Squeezing fNL out of the matter bispectrum with consistency relations
High Energy Physics - Theory
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
High Energy Physics - Theory (hep-th)
FOS: Physical sciences
Primordial non-gaussianity, consistency relations, large scale structures
General Relativity and Quantum Cosmology (gr-qc)
General Relativity and Quantum Cosmology
Astrophysics - Cosmology and Nongalactic Astrophysics
DOI:
10.1103/physrevd.106.123525
Publication Date:
2022-12-29T15:02:21Z
AUTHORS (7)
ABSTRACT
We show how consistency relations can be used to robustly extract the amplitude of local primordial non-Gaussianity (${f}_{\mathrm{NL}}$) from squeezed limit matter bispectrum, well into nonlinear regime. First, we derive a nonperturbative relation between and leading term in revising some results present literature. This is then successfully measure ${f}_{\mathrm{NL}}$ $N$-body simulations. discuss dependence our on different scale cuts redshifts. Specifically, analysis strongly dependent choice smallest soft momentum, ${q}_{\mathrm{min}}$, which most sensitive bispectrum contributions, but largely independent largest hard ${k}_{\mathrm{max}}$, due non-Gaussian nature covariance. also constraints improve at higher redshift, reduced off-diagonal In particular, for simulation with ${f}_{\mathrm{NL}}=100$ volume $(2.4\text{ }\text{ }\mathrm{Gpc}/h{)}^{3}$, ${f}_{\mathrm{NL}}=98\ifmmode\pm\else\textpm\fi{}12$ redshift $z=0$ ${f}_{\mathrm{NL}}=97\ifmmode\pm\else\textpm\fi{}8$ $z=0.97$. Finally, compare Fisher forecast, showing that current version satisfactorily close error. regard this as first step towards realistic application constrain using observations.
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