Gravitational Wave Detection by Interferometry (Ground and Space)

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Significant progress has been made in recent years on the development of gravitational-wave detectors. Sources such as coalescing compact binary systems, neutron stars in low-mass X-ray binaries, stellar collapses and pulsars are all possible candidates for detection. The most promising design of gr...

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Detalles Bibliográficos
Autores principales: Pitkin, Matthew, Reid, Stuart, Rowan, Sheila, Hough, Jim
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer International Publishing 2011
Materias:
Review Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5253843/
https://www.ncbi.nlm.nih.gov/pubmed/28163618
http://dx.doi.org/10.12942/lrr-2011-5

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5253843/
https://www.ncbi.nlm.nih.gov/pubmed/28163618
http://dx.doi.org/10.12942/lrr-2011-5

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