Local Primordial Non-Gaussian Bias at the Field Level
James M. Sullivan, Shi-Fan Chen

TL;DR
This paper measures local primordial non-Gaussian bias parameters at the field level using simulations, compares them with theoretical predictions, and discusses implications for constraining primordial non-Gaussianity in galaxy surveys.
Contribution
First field-level measurement of bias parameters related to local primordial non-Gaussianity using N-body simulations, with analysis of their impact on constraining $f_{NL}^{(loc)}$.
Findings
Qualitative consistency with universality and separate universe predictions.
Marginalizing over bias parameters degrades $f_{NL}^{(loc)}$ constraints by 2-3 times.
Biases in $f_{NL}^{(loc)}$ constraints due to degeneracies with bias parameters.
Abstract
Local primordial non-Gaussianity (LPNG) couples long-wavelength cosmological fluctuations to the short-wavelength behavior of galaxies. This coupling is encoded in bias parameters including and at linear and quadratic order in the large-scale biasing framework. We perform the first field-level measurement of and using Lagrangian bias and non-linear displacements from N-body simulations. We compare our field level measurements with universality predictions and separate universe results, finding qualitative consistency, but disagreement in detail. We also quantify the information on available in the field given various assumptions on knowledge of at fixed initial conditions. We find that it is not possible to precisely constrain when marginalizing over…
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Taxonomy
TopicsForecasting Techniques and Applications · Risk and Portfolio Optimization · Financial Risk and Volatility Modeling
