
本文提出了一種基於迭代密度估計的新方法，用於從重力波觀測中重建合併黑洞雙星的質量分佈，發現雙星質量比並不如先前研究所認為的那樣傾向於接近相等，且質量比分佈會隨著主星質量的變化而改變。


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基於迭代密度估計的合併黑洞雙星質量分佈

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This research introduces a novel iterative density estimation method to accurately reconstruct the mass distribution of merging black hole binaries from gravitational wave observations, revealing a weaker preference for near-equal mass binaries than previously thought and suggesting a more complex relationship between primary and secondary black hole masses.


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Estimating the Mass Distribution of Merging Black Hole Binaries from Gravitational Wave Observations Using an Iterative Density Estimation Method
