Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries

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To be observed and analyzed by the network of gravitational wave detectors on ground (LIGO, VIRGO, etc.) and by the future detectors in space (eLISA, etc.), inspiralling compact binaries — binary star systems composed of neutron stars and/or black holes in their late stage of evolution — require hig...

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Detalles Bibliográficos
Autor principal: Blanchet, Luc
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer International Publishing 2014
Materias:
Review Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5256563/
https://www.ncbi.nlm.nih.gov/pubmed/28179846
http://dx.doi.org/10.12942/lrr-2014-2

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5256563/
https://www.ncbi.nlm.nih.gov/pubmed/28179846
http://dx.doi.org/10.12942/lrr-2014-2

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