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Multitracer technique for galaxy bispectrum - An application to constraints on non-local primordial non-Gaussianities -

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arxiv 1611.03590 v2 pith:W74SQXCH submitted 2016-11-11 astro-ph.CO

classification astro-ph.CO
keywords galaxyprimordialconstraintsmultitracernon-gaussianitiesbispectrabispectrumfuture
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abstract

We explore the use of galaxy bispectra with multitracer technique as a possible probe of primordial non-Gaussianities. We forecast future constraints on non-linearity parameters, $f_{\rm NL}^{\rm eq}$ and $f_{\rm NL}^{\rm orth}$, which respectively characterize the equilateral- and orthogonal-types primordial bispectra, and show that the multitracer analysis would be effective with reducing the cosmic-variance noise if the number density of galaxies is high enough. We find that the measurement of galaxy bispectrum by future galaxy surveys can reach the constraints on the non-local type primordial non-Gaussianities to the level severer than current one which has been obtained by cosmic microwave background observations.

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Forward citations

Cited by 3 Pith papers

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    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    UNIONS Lyman-break galaxy auto-clustering is unusable at large scales due to imaging systematics, but LBG x CMB-lensing and LBG x quasar cross-spectra are measured robustly, with amplitudes consistent with predictions.

  2. Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy

    astro-ph.CO 2026-03 conditional novelty 6.0 of 10

    DDE sound modes induce scale-dependent growth and halo bias comparable to massless neutrinos; multi-tracer P+B forecasts detect it for c_s^{2} ~ 10^{-2}–10^{-4}, while lower speeds produce ~10% drag on cluster growth-...

  3. Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection

    astro-ph.CO 2019-08 accept novelty 6.0 of 10

    For dark matter halos at z=1, a tree-level three-parameter bias model with Poissonian shot noise describes the halo bispectrum up to k about 0.08 h/Mpc, and Bayesian model selection disfavours local Eulerian and Lagra...

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