Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
ABSTRACT. In this paper, we propose a novel technique to constrain the progenitor binary black hole (BBH) formation history using the remnant masses and spins
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2019
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 482, Heft: 3, Pages: 2991-3010 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2764 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2764 Verlag, Volltext: https://academic.oup.com/mnras/article/482/3/2991/5128518 
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| Verfasserangaben: | M. Arca Sedda and M. Benacquista |
| Zusammenfassung: | ABSTRACT. In this paper, we propose a novel technique to constrain the progenitor binary black hole (BBH) formation history using the remnant masses and spins |
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| Beschreibung: | Gesehen am 15.01.2019 Advance access publication 2018 October 12 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2764 |