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- W2982460677 abstract "Recent theoretical advances have provided an analytical expression for the Q of gravitationally-small sources of gravitational radiation, along lines similar to the Wheeler-Chu limit for electrically-small antennas. This paper presents the first published results using this new theory to analyze the Q of a black-hole inspiral, using observed transient gravitational wave data from the GW170608 black-hole merger. Despite the astronomical scale of a radiation source comprised of two black holes having upwards of 7 solar masses each, the GW170608 binary black hole is shown to be a gravitationally-small high-Q radiator at the very low frequencies of the gravitational waves." @default.
- W2982460677 created "2019-11-08" @default.
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- W2982460677 date "2019-07-01" @default.
- W2982460677 modified "2023-09-24" @default.
- W2982460677 title "Observed Q and Gravitationally-Small Antenna Behavior of a Binary Black Hole Radiator" @default.
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- W2982460677 doi "https://doi.org/10.1109/apusncursinrsm.2019.8889298" @default.
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