Have hierarchical three-body mergers been detected by LIGO/Virgo?
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Have hierarchical three-body mergers been detected by LIGO/Virgo? / Veske, Doga; Marka, Zsuzsa; Sullivan, Andrew G.; Bartos, Imre; Corley, K. Rainer; Samsing, Johan; Marka, Szabolcs.
In: Monthly Notices of the Royal Astronomical Society, Vol. 498, No. 1, 11.10.2020, p. L46-L52.Research output: Contribution to journal › Journal article › Research › peer-review
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TY - JOUR
T1 - Have hierarchical three-body mergers been detected by LIGO/Virgo?
AU - Veske, Doga
AU - Marka, Zsuzsa
AU - Sullivan, Andrew G.
AU - Bartos, Imre
AU - Corley, K. Rainer
AU - Samsing, Johan
AU - Marka, Szabolcs
PY - 2020/10/11
Y1 - 2020/10/11
N2 - One of the proposed channels of binary black holemergers involves dynamical interactions of three black holes. In such scenarios, it is possible that all three black holes merge in a so-called hierarchical merger chain, where two of the black holes merge first and then their remnant subsequently merges with the remaining single black hole. Depending on the dynamical environment, it is possible that both mergers will appear within the observable time window. Here, we perform a search for such merger pairs in the public available LIGO and Virgo data from the O1/O2 runs. Using a frequentist p-value assignment statistics, we do not find any significant merger pair candidates, the most significant being GW170809-GW151012 pair. Assuming no observed candidates in O3/O4, we derive upper limits on merger pairs to be similar to 11-110 yr(-1) Gpc(-3), corresponding to a rate that relative to the total merger rate is similar to 0.1-1.0. From this, we argue that both a detection and a non-detection within the next few years can be used to put useful constraints on some dynamical progenitor models.
AB - One of the proposed channels of binary black holemergers involves dynamical interactions of three black holes. In such scenarios, it is possible that all three black holes merge in a so-called hierarchical merger chain, where two of the black holes merge first and then their remnant subsequently merges with the remaining single black hole. Depending on the dynamical environment, it is possible that both mergers will appear within the observable time window. Here, we perform a search for such merger pairs in the public available LIGO and Virgo data from the O1/O2 runs. Using a frequentist p-value assignment statistics, we do not find any significant merger pair candidates, the most significant being GW170809-GW151012 pair. Assuming no observed candidates in O3/O4, we derive upper limits on merger pairs to be similar to 11-110 yr(-1) Gpc(-3), corresponding to a rate that relative to the total merger rate is similar to 0.1-1.0. From this, we argue that both a detection and a non-detection within the next few years can be used to put useful constraints on some dynamical progenitor models.
KW - gravitational waves
KW - (transients:) black hole mergers
KW - BLACK-HOLE MERGERS
KW - GLOBULAR-CLUSTERS
KW - EVOLUTION
KW - BINARIES
KW - CATALOG
KW - TESTS
KW - LIGO
U2 - 10.1093/mnrasl/slaa123
DO - 10.1093/mnrasl/slaa123
M3 - Journal article
VL - 498
SP - L46-L52
JO - Royal Astronomical Society. Monthly Notices
JF - Royal Astronomical Society. Monthly Notices
SN - 0035-8711
IS - 1
ER -
ID: 252878140