Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe

Understand

We constrain three cosmological models, i.e.

• the concordance cold dark matter plus a cosmological constant ($\Lambda$CDM) model, Power-law (PL) model, and $R_h=ct$ model using the available local probes, which includes the JLA compilation of type-Ia supernovae (SNe Ia), the direct measurement of Hubble constant (H(z)), and the baryon acoustic oscillations (BAO).
• For $\Lambda$CDM model, we consider two different cases, i.e.
• zero and non-zero spatial curvature.