
This research paper introduces a novel, dark energy model-independent method for determining the spatial curvature of the universe (Ω𝐾) by parameterizing the comoving radial distance and utilizing data from Baryon Acoustic Oscillations, Type Ia Supernovae, and Observational Hubble Data.


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A New Method for Determining the Spatial Curvature of the Universe Independently of Dark Energy Parameterization
