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A NEW MEASURE OF σ8 USING THE LENSING DISPERSION IN HIGH-z TYPE Ia SUPERNOVAE

机译:利用高z型Ia超新星的透镜色散测量σ8

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摘要

The gravitational lensing magnification or demagnification due to large-scale structures induces a scatter in peak magnitudes of high-redshift Type Ia supernovae (SNe Ia). The amplitude of the lensing dispersion strongly depends on that of density fluctuations characterized by the σ_8 parameter. Therefore the value of σ_8 is constrained by measuring the dispersion in the peak magnitudes. We examine how well SN Ia data will provide a constraint on the value of σ_8 using a likelihood analysis method. It is found that the number and quality of SN Ia data needed for placing a useful constraint on σ _8 is attain- able with the Next Generation Space Telescope.
机译:由于大型结构而引起的引力透镜放大或缩小会导致高红移Ia型超新星(SNe Ia)的峰值幅度发生散射。透镜色散的幅度在很大程度上取决于以σ_8参数为特征的浓度波动的幅度。因此,通过测量峰值幅度的离散度来限制σ_8的值。我们使用似然分析方法检查SN Ia数据对σ_8值的约束程度。发现使用下一代太空望远镜可以获得对σ_8施加有用约束所需的SN Ia数据的数量和质量。

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