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The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to current data, but few statistically significant tensions and anomalies were found in the latest data analyses. While these could be due presence of systematic errors experiments, they also indicate need for new physics beyond model. In this Letter Interest we focus on tension between Planck weak lensing measurements redshift surveys, value matter energy density Ωm amplitude σ8 (or growth rate fσ8) cosmic structure. We list promising models solving tension, discuss importance trying multiple datasets with complete physical models, rather than fitting individual handpicked theoretical parameters.