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Relativistic dynamics and extreme mass ratio inspirals
It is now well-established that a dark, compact object, very likely a massive black hole (MBH) of around four million solar masses is lurking at the centre of the Milky Way. While a consensus is emerging about the origin and growth of supermassive black holes (with masses larger than a billion solar...
Autor principal: | Amaro-Seoane, Pau |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer International Publishing
2018
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5954169/ https://www.ncbi.nlm.nih.gov/pubmed/29780279 http://dx.doi.org/10.1007/s41114-018-0013-8 |
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