Model-independent constraints on cosmic curvature: implication from updated Hubble diagram of high-redshift standard candles

Understand

The cosmic curvature ($\Omega_k$) is a fundamental parameter for cosmology.

• In this paper, we propose an improved model-independent method to constrain the cosmic curvature, which is geometrically related to the Hubble parameter $H(z)$ and luminosity distance $D_L(z)$.
• Using the currently largest $H(z)$ sample from the well-known cosmic chronometers, as well as the luminosity distance $D_L(z)$ from the relation between the UV and X-ray luminosities of 1598 quasars and the newly-compiled Pantheon sample including 1048 SNe Ia, 31 independent measurements of the cosmic curvature $\Omega_k(z)$ can be expected covering the redshift range of $0.07<z<2$.
• Our estimation of $\Omega_k(z)$ is fully compatible with flat Universe at the current level of observational precision.