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Analysis

This paper presents a novel approach to modeling biased tracers in cosmology using the Boltzmann equation. It offers a unified description of density and velocity bias, providing a more complete and potentially more accurate framework than existing methods. The use of the Boltzmann equation allows for a self-consistent treatment of bias parameters and a connection to the Effective Field Theory of Large-Scale Structure.
Reference

At linear order, this framework predicts time- and scale-dependent bias parameters in a self-consistent manner, encompassing peak bias as a special case while clarifying how velocity bias and higher-derivative effects arise.