  We live in the golden era of cosmology due to next redshift surveys will map
a significant volume of the Universe across a wide range of redshifts. We
analyze the clustering of the eBOSS luminous red galaxy sample (eBOSS LRG). We
measure the multipole power spectra inferred from the NGC sample (107500
galaxies) and SGC sample (67316 galaxies) between redshifts 0.6 and 1.0, with
effective redshift zeff=0.695 and zeff=0.704 for NGC and SGC samples,
respectively. We use the non-linear perturbation theory to model the the
redshift space multipoles of the galaxy power spectrum.
