Catalog variance of testing general relativity with gravitational-wave data

被引:2
|
作者
Pacilio, Costantino [1 ,2 ]
Gerosa, Davide [1 ,2 ,3 ,4 ]
Bhagwat, Swetha [3 ,4 ]
机构
[1] Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
[2] Ist Nazl Fis Nucl, Sez Milano Bicocca, Piazza Sci 3, I-20126 Milan, Italy
[3] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, England
[4] Univ Birmingham, Inst Gravitat Wave Astron, Birmingham B15 2TT, England
基金
欧洲研究理事会;
关键词
PARAMETERS;
D O I
10.1103/PhysRevD.109.L081302
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Combining multiple gravitational-wave observations allows for stringent tests of general relativity, targeting effects that would otherwise be undetectable using single-event analyses. We highlight how the finite size of the observed catalog induces a significant source of variance. If not appropriately accounted for, general relativity can be excluded with arbitrarily large credibility even if it is the underlying theory of gravity. This effect is generic and holds for arbitrarily large catalogs. Moreover, we show that it cannot be suppressed by selecting "golden" observations with large signal-to-noise ratios. We present a mitigation strategy based on bootstrapping (i.e. resampling with repetition) that allows assigning uncertainties to one's credibility on the targeted test. We demonstrate our findings using both toy models and real gravitationalwave data. In particular, we quantify the impact of the catalog variance on the ringdown properties of black holes using the latest LIGO/Virgo catalog.
引用
收藏
页数:6
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