nature of the dark sector hence will resultin intrinsic discrepancy/tension between the local and global determinations ofvalues of the Hubble constant.

H_0 tension: clue to common nature of dark sector?