TY - GEN
T1 - Gravitational waves from precessing black hole-neutron star mergers
AU - Kawaguchi, Kyohei
AU - Kyutoku, Kotarou
AU - Nakano, Hiroyuki
AU - Okawa, Hirotada
AU - Shibata, Masaru
AU - Taniguchi, Keisuke
N1 - Publisher Copyright:
© Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. All rights reserved.
Copyright:
Copyright 2021 Elsevier B.V., All rights reserved.
PY - 2015
Y1 - 2015
N2 - The QA+ method can be useful for separating the effect of the orbital precession from the precessing BHNS waveforms in the merger phase. • The QA+ waveforms may have some connection to the non-precessing BHNS waveforms. • The dependence of cutoff frequency on the NS compactness is clearly seen in the QA+ spectra.
AB - The QA+ method can be useful for separating the effect of the orbital precession from the precessing BHNS waveforms in the merger phase. • The QA+ waveforms may have some connection to the non-precessing BHNS waveforms. • The dependence of cutoff frequency on the NS compactness is clearly seen in the QA+ spectra.
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M3 - Conference contribution
AN - SCOPUS:85092243835
T3 - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
SP - 297
EP - 303
BT - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
PB - Kyoto University, Yukawa Institute for Theoretical Physics
T2 - 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Y2 - 7 December 2015 through 11 December 2015
ER -