Matches in SemOpenAlex for { <https://semopenalex.org/work/W3124756330> ?p ?o ?g. }
- W3124756330 endingPage "53" @default.
- W3124756330 startingPage "53" @default.
- W3124756330 abstract "The gravitational wave event, GW190521 is the most massive binary black hole merger observed by ground-based gravitational wave observatories LIGO/Virgo to date. While the observed gravitational-wave signal is mainly in the merger and ringdown phases, the inspiral gravitational-wave signal of GW190521-like binary will be more visible by space-based detectors in the low-frequency band. In addition, the ringdown gravitational-wave signal will be more loud with the next generation (3G) of ground-based detectors in the high-frequency band, displaying a great potential of the multiband gravitational wave observations. In this paper, we explore the scientific potential of multiband observations of GW190521-like binaries with milli-Hz gravitational wave observatory: LISA, deci-Hz observatory: B-DECIGO, and (next generation of) hecto-Hz observatories: aLIGO and ET. In the case of quasicircular evolution, the triple-band observation by LISA, B-DECIGO and ET will provide parameter estimation errors of the masses and spin amplitudes of component black holes at the level of order 1% -- 10%. This would allow consistency tests of general relativity in the strong-field at an unparalleled precision, particularly with the B-DECIGO + ET observation. In the case of eccentric evolution, the multiband signal-to-noise ratio by B-DECIGO + ET observation would be larger than 100 for a five year observation prior to coalescence, even with high final eccentricities." @default.
- W3124756330 created "2021-02-01" @default.
- W3124756330 creator A5017434183 @default.
- W3124756330 creator A5017742764 @default.
- W3124756330 creator A5043332654 @default.
- W3124756330 creator A5055106955 @default.
- W3124756330 date "2021-03-03" @default.
- W3124756330 modified "2023-10-17" @default.
- W3124756330 title "Scope Out Multiband Gravitational-Wave Observations of GW190521-Like Binary Black Holes with Space Gravitational Wave Antenna B-DECIGO" @default.
- W3124756330 cites W1731811386 @default.
- W3124756330 cites W1890730520 @default.
- W3124756330 cites W1971068715 @default.
- W3124756330 cites W1977684498 @default.
- W3124756330 cites W1981411266 @default.
- W3124756330 cites W1984180949 @default.
- W3124756330 cites W1985536898 @default.
- W3124756330 cites W1987471028 @default.
- W3124756330 cites W1989170879 @default.
- W3124756330 cites W1997367763 @default.
- W3124756330 cites W2005280645 @default.
- W3124756330 cites W2016405928 @default.
- W3124756330 cites W2024142197 @default.
- W3124756330 cites W2027523908 @default.
- W3124756330 cites W2027859446 @default.
- W3124756330 cites W2030979937 @default.
- W3124756330 cites W2031486433 @default.
- W3124756330 cites W2032765055 @default.
- W3124756330 cites W2037939815 @default.
- W3124756330 cites W2040216147 @default.
- W3124756330 cites W2052438420 @default.
- W3124756330 cites W2055125111 @default.
- W3124756330 cites W2061083933 @default.
- W3124756330 cites W2063242363 @default.
- W3124756330 cites W2064816908 @default.
- W3124756330 cites W2068755831 @default.
- W3124756330 cites W2074023319 @default.
- W3124756330 cites W2076480618 @default.
- W3124756330 cites W2089091918 @default.
- W3124756330 cites W2106027709 @default.
- W3124756330 cites W2114869293 @default.
- W3124756330 cites W2120591606 @default.
- W3124756330 cites W2121273870 @default.
- W3124756330 cites W2121634014 @default.
- W3124756330 cites W2128789282 @default.
- W3124756330 cites W2128918391 @default.
- W3124756330 cites W2134997235 @default.
- W3124756330 cites W2147829712 @default.
- W3124756330 cites W2153135464 @default.
- W3124756330 cites W2160511150 @default.
- W3124756330 cites W2163389455 @default.
- W3124756330 cites W2169650135 @default.
- W3124756330 cites W2174458751 @default.
- W3124756330 cites W2245922284 @default.
- W3124756330 cites W2252795400 @default.
- W3124756330 cites W2254226187 @default.
- W3124756330 cites W2266612357 @default.
- W3124756330 cites W2268619227 @default.
- W3124756330 cites W2273892807 @default.
- W3124756330 cites W2273991482 @default.
- W3124756330 cites W2279134017 @default.
- W3124756330 cites W2287311144 @default.
- W3124756330 cites W2299665860 @default.
- W3124756330 cites W2345330883 @default.
- W3124756330 cites W2345978248 @default.
- W3124756330 cites W2366602053 @default.
- W3124756330 cites W2415259147 @default.
- W3124756330 cites W2418431764 @default.
- W3124756330 cites W2468454158 @default.
- W3124756330 cites W2512252990 @default.
- W3124756330 cites W2528224993 @default.
- W3124756330 cites W2546409652 @default.
- W3124756330 cites W2547616757 @default.
- W3124756330 cites W2580073214 @default.
- W3124756330 cites W2597373350 @default.
- W3124756330 cites W2608556391 @default.
- W3124756330 cites W2609524736 @default.
- W3124756330 cites W2613872539 @default.
- W3124756330 cites W2613986779 @default.
- W3124756330 cites W2617090823 @default.
- W3124756330 cites W2754075545 @default.
- W3124756330 cites W2760814915 @default.
- W3124756330 cites W2778863159 @default.
- W3124756330 cites W2784753831 @default.
- W3124756330 cites W2788861935 @default.
- W3124756330 cites W2790783203 @default.
- W3124756330 cites W2801462076 @default.
- W3124756330 cites W2806591638 @default.
- W3124756330 cites W2810799428 @default.
- W3124756330 cites W2811491590 @default.
- W3124756330 cites W2870444762 @default.
- W3124756330 cites W2883722058 @default.
- W3124756330 cites W2889606121 @default.
- W3124756330 cites W2893690135 @default.
- W3124756330 cites W2901378136 @default.
- W3124756330 cites W2908886604 @default.
- W3124756330 cites W2912475769 @default.
- W3124756330 cites W2916169135 @default.
- W3124756330 cites W2931312877 @default.