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来自莱曼α森林数据和流体动力学模拟对模糊暗物质的首次限制。

First Constraints on Fuzzy Dark Matter from Lyman-α Forest Data and Hydrodynamical Simulations.

作者信息

Iršič Vid, Viel Matteo, Haehnelt Martin G, Bolton James S, Becker George D

机构信息

University of Washington, Department of Astronomy, 3910 15th Avenue Northeast, Seattle, Washington 98195-1580, USA.

Institute for Advanced Study, 1 Einstein Drive, Princeton, New Jersey 08540, USA.

出版信息

Phys Rev Lett. 2017 Jul 21;119(3):031302. doi: 10.1103/PhysRevLett.119.031302. Epub 2017 Jul 20.

DOI:10.1103/PhysRevLett.119.031302
PMID:28777592
Abstract

We present constraints on the masses of extremely light bosons dubbed fuzzy dark matter (FDM) from Lyman-α forest data. Extremely light bosons with a de Broglie wavelength of ∼1  kpc have been suggested as dark matter candidates that may resolve some of the current small scale problems of the cold dark matter model. For the first time, we use hydrodynamical simulations to model the Lyman-α flux power spectrum in these models and compare it to the observed flux power spectrum from two different data sets: the XQ-100 and HIRES/MIKE quasar spectra samples. After marginalization over nuisance and physical parameters and with conservative assumptions for the thermal history of the intergalactic medium (IGM) that allow for jumps in the temperature of up to 5000 K, XQ-100 provides a lower limit of 7.1×10^{-22}  eV, HIRES/MIKE returns a stronger limit of 14.3×10^{-22}  eV, while the combination of both data sets results in a limit of 20×10^{-22}  eV (2σ C.L.). The limits for the analysis of the combined data sets increases to 37.5×10^{-22}  eV (2σ C.L.) when a smoother thermal history is assumed where the temperature of the IGM evolves as a power law in redshift. Light boson masses in the range 1-10×10^{-22}  eV are ruled out at high significance by our analysis, casting strong doubts that FDM helps solve the "small scale crisis" of the cold dark matter models.

摘要

我们根据莱曼-α森林数据给出了被称为模糊暗物质(FDM)的极轻玻色子质量的限制。具有约1千秒差距德布罗意波长的极轻玻色子已被提议作为暗物质候选者,它们可能解决当前冷暗物质模型的一些小尺度问题。我们首次使用流体动力学模拟对这些模型中的莱曼-α通量功率谱进行建模,并将其与来自两个不同数据集(XQ - 100和HIRES/MIKE类星体光谱样本)观测到的通量功率谱进行比较。在对讨厌参数和物理参数进行边缘化处理,并对星系际介质(IGM)的热历史做出保守假设(允许温度跃升高达5000 K)后,XQ - 100给出了7.1×10⁻²² eV的下限,HIRES/MIKE给出了更强的14.3×10⁻²² eV的限制,而两个数据集的组合给出了20×10⁻²² eV(2σ置信水平)的限制。当假设更平滑的热历史(其中IGM的温度随红移呈幂律演化)时,组合数据集分析的限制增加到37.5×10⁻²² eV(2σ置信水平)。我们的分析在高显著性水平上排除了1 - 10×10⁻²² eV范围内的轻玻色子质量,这强烈质疑了FDM有助于解决冷暗物质模型的“小尺度危机”。

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