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Testing one-loop galaxy bias: Joint analysis of power spectrum and bispectrum

Eggemeier, Alexander; Scoccimarro, Román; Smith, Robert E.; Crocce, Martin; Pezzotta, Andrea; Sánchez, Ariel G.

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Authors

Alexander Eggemeier

Román Scoccimarro

Robert E. Smith

Martin Crocce

Andrea Pezzotta

Ariel G. Sánchez



Abstract

We present a joint likelihood analysis of the real-space power spectrum and bispectrum measured from a variety of halo and galaxy mock catalogs. A novel aspect of this work is the inclusion of nonlinear triangle configurations for the bispectrum, made possible by a complete next-to-leading order (“one-loop”) description of galaxy bias, as is already common practice for the power spectrum. Based on the goodness of fit and the unbiasedness of the parameter posteriors, we accomplish a stringent validation of this model compared to the leading order (“tree-level”) bispectrum. Using measurement uncertainties that correspond to an effective survey volume of 6 ðGpc=hÞ3, we determine that the one-loop corrections roughly double the applicable range of scales, from ∼0.17 h=Mpc (tree level) to ∼0.3 h=Mpc. This converts into a 1.5–2x improvement on constraints of the linear bias parameter at fixed cosmology, and a 1.5–2.4x shrinkage of uncertainties on the amplitude of fluctuations As, which clearly demonstrates the benefit of extracting information from nonlinear scales despite having to marginalize over a larger number of bias parameters. Besides, our precise measurements of galaxy bias parameters up to fourth order allow for thorough comparisons to coevolution relations, showing excellent agreement for all contributions generated by the nonlocal action of gravity. Using these relations in the likelihood analysis does not compromise the model validity and is crucial for obtaining the quoted improvements on As. We also analyzed the impact of higherderivative and scale-dependent stochastic terms, finding that for a subset of our tracers the former can boost the performance of the tree-level model with constraints on As that are only slightly degraded compared to the one-loop model.

Citation

Eggemeier, A., Scoccimarro, R., Smith, R. E., Crocce, M., Pezzotta, A., & Sánchez, A. G. (2021). Testing one-loop galaxy bias: Joint analysis of power spectrum and bispectrum. Physical Review D, 103(12), Article 123550. https://doi.org/10.1103/physrevd.103.123550

Journal Article Type Article
Acceptance Date Jun 3, 2021
Online Publication Date Jun 30, 2021
Publication Date 2021
Deposit Date Nov 16, 2021
Publicly Available Date Nov 17, 2021
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 103
Issue 12
Article Number 123550
DOI https://doi.org/10.1103/physrevd.103.123550
Public URL https://durham-repository.worktribe.com/output/1221685

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Copyright Statement
Reprinted with permission from the American Physical Society: Eggemeier, Alexander, Scoccimarro, Román, Smith, Robert E., Crocce, Martin, Pezzotta, Andrea & Sánchez, Ariel G. (2021). Testing one-loop galaxy bias: Joint analysis of power spectrum and bispectrum. Physical Review D 103(12): 123550. © 2021 by the American Physical Society. Readers may view, browse, and/or download material for temporary copying purposes only, provided these uses are for noncommercial personal purposes. Except as provided by law, this material may not be further reproduced, distributed, transmitted, modified, adapted, performed, displayed, published, or sold in whole or part, without prior written permission from the American Physical Society.






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