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

机译:Galaxy BISPectrum的多层技术:对非局部原始非高斯的限制应用

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摘要

We explore the use of galaxy bispectra with the multitracer technique as a possible probe of primordial non-Gaussianities. We forecast future constraints on non-linearity parameters, f_(NL)~(eq) and f_(NL)~(orth) , which, respectively, characterize the equilateral- and orthogonal-type 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 the galaxy bispectrum by future galaxy surveys can reach the constraints on the nonlocal-type primordial non-Gaussianities to the level more severe than current one which has been obtained by cosmic microwave background observations.
机译:我们探索了Galaxy Bispectra与多种间隔技术作为原始非高斯的可能探针。我们预测非线性参数的未来限制,F_(NL)〜(EQ)和F_(NL)〜(oRTH),它们分别表征等边和正交式原始BISPECTRA,并表明多型分析将是如果Galaxies的数量密度足够高,则有效地减少宇宙 - 方差噪声。我们发现,未来的星系调查的Galaxy BiSpectrum的测量可以达到非本体型原始非高斯的限制,而不是通过宇宙微波背景观测获得的电流更严重的水平。

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  • 来源
    《Physical Review D》 |2017年第8期|063530.1-063530.6|共6页
  • 作者单位

    Faculty of Engineering Kanagawa University Kanagawa 221-8686 Japan;

    Department of Physics Rikkyo University Tokyo 171-8501 Japan;

    Faculty of Science Kumamoto University 2-39-1 Kurokami Kumamoto 860-8555 Japan;

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