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

机译:Lyman-alpha森林数据和流体动力学模拟对模糊暗物质的第一个约束

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摘要

We present constraints on the masses of extremely light bosons dubbed fuzzy dark matter from Lyman-a forest data. Extremely light bosons with a De Broglie wavelength of similar to 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-alpha a flux power spectrum in these models and compare with 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 IGM that allow for jumps in the temperature of up to 5000K, XQ-100 provides a lower limit of 7.1x10(-22) eV, HIRES/MIKE returns a stronger limit of 14.3x10(-22) eV, while the combination of both data sets results in a limit of 20 x10(-22) eV (2s C.L.). The limits for the analysis of the combined data sets increases to 37.5x10(-22) eV (2s 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 1-10x10(-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
机译:我们从莱曼森林数据中提出了对被称为模糊暗物质的极轻玻色子的质量的约束。有人建议将De Broglie波长类似于1 kpc的极轻玻色子作为候选暗物质,以解决当前冷暗物质模型的一些小规模问题。我们首次使用流体动力学模拟对这些模型中的Lyman-αa磁通功率谱建模,并与来自两个不同数据集的观测到的磁通功率谱进行比较:XQ-100和HIRES / MIKE类星体谱样本。在对干扰和物理参数进行边缘化处理之后,并且对IGM的热历史进行了保守的假设(允许温度跃升至5000K),XQ-100的下限为7.1x10(-22)eV,HIRES / MIKE返回上限为14.3x10(-22)eV,而两个数据集的组合得出的上限为20 x10(-22)eV(2s CL)。当假定IGM的温度随着红移的幂律而变化时,假设热历史更平稳,则组合数据集的分析极限将增加到37.5x10(-22)eV(2s C.L.)。我们的分析排除了在1-10x10(-22)eV范围内的轻玻色子质量具有很高的意义,这使人们强烈怀疑FDM有助于解决冷暗物质模型的“小规模危机”

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  • 来源
    《Physical review letters》 |2017年第3期|031302.1-031302.7|共7页
  • 作者单位

    Univ Washington, Dept Astron, 3910 15th Ave Northeast, Seattle, WA 98195 USA|Inst Adv Study, 1 Einstein Dr, Princeton, NJ 08540 USA|Abdus Salam Int Ctr Theoret Phys, Str Costiera 11, I-34151 Trieste, Italy;

    SISSA Int Sch Adv Studies, Via Bonomea 265, I-34136 Trieste, Italy|INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy|Ist Nazl Fis Nucl, Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy;

    Inst Astron, Madingley Rd, Cambridge CB3 0HA, England|Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England;

    Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England;

    Inst Astron, Madingley Rd, Cambridge CB3 0HA, England|Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England|Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA;

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