Null test of the cosmic curvature using H(z) and supernovae data 后印本

摘要: We introduce a model-independent approach to the null test of the cosmic curvature which is geometrically related to the Hubble parameter H(z) and luminosity distance dL(z). Combining the independent observations of H(z) and dL(z), we use the model-independent smoothing technique,Gaussian processes, to reconstruct them and determine the cosmic curvature (0)K in the null test relation. The null test is totally geometrical and does not assume any cosmological model. We show that the cosmic curvature (0)K = 0 is consistent with current observational data sets, falling within the 1#27; limit. To demonstrate the effect on the precision of the null test, we produce a series of simulated data of the models with different (0) K . Future observations in better quality can provide a greater improvement to constrain or refute the flat universe with (0)K = 0.