Built on

S. Matarrese, F. Lucchin, and S. Bonometto, “A Path Integral Approach to Large-Scale Matter Distribution Originated by Non-Gaussian Fluctuations,” Astrophys. J
1986
Earlier work this paper cites.
S. Cole and N. Kaiser, “Biased Clustering in the Cold Dark Matter Cosmogony,” Mon. Not. Roy. Astron. Soc
1989
Earlier work this paper cites.
J. Fry and E. Gaztanaga, “Biasing and Hierarchical Statistics in Large-Scale Structure,” Astrophys. J
1993
Earlier work this paper cites.
H. Mo and S. White, “An Analytic Model for the Spatial Clustering of Dark Matter Halos,” Mon. Not. Roy. Astron. Soc
1996
Earlier work this paper cites.
P. Catelan, C. Porciani, and M. Kamionkowski, “Two Ways of Biasing Galaxy Formation,” Mon. Not. Roy. Astron. Soc
2000
Earlier work this paper cites.
E. Komatsu and D. Spergel, “Acoustic Signatures in the Primary Microwave Background Bispectrum,” Phys. Rev
2001
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztañaga, and R. Scoccimarro, “Large-Scale Structure of the Universe and Cosmological Perturbation Theory,” Phys. Rep
2002
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, “Large-Scale Structure of the Universe and Cosmological Perturbation Theory,” Phys. Rept
2002
Earlier work this paper cites.
M. Alishahiha, E. Silverstein, and D. Tong, “DBI in the Sky,” Phys. Rev
2004
Earlier work this paper cites.
P. McDonald, “Clustering of Dark Matter Tracers: Renormalizing the Bias Parameters,” Phys. Rev
2006
Earlier work this paper cites.
X. Chen, M.-x. Huang, S. Kachru, and G. Shiu, “Observational Signatures and Non-Gaussianities of General Single-Field Inflation,” JCAP
2007
Earlier work this paper cites.
N. Dalal, O. Doré, D. Huterer, and A. Shirokov, “Imprints of Primordial non-Gaussianities on Large-Scale Structure: Scale-Dependent Bias and Abundance of Virialized Objects,” Phys. Rev
Original
2008
Earlier work this paper cites.
S. Matarrese and L. Verde, “The Effect of Primordial Non-Gaussianity on Halo Bias,” Astrophys. J
Original
2008
Earlier work this paper cites.
A. Slosar et al
Original
2008
Earlier work this paper cites.
P. McDonald, “Primordial Non-Gaussianity: Large-Scale Structure Signature in the Perturbative Bias Model,” Phys. Rev
Original
2008
Earlier work this paper cites.
P. McDonald and A. Roy, “Clustering of Dark Matter Tracers: Generalizing Bias for the Coming Era of Precision LSS,” JCAP
Original
2009
Earlier work this paper cites.

Similar

F. Schmidt and M. Kamionkowski, “Halo Clustering with Non-Local Non-Gaussianity,” Phys. Rev
Original
2010
Cited alongside, same era.
T. Giannantonio and C. Porciani, “Structure Formation from Non-Gaussian Initial Conditions: Multivariate Biasing, Statistics, and Comparison with N-body Simulations,” Phys. Rev
Original
2010
Cited alongside, same era.
X. Chen and Y. Wang, “Quasi-Single Field Inflation and Non-Gaussianities,” JCAP
Original
2010
Cited alongside, same era.
D. Tseliakhovich, C. Hirata, and A. Slosar, “Non-Gaussianity and Large-Scale Structure in a Two-Field Inflationary Model,” Phys. Rev
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2010
Cited alongside, same era.
V. Desjacques and U. Seljak, “Signature of Primordial Non-Gaussianity of ϕ 3 \phi^{3} -Type in the Mass Function and Bias of Dark Matter Haloes,” Phys. Rev

