With the advent of next-generation surveys, constraints on cosmological parameters are anticipated to become more stringent, particularly for the total neutrino mass. This study forecasts such constraints utilizing galaxy clusters from the Chinese Space Station Survey Telescope (CSST). Employing Fisher matrix techniques, we derive the constraint $\sigma (M_{\nu })$ from cluster number counts, cluster power spectrum, and their combination. The investigation covers both the standard cosmological model with massive neutrinos $\nu \mathrm{\Lambda }\mathrm{CDM}$ and the inclusion of dynamical dark energy in the $\nu w_0{w}_a\mathrm{CDM}$ model, revealing a minor impact of dark energy on neutrino mass constraints. We examine the largest source of systematic arising from the mass-observable relation uncertainties and find that, with perfect knowledge of the scaling relation parameters, CSST clusters have the potential to enhance precision, tightening constraints to $\sim 0.03\mathrm{eV}$. We also study the effects of the maximum redshift $z_{\max }$ and other uncertainties, including those in redshift, halo mass function, and bias. Furthermore, we emphasize the significance of accounting for the growth-induced scale-dependent bias effect, which we find can tighten the final constraint by a factor of 1.2–2.2.

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• Cosmology
• Dark energy
• Large scale structure of the Universe
• Galaxy clusters
• Neutrino mass