从伽马射线暴的飞秒透镜效应和光谱条纹看原初黑洞的特征
Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts
AI总结：
研究利用伽马射线暴的飞秒透镜效应和光谱条纹，分析原初黑洞对暗物质的影响，通过统计方法确定其质量上限。
摘要：
利用伽马射线暴的飞秒透镜效应和光谱条纹研究原初黑洞的特征，通过统计分析确定其对暗物质的影响，并得出质量上限。
英文摘要：
Femtolensing of gamma-ray bursts (GRBs) is vastly studied to constrain primordial black holes lighter than $10^{-13}$ solar mass and may close the window for PBH dark matter. In this case, wave optics formalism is required and carefully implemented in our analysis. Incorporating the GRB observational data from Swift XRT, we perform the statistical analysis of PBH lensing, comparing it with the null hypothesis where the BAND model is used to parametrize the GRB spectrum. We found a few GRB data manifest the spectral fringe which characterizes the feature of femtolensing by PBHs, and the analysis shows moderate statistical preference in terms of goodness of fit. Conversely, since most of the fits to GRB spectral data do not improve with PBH lensing, we utilize this to obtain an upper bound on the PBH fractional abundance with respect to dark matter. However, the robust constraint cannot be achieved, unless the size of GRBs is smaller than $5\times 10^7$ m for PBH mass around $5\times 10^{-15}$ solar mass.
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