Application of the sample copula of order m in the estimation of cosmological parameters

Key Points

• Key findings demonstrate the effectiveness of sample copula in estimating cosmological parameters accurately, enhancing reliability in cosmological analysis.
• An improvement in estimation methods was shown through statistical comparisons, with notable accuracy metrics reported.
• Application of m-order copula provided a robust framework for analyzing complex dependencies in cosmological datasets.
• These findings indicate potential advancements in theoretical frameworks guiding future cosmological studies, requiring further investigation.