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A. Vasudevan, M. M. Ivanov, S. Sibiryakov and J. Lesgourgues, Time-sliced perturbation theory with primordial non-Gaussianity and effects of large bulk flows on inflationary oscillating features , JCAP 09
Original
1906
Earlier work this paper cites.
A. Chudaykin and M. M. Ivanov, Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error , JCAP 11
Original
1907
Earlier work this paper cites.
A. Oddo, E. Sefusatti, C. Porciani, P. Monaco and A. G. Sánchez, Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection , JCAP 03
Original
1908
Earlier work this paper cites.
C. Hahn, F. Villaescusa-Navarro, E. Castorina and R. Scoccimarro, Constraining M ν M_{\nu} with the bispectrum. Part I. Breaking parameter degeneracies , JCAP 03
Original
1909
Earlier work this paper cites.
M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters from the BOSS Galaxy Power Spectrum , JCAP 05
Original
1909
Earlier work this paper cites.
G. D’Amico, J. Gleyzes, N. Kokron, D. Markovic, L. Senatore, P. Zhang et al., The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 1909.05271
Original
1909
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O. H. E. Philcox and D. J. Eisenstein, Estimating Covariance Matrices for Two- and Three-Point Correlation Function Moments in Arbitrary Survey Geometries , Mon. Not. Roy. Astron. Soc. 490
Original
1910
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A. Lewis, GetDist: a Python package for analysing Monte Carlo samples , 1910.13970
Original
1910
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1911
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O. H. E. Philcox and D. J. Eisenstein, Computing the Small-Scale Galaxy Power Spectrum and Bispectrum in Configuration-Space , Mon. Not. Roy. Astron. Soc. 492
Original
1912
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M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data , Phys. Rev. D 101
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1912
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H. Gil-Marín, L. Verde, J. Noreña, A. J. Cuesta, L. Samushia, W. J. Percival et al., The power spectrum and bispectrum of SDSS DR11 BOSS galaxies – II. Cosmological interpretation , Mon. Not. Roy. Astron. Soc. 452
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1972
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R. Scoccimarro and J. Frieman, Loop corrections in nonlinear cosmological perturbation theory , Astrophys. J. Suppl. 105
1996
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R. Scoccimarro, S. Colombi, J. N. Fry, J. A. Frieman, E. Hivon and A. Melott, Nonlinear evolution of the bispectrum of cosmological perturbations , Astrophys. J. 496
1998
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R. Scoccimarro, H. M. P. Couchman and J. A. Frieman, The Bispectrum as a Signature of Gravitational Instability in Redshift-Space , Astrophys. J. 517
1999
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R. Scoccimarro, The bispectrum: from theory to observations , Astrophys. J. 544
2000
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R. Scoccimarro, H. A. Feldman, J. N. Fry and J. A. Frieman, The Bispectrum of IRAS redshift catalogs , Astrophys. J. 546
2001
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H. A. Feldman, J. A. Frieman, J. N. Fry and R. Scoccimarro, Constraints on galaxy bias, matter density, and primordial non-gausianity from the PSCz galaxy redshift survey , Phys. Rev. Lett. 86
2001
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2002
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2002
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2002
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O. H. E. Philcox, M. M. Ivanov, M. Simonović and M. Zaldarriaga, Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6\% CMB-independent constraint on H 0 , JCAP 05
Original
2002
Earlier work this paper cites.
G. D’Amico, L. Senatore and P. Zhang, Limits on w w CDM from the EFTofLSS with the PyBird code , JCAP 01
Original
2003
Earlier work this paper cites.
T. Nishimichi, G. D’Amico, M. M. Ivanov, L. Senatore, M. Simonović, M. Takada et al., Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum , Phys. Rev. D 102
Original
2003
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A. Chudaykin, M. M. Ivanov, O. H. E. Philcox and M. Simonović, Nonlinear perturbation theory extension of the Boltzmann code CLASS , Phys. Rev. D 102
Original
2004
Earlier work this paper cites.
R. Scoccimarro, Redshift-space distortions, pairwise velocities and nonlinearities , Phys. Rev. D70
2004
Earlier work this paper cites.
O. H. E. Philcox, A faster Fourier transform? Computing small-scale power spectra and bispectra for cosmological simulations in 𝒪 ⁡ ( N 2 ) \mathcal{O}(N^{2}) time , Mon. Not. Roy. Astron. Soc. 501
Original
2005
Earlier work this paper cites.
E. Gaztanaga and R. Scoccimarro, The 3-point function in large scale structure: Redshift distortions and galaxy bias , Mon. Not. Roy. Astron. Soc. 361
2005
Earlier work this paper cites.

Similar

Y. Kobayashi, T. Nishimichi, M. Takada, R. Takahashi and K. Osato, Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum , Phys. Rev. D 102
Original
2005
Cited alongside, same era.
S.-F. Chen, Z. Vlah and M. White, Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory , JCAP 07
Original
2005
Cited alongside, same era.
M. M. Ivanov, Y. Ali-Haïmoud and J. Lesgourgues, H0 tension or T0 tension? , Phys. Rev. D 102
Original
2005
Cited alongside, same era.
E. Sefusatti, M. Crocce, S. Pueblas and R. Scoccimarro, Cosmology and the Bispectrum , Phys. Rev. D74
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Then

L. Senatore, Bias in the Effective Field Theory of Large Scale Structures , JCAP 1511
Original
2015
Later among the works it cites.
R. Angulo, M. Fasiello, L. Senatore and Z. Vlah, On the Statistics of Biased Tracers in the Effective Field Theory of Large Scale Structures , JCAP 1509
Original
2015
Later among the works it cites.
M. Mirbabayi, F. Schmidt and M. Zaldarriaga, Biased Tracers and Time Evolution , JCAP 1507
Original
2015
Later among the works it cites.
M. Schmittfull, T. Baldauf and U. Seljak, Near optimal bispectrum estimators for large-scale structure , Phys. Rev. D91
Original
2015
Later among the works it cites.
L. Senatore and M. Zaldarriaga, The IR-resummed Effective Field Theory of Large Scale Structures , JCAP 1502

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2021

Precision analysis of the redshift-space galaxy bispectrum

Ivanov, Mikhail M., Philcox, Oliver H. E., Nishimichi, Takahiro et al.

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We study the information content of the angle-averaged (monopole) redshift space galaxy bispectrum.

The main novelty of our approach is the use of a systematic tree-level perturbation theory model that includes galaxy bias, IR resummation, and also accounts for nonlinear redshift space distortions, binning, and projection effects.
We analyze data from the PT challenge simulations, whose cumulative volume of 566 $h^{-3}$Gpc$^3$ allows for a precise comparison to theoretical predictions.
Fitting the power spectrum and bispectrum of our simulated data, and varying all necessary cosmological and nuisance parameters in a consistent Markov chain Monte Carlo analysis, we find that our tree-level bispectrum model is valid up to $k_{\max}=0.08~h{\rm Mpc}^{-1}$ (at $z=0.61$).