We present , a differentiable, -based implementation of , using internal neural network emulators to accelerate computationally costly operations for rapid large-scale structure (LSS) analysis. computes one-loop EFTofLSS predictions for redshift-space galaxy power spectrum multipoles in 1.2 ms on a CPU and 0.2 ms on a GPU, achieving 3-4 orders of magnitude speed-up over . The emulators take a compact spline-based representation of the input linear power spectrum as feature vectors, making the approach applicable to a wide range of cosmological models. We rigorously validate its accuracy against large-volume simulations and on BOSS data, including cosmologies not explicitly represented in the training set. Leveraging automatic differentiation, supports Fisher forecasting, Taylor expansion of model predictions, gradient-based searches, and vectorised ensemble sampling. Interfaced with a variety of samplers and Boltzmann solvers, provides a high-performance, end-to-end inference pipeline. Combined with a symbolic- generator, a typical Stage-4 LSS MCMC converges in minutes on a GPU. Our results demonstrate that delivers the precision and speed required for upcoming LSS surveys, opening the door to accelerated cosmological inference with minimal accuracy loss and no pretraining. In a companion paper [1], we put to use in achieving LSS marginalised constraints free from volume projection effects through non-flat measures.

生成讲解博客的中文版本

生成AI智能校验的中文版本