Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant

We search for sterile neutrinos in the holographic dark energy cosmology by using the latest observational data. To perform the analysis, we employ the current cosmological observations, including the cosmic microwave background temperature power spectrum data from the Planck mission, the baryon acoustic oscillation measurements, the type Ia supernova data, the redshift space distortion measurements, the shear data of weak lensing observation, the Planck lensing measurement, and the latest direct measurement of H-0 as well. We show that, compared to the Lambda CDM cosmology, the holographic dark energy cosmology with sterile neutrinos can relieve the tension between the Planck observation and the direct measurement of H-0 much better. Once we include the H-0 measurement in the global fit, we find that the hint of the existence of sterile neutrinos in the holographic dark energy cosmology can be given. Under the constraint of the all-data combination, we obtain N-eff = 3.76 +/- 0.26 and m(v,sterile)(eff) < 0.215 eV, indicating that the detection of Delta N-eff > 0 in the holographic dark energy cosmology is at the 2.75 sigma level and the massless or very light sterile neutrino is favored by the current observations.