Test the growth models of black hole by jointing LIGO and Insight-HXMT observations
Rong-Jia Yang, Zhiwei Guo, Yaoguang Zheng, Shuang-Nan Zhang

TL;DR
This paper tests two black hole growth models using combined LIGO and Insight-HXMT data, finding the stationary model inconsistent with observations, thus providing insights into black hole evolution.
Contribution
It introduces a joint observational approach to distinguish between stationary and time-dependent black hole growth models.
Findings
Stationary growth model is inconsistent with observational data.
Time-dependent growth model aligns better with observations.
Joint LIGO and Insight-HXMT data effectively tests black hole growth theories.
Abstract
The growth model of black hole is still a controversial topic. In the stationary metric, all in-falling matter must be accumulated outside the event horizon of the black hole, as clocked by a distant external observer. In the time-dependent metric, all in-falling matter can fall into the event horizon of the final black hole within very short time. We test these two growth models by joining LIGO and Insight-HXMT observations. We find the stationary model is inconsistent with LIGO and Insight-HXMT observations.
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