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- W4283639800 abstract "Measuring the quasi-normal mode~(QNM) spectrum emitted by a perturbed black-hole~(BH) --~also known as BH spectroscopy~-- provides an excellent opportunity to test the predictions of general relativity in the strong-gravity regime. We investigate the prospects and precision of BH spectroscopy in massive binary black hole ringdowns, one of the primary science objectives of the future Laser Interferometric Space Antenna~(LISA) mission. We simulate various massive binary BH population models, featuring competing prescriptions for the Delays between galaxy and BH mergers, for the impact of supernova feedback on massive BH growth, and for the initial population of high redshift BH seeds (light versus heavy seeds). For each of these scenarios, we compute the average number of expected events for precision BH spectroscopy using a Fisher-matrix analysis. We find that, for any heavy seed scenario, LISA will measure the dominant mode frequency within ${cal O}(0.1) %$ relative uncertainty and will estimate at least 3 independent QNM parameters within $1 %$ error. The most optimistic heavy seed scenarios produce $mathcal{O}(100)$ events with $1 %$ measurability for 3 or more QNM quantities during LISA's operational time. On the other hand, light seed scenarios produce lighter merger remnants, which ring at frequencies higher than LISA's sensitivity. Interestingly, the light seed models give rise to a fraction of mergers in the band of Einstein Telescope, allowing for the measurement of 3 QNM parameters with $sim 10 %$ relative errors in approximately a few to ten events/yr. More precise BH spectroscopy in the light seed scenarios would require instruments operating in the deciHertz band." @default.
- W4283639800 created "2022-06-29" @default.
- W4283639800 creator A5016911084 @default.
- W4283639800 creator A5025182918 @default.
- W4283639800 creator A5049026088 @default.
- W4283639800 creator A5050737016 @default.
- W4283639800 date "2022-06-28" @default.
- W4283639800 modified "2023-10-10" @default.
- W4283639800 title "Landscape of massive black-hole spectroscopy with LISA and the Einstein Telescope" @default.
- W4283639800 cites W1631788275 @default.
- W4283639800 cites W1939384555 @default.
- W4283639800 cites W1967852555 @default.
- W4283639800 cites W1969449998 @default.
- W4283639800 cites W1973368884 @default.
- W4283639800 cites W1996169450 @default.
- W4283639800 cites W2004499374 @default.
- W4283639800 cites W2010218176 @default.
- W4283639800 cites W2012886609 @default.
- W4283639800 cites W2014804681 @default.
- W4283639800 cites W2023746249 @default.
- W4283639800 cites W2024532173 @default.
- W4283639800 cites W2027523908 @default.
- W4283639800 cites W2030007862 @default.
- W4283639800 cites W2031486433 @default.
- W4283639800 cites W2032317739 @default.
- W4283639800 cites W2040216147 @default.
- W4283639800 cites W2042181581 @default.
- W4283639800 cites W2050092976 @default.
- W4283639800 cites W2055524364 @default.
- W4283639800 cites W2060191906 @default.
- W4283639800 cites W2069764580 @default.
- W4283639800 cites W2072815594 @default.
- W4283639800 cites W2084852948 @default.
- W4283639800 cites W2090459210 @default.
- W4283639800 cites W2096659135 @default.
- W4283639800 cites W2097783118 @default.
- W4283639800 cites W2098266183 @default.
- W4283639800 cites W2103857591 @default.
- W4283639800 cites W2104494725 @default.
- W4283639800 cites W2113893006 @default.
- W4283639800 cites W2116923776 @default.
- W4283639800 cites W2118840719 @default.
- W4283639800 cites W2128808878 @default.
- W4283639800 cites W2134997235 @default.
- W4283639800 cites W2144890838 @default.
- W4283639800 cites W2147829712 @default.
- W4283639800 cites W2154231449 @default.
- W4283639800 cites W2164387557 @default.
- W4283639800 cites W2165603825 @default.
- W4283639800 cites W2167086789 @default.
- W4283639800 cites W2169650135 @default.
- W4283639800 cites W2170924363 @default.
- W4283639800 cites W2179996778 @default.
- W4283639800 cites W2268619227 @default.
- W4283639800 cites W2273892807 @default.
- W4283639800 cites W2287311144 @default.
- W4283639800 cites W2343385133 @default.
- W4283639800 cites W2417863416 @default.
- W4283639800 cites W2418431764 @default.
- W4283639800 cites W2419016325 @default.
- W4283639800 cites W2489062076 @default.
- W4283639800 cites W2502015268 @default.
- W4283639800 cites W2513152708 @default.
- W4283639800 cites W2520787834 @default.
- W4283639800 cites W2580073214 @default.
- W4283639800 cites W2746963572 @default.
- W4283639800 cites W2748435155 @default.
- W4283639800 cites W2754340245 @default.
- W4283639800 cites W2754352294 @default.
- W4283639800 cites W2763316094 @default.
- W4283639800 cites W2783246754 @default.
- W4283639800 cites W2799244439 @default.
- W4283639800 cites W2801462076 @default.
- W4283639800 cites W2889606121 @default.
- W4283639800 cites W2890935589 @default.
- W4283639800 cites W2896371533 @default.
- W4283639800 cites W2903518599 @default.
- W4283639800 cites W2942867706 @default.
- W4283639800 cites W2962876006 @default.
- W4283639800 cites W2973189566 @default.
- W4283639800 cites W2981083955 @default.
- W4283639800 cites W2982489998 @default.
- W4283639800 cites W2982542617 @default.
- W4283639800 cites W2982902439 @default.
- W4283639800 cites W2987251817 @default.
- W4283639800 cites W3003742949 @default.
- W4283639800 cites W3021397378 @default.
- W4283639800 cites W3037269817 @default.
- W4283639800 cites W3038756136 @default.
- W4283639800 cites W3047115840 @default.
- W4283639800 cites W3090096711 @default.
- W4283639800 cites W3095529157 @default.
- W4283639800 cites W3096163345 @default.
- W4283639800 cites W3098197608 @default.
- W4283639800 cites W3099471130 @default.
- W4283639800 cites W3099518669 @default.
- W4283639800 cites W3100187076 @default.
- W4283639800 cites W3100244417 @default.
- W4283639800 cites W3102496762 @default.
- W4283639800 cites W3102598661 @default.