Observability of gravitational waves excited by binary stars orbiting around a supermassive black hole by space-based gravitational wave observatory
Abstract We produce the gravitational waveforms for the extreme mass ratio inspiral systems (EMRIs) of binary stars moving around central supermassive black hole (SBH), or called B-EMRIs. We calculate the external orbits of the binary stars via the commonly used Hamilton–Jacobi (HJ) approach, and ca...
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| Autors principals: | , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
SpringerOpen
2026-03-01
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| Col·lecció: | European Physical Journal C: Particles and Fields |
| Accés en línia: | https://doi.org/10.1140/epjc/s10052-026-15455-z |
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