Then

M. Shiraishi, D. Nitta, S. Yokoyama, and K. Ichiki, “Optimal Limits on Primordial Magnetic Fields from CMB Temperature Bispectrum of Passive Modes,” JCAP
Original
2012
Later among the works it cites.
D. Jeong, F. Schmidt, and C. Hirata, “Large-Scale Clustering of Galaxies in General Relativity,” Phys. Rev
Original
2012
Later among the works it cites.
T. Giannantonio, C. Porciani, J. Carron, A. Amara, and A. Pillepich, “Constraining Primordial Non-Gaussianity with Future Galaxy Surveys,” MNRAS
Original
2012
Later among the works it cites.
K. Smith, S. Ferraro, and M. LoVerde, “Halo Clustering and g NL g_{\rm NL} -type Primordial Non-Gaussianity,” JCAP
Original
2012
Later among the works it cites.
F. Schmidt, D. Jeong, and V. Desjacques, “Peak-Background Split, Renormalization, and Galaxy Clustering,” Phys.Rev

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2015

Galaxy Bias and Primordial Non-Gaussianity

Assassi, Valentin, Baumann, Daniel, Schmidt, Fabian

Understand

We present a systematic study of galaxy biasing in the presence of primordial non-Gaussianity.

For a large class of non-Gaussian initial conditions, we define a general bias expansion and prove that it is closed under renormalization, thereby showing that the basis of operators in the expansion is complete.
We then study the effects of primordial non-Gaussianity on the statistics of galaxies.
We show that the equivalence principle enforces a relation between the scale-dependent bias in the galaxy power spectrum and that in the dipolar part of the bispectrum.

Built on

S. Matarrese, F. Lucchin, and S. Bonometto, “A Path Integral Approach to Large-Scale Matter Distribution Originated by Non-Gaussian Fluctuations,” Astrophys. J
1986
Earlier work this paper cites.
S. Cole and N. Kaiser, “Biased Clustering in the Cold Dark Matter Cosmogony,” Mon. Not. Roy. Astron. Soc
1989
Earlier work this paper cites.
J. Fry and E. Gaztanaga, “Biasing and Hierarchical Statistics in Large-Scale Structure,” Astrophys. J
1993
Earlier work this paper cites.
H. Mo and S. White, “An Analytic Model for the Spatial Clustering of Dark Matter Halos,” Mon. Not. Roy. Astron. Soc
1996
Earlier work this paper cites.
P. Catelan, C. Porciani, and M. Kamionkowski, “Two Ways of Biasing Galaxy Formation,” Mon. Not. Roy. Astron. Soc
2000
Earlier work this paper cites.
E. Komatsu and D. Spergel, “Acoustic Signatures in the Primary Microwave Background Bispectrum,” Phys. Rev
2001
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztañaga, and R. Scoccimarro, “Large-Scale Structure of the Universe and Cosmological Perturbation Theory,” Phys. Rep
2002
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, “Large-Scale Structure of the Universe and Cosmological Perturbation Theory,” Phys. Rept
2002
Earlier work this paper cites.
M. Alishahiha, E. Silverstein, and D. Tong, “DBI in the Sky,” Phys. Rev
2004
Earlier work this paper cites.
P. McDonald, “Clustering of Dark Matter Tracers: Renormalizing the Bias Parameters,” Phys. Rev
2006
Earlier work this paper cites.
X. Chen, M.-x. Huang, S. Kachru, and G. Shiu, “Observational Signatures and Non-Gaussianities of General Single-Field Inflation,” JCAP
2007
Earlier work this paper cites.
N. Dalal, O. Doré, D. Huterer, and A. Shirokov, “Imprints of Primordial non-Gaussianities on Large-Scale Structure: Scale-Dependent Bias and Abundance of Virialized Objects,” Phys. Rev
Original
2008
Earlier work this paper cites.
S. Matarrese and L. Verde, “The Effect of Primordial Non-Gaussianity on Halo Bias,” Astrophys. J
Original
2008
Earlier work this paper cites.
A. Slosar et al
Original
2008
Earlier work this paper cites.
P. McDonald, “Primordial Non-Gaussianity: Large-Scale Structure Signature in the Perturbative Bias Model,” Phys. Rev
Original
2008
Earlier work this paper cites.
P. McDonald and A. Roy, “Clustering of Dark Matter Tracers: Generalizing Bias for the Coming Era of Precision LSS,” JCAP
Original
2009
Earlier work this paper cites.