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General and explicit predictions from the integrated perturbation theory(iPT) for power spectra and correlation functions of biased tracers are derivedand presented in the one-loop approximation. The iPT is a general framework ofthe nonlinear perturbation theory of cosmological density fields in presence ofnonlocal bias, redshift-space distortions, and primordial non-Gaussianity.Analytic formulas of auto and cross power spectra of nonlocally biased tracersin both real and redshift spaces are derived and the results arecomprehensively summarized. The main difference from previous formulas derivedby the present author is to include effects of generally nonlocal Lagrangianbias and primordial non-Gaussianity, and the derivation method of the newformula is fundamentally different from the previous one. Relations to recentwork on improved methods of nonlinear perturbation theory in literature areclarified and discussed.

Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers