Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band

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Post-Newtonian dynamics in dense star clusters : Binary black holes in the LISA band. / Kremer, Kyle; Rodriguez, Carl L.; Amaro-Seoane, Pau; Breivik, Katelyn; Chatterjee, Sourav; Katz, Michael L.; Larson, Shane L.; Rasio, Frederic A.; Samsing, Johan; Ye, Claire S.; Zevin, Michael.

I: Physical Review D, Bind 99, Nr. 6, 063003, 15.03.2019.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Kremer, K, Rodriguez, CL, Amaro-Seoane, P, Breivik, K, Chatterjee, S, Katz, ML, Larson, SL, Rasio, FA, Samsing, J, Ye, CS & Zevin, M 2019, 'Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band', Physical Review D, bind 99, nr. 6, 063003. https://doi.org/10.1103/PhysRevD.99.063003

APA

Kremer, K., Rodriguez, C. L., Amaro-Seoane, P., Breivik, K., Chatterjee, S., Katz, M. L., Larson, S. L., Rasio, F. A., Samsing, J., Ye, C. S., & Zevin, M. (2019). Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band. Physical Review D, 99(6), [063003]. https://doi.org/10.1103/PhysRevD.99.063003

Vancouver

Kremer K, Rodriguez CL, Amaro-Seoane P, Breivik K, Chatterjee S, Katz ML o.a. Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band. Physical Review D. 2019 mar. 15;99(6). 063003. https://doi.org/10.1103/PhysRevD.99.063003

Author

Kremer, Kyle ; Rodriguez, Carl L. ; Amaro-Seoane, Pau ; Breivik, Katelyn ; Chatterjee, Sourav ; Katz, Michael L. ; Larson, Shane L. ; Rasio, Frederic A. ; Samsing, Johan ; Ye, Claire S. ; Zevin, Michael. / Post-Newtonian dynamics in dense star clusters : Binary black holes in the LISA band. I: Physical Review D. 2019 ; Bind 99, Nr. 6.

Bibtex

@article{ba163422207c480898c1c4522d5a5f8b,
title = "Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band",
abstract = "The dynamical processing of black holes in the dense cores of globular clusters (GCs) makes them efficient factories for producing binary black holes (BBHs). Here we explore the population of BBHs that form dynamically in GCs and may be observable at mHz frequencies or higher with the future space-based gravitational-wave observatory LISA. We use our Monte Carlo stellar dynamics code, which includes gravitational radiation reaction effects for all BH encounters. By creating a representative local universe of GCs, we show that up to dozens of these systems may be resolvable by LISA. Approximately one-third of these binaries will have measurable eccentricities (e>10-3) in the LISA band, and a small number ( 5) may evolve from the LISA band to the LIGO band during the LISA mission.",
author = "Kyle Kremer and Rodriguez, {Carl L.} and Pau Amaro-Seoane and Katelyn Breivik and Sourav Chatterjee and Katz, {Michael L.} and Larson, {Shane L.} and Rasio, {Frederic A.} and Johan Samsing and Ye, {Claire S.} and Michael Zevin",
year = "2019",
month = mar,
day = "15",
doi = "10.1103/PhysRevD.99.063003",
language = "English",
volume = "99",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "6",

}

RIS

TY - JOUR

T1 - Post-Newtonian dynamics in dense star clusters

T2 - Binary black holes in the LISA band

AU - Kremer, Kyle

AU - Rodriguez, Carl L.

AU - Amaro-Seoane, Pau

AU - Breivik, Katelyn

AU - Chatterjee, Sourav

AU - Katz, Michael L.

AU - Larson, Shane L.

AU - Rasio, Frederic A.

AU - Samsing, Johan

AU - Ye, Claire S.

AU - Zevin, Michael

PY - 2019/3/15

Y1 - 2019/3/15

N2 - The dynamical processing of black holes in the dense cores of globular clusters (GCs) makes them efficient factories for producing binary black holes (BBHs). Here we explore the population of BBHs that form dynamically in GCs and may be observable at mHz frequencies or higher with the future space-based gravitational-wave observatory LISA. We use our Monte Carlo stellar dynamics code, which includes gravitational radiation reaction effects for all BH encounters. By creating a representative local universe of GCs, we show that up to dozens of these systems may be resolvable by LISA. Approximately one-third of these binaries will have measurable eccentricities (e>10-3) in the LISA band, and a small number ( 5) may evolve from the LISA band to the LIGO band during the LISA mission.

AB - The dynamical processing of black holes in the dense cores of globular clusters (GCs) makes them efficient factories for producing binary black holes (BBHs). Here we explore the population of BBHs that form dynamically in GCs and may be observable at mHz frequencies or higher with the future space-based gravitational-wave observatory LISA. We use our Monte Carlo stellar dynamics code, which includes gravitational radiation reaction effects for all BH encounters. By creating a representative local universe of GCs, we show that up to dozens of these systems may be resolvable by LISA. Approximately one-third of these binaries will have measurable eccentricities (e>10-3) in the LISA band, and a small number ( 5) may evolve from the LISA band to the LIGO band during the LISA mission.

UR - http://www.scopus.com/inward/record.url?scp=85064050626&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.99.063003

DO - 10.1103/PhysRevD.99.063003

M3 - Journal article

AN - SCOPUS:85064050626

VL - 99

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 6

M1 - 063003

ER -

ID: 236270933