The Origin of the Nano-Hertz Stochastic Gravitational-wave Background: The Contribution from z ≳ 1 Supermassive Black Hole Binaries
The nano-Hertz gravitational wave background (GWB) is a key probe of supermassive black hole (SMBH) formation and evolution if the background arises predominantly from SMBH binaries (SMBHBs). The GWB amplitude, which is typically quantified as the characteristic strain, A _yr at a frequency 1 yr ^−1...
-д хадгалсан:
| Үндсэн зохиолчид: | , |
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| Формат: | Artigo |
| Хэл сонгох: | Inglês |
| Хэвлэсэн: |
IOP Publishing
2025-01-01
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| Цуврал: | The Astrophysical Journal |
| Нөхцлүүд: | |
| Онлайн хандалт: | https://doi.org/10.3847/1538-4357/adbc62 |
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