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State-resolved integral cross sections and corresponding thermal rate coefficients are computed for the HD + ortho-/para-H2 rotational energy transfer collision at low temperatures of astrophysical interest: 2 K ≲ T ≲ 300 K. A recent original full-dimensional H2-H2 potential energy surface (PES) was adopted and appropriately modified for the current non-symmetrical four-atomic system

HD +ortho-/para-H2rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K