Have hierarchical three-body mergers been detected by LIGO/Virgo?

Research output: Contribution to journalJournal articleResearchpeer-review

Standard

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 journalJournal articleResearchpeer-review

Harvard

Veske, D, Marka, Z, Sullivan, AG, Bartos, I, Corley, KR, Samsing, J & Marka, S 2020, 'Have hierarchical three-body mergers been detected by LIGO/Virgo?', Monthly Notices of the Royal Astronomical Society, vol. 498, no. 1, pp. L46-L52. https://doi.org/10.1093/mnrasl/slaa123

APA

Veske, D., Marka, Z., Sullivan, A. G., Bartos, I., Corley, K. R., Samsing, J., & Marka, S. (2020). Have hierarchical three-body mergers been detected by LIGO/Virgo? Monthly Notices of the Royal Astronomical Society, 498(1), L46-L52. https://doi.org/10.1093/mnrasl/slaa123

Vancouver

Veske D, Marka Z, Sullivan AG, Bartos I, Corley KR, Samsing J et al. Have hierarchical three-body mergers been detected by LIGO/Virgo? Monthly Notices of the Royal Astronomical Society. 2020 Oct 11;498(1):L46-L52. https://doi.org/10.1093/mnrasl/slaa123

Author

Veske, Doga ; Marka, Zsuzsa ; Sullivan, Andrew G. ; Bartos, Imre ; Corley, K. Rainer ; Samsing, Johan ; Marka, Szabolcs. / Have hierarchical three-body mergers been detected by LIGO/Virgo?. In: Monthly Notices of the Royal Astronomical Society. 2020 ; Vol. 498, No. 1. pp. L46-L52.

Bibtex

@article{47f21cacd9d24d249d1be2887531b443,
title = "Have hierarchical three-body mergers been detected by LIGO/Virgo?",
abstract = "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.",
keywords = "gravitational waves, (transients:) black hole mergers, BLACK-HOLE MERGERS, GLOBULAR-CLUSTERS, EVOLUTION, BINARIES, CATALOG, TESTS, LIGO",
author = "Doga Veske and Zsuzsa Marka and Sullivan, {Andrew G.} and Imre Bartos and Corley, {K. Rainer} and Johan Samsing and Szabolcs Marka",
year = "2020",
month = oct,
day = "11",
doi = "10.1093/mnrasl/slaa123",
language = "English",
volume = "498",
pages = "L46--L52",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "1",

}

RIS

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