Accelerated binary black holes in globular clusters: forecasts and detectability in the era of space-based gravitational-wave detectors Article Swipe
Avinash Tiwari
,
A. Vijaykumar
,
S. J. Kapadia
,
Giacomo Fragione
,
Sourav Chatterjee
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stad3749
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stad3749
The motion of the centre of mass of a coalescing binary black hole (BBH) in a gravitational potential, imprints a line-of-sight acceleration (LOSA) on to the emitted gravitational-wave (GW) signal. The acceleration could be sufficiently large in dense stellar environments, such as globular clusters (GCs), to be detectable with next-generation space-based detectors. In this work, we use outputs of the cluster monte carlo (cmc) simulations of dense star clusters to forecast the distribution of detectable LOSAs in DECIGO and LISA eras. We study the effect of cluster properties – metallicity, virial and galactocentric radii – on the distribution of detectable accelerations, account for cosmologically motivated distributions of cluster formation times, masses, and metallicities, and also incorporate the delay time between the formation of BBHs and their merger in our analysis. We find that larger metallicities provide a larger fraction of detectable accelerations by virtue of a greater abundance of relatively lighter BBHs, which allow a higher number of GW cycles in the detectable frequency band. Conversely, smaller metallicities result in fewer detections, most of which come from relatively more massive BBHs with fewer cycles but larger LOSAs. We similarly find correlations between the virial radii of the clusters and the fractions of detectable accelerations. Our work, therefore, provides an important science case for space-based GW detectors in the context of probing GC properties via the detection of LOSAs of merging BBHs.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/stad3749
- https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad3749/54042175/stad3749.pdf
- OA Status
- hybrid
- Cited By
- 12
- References
- 113
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4389427925
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Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4389427925Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/stad3749Digital Object Identifier
- Title
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Accelerated binary black holes in globular clusters: forecasts and detectability in the era of space-based gravitational-wave detectorsWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
-
2023Year of publication
- Publication date
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2023-11-27Full publication date if available
- Authors
-
Avinash Tiwari, A. Vijaykumar, S. J. Kapadia, Giacomo Fragione, Sourav ChatterjeeList of authors in order
- Landing page
-
https://doi.org/10.1093/mnras/stad3749Publisher landing page
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad3749/54042175/stad3749.pdfDirect link to full text PDF
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YesWhether a free full text is available
- OA status
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hybridOpen access status per OpenAlex
- OA URL
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad3749/54042175/stad3749.pdfDirect OA link when available
- Concepts
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Physics, Globular cluster, Astrophysics, Binary black hole, Gravitational wave, Star cluster, Virial theorem, Context (archaeology), Metallicity, Cluster (spacecraft), Astronomy, Galaxy, Paleontology, Programming language, Biology, Computer scienceTop concepts (fields/topics) attached by OpenAlex
- Cited by
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12Total citation count in OpenAlex
- Citations by year (recent)
-
2025: 8, 2024: 4Per-year citation counts (last 5 years)
- References (count)
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113Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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