Population III binary black holes with chirp mass of ~30 Msun and detectability of the quasi-normal mode with frequency ~200 Hz to confirm or refute the Einstein’s gravity theory in the strong gravity region
Population III binary black holes with chirp mass of ~30 Msun and detectability of the quasi-normal mode with frequency ~200 Hz to confirm or refute the Einstein’s gravity theory in the strong gravity region
复制标题
啁啾质量~30 Msun的族群III双黑洞和频率~200 Hz的准正则模式的可探测性，以证实或反驳爱因斯坦在强引力区的引力理论
DOI：
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发表时间：
2015
期刊：
影响因子：
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通讯作者：
T. Nakamura
中科院分区：
文献类型：
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作者：
T. Kinugawa;A. Miyamoto;N. Kanada;T. Nakamura
