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Gravitational-wave asteroseismology with fundamental modes from compact binary inspirals
Gravitational waves (GWs) from binary neutron stars encode unique information about ultra-dense matter through characterisic signatures associated with a variety of phenomena including tidal effects during the inspiral. The main tidal signature depends predominantly on the equation of state (EoS)-re...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2020
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7242351/ https://www.ncbi.nlm.nih.gov/pubmed/32439905 http://dx.doi.org/10.1038/s41467-020-15984-5 |