Alexander Eggemeier
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.
Authors
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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