Astronomi gelombang kegravitian

Astronomi gelombang kegravitian (Jawi: استرونومي ݢلومبڠ کݢراۏيتين‎) ialah cabang memuncul falak cerapan yang bertujuan menggunakan gelombang kegravitian (herotan minit ruang-masa diramalkan oleh teori Albert Einstein kerelatifan am) untuk mengumpul data pemerhatian tentang objek seperti bintang neutron dan lohong hitam, peristiwa seperti supernova, dan proses termasuk yang dari alam semesta awal tidak lama selepas Letupan Besar.

Lihat juga[sunting | sunting sumber]

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^ Peters, P. (1964). "Gravitational Radiation and the Motion of Two Point Masses" (PDF). Physical Review. 136 (4B): B1224–B1232. Bibcode:1964PhRv..136.1224P. doi:10.1103/PhysRev.136.B1224.

Cutler, Curt; Thorne, Kip S. (2002), "An overview of gravitational-wave sources", dalam Bishop, Nigel; Maharaj, Sunil D. (penyunting), Proceedings of 16th International Conference on General Relativity and Gravitation (GR16), World Scientific, m/s. 4090, arXiv:gr-qc/0204090, Bibcode:2002gr.qc.....4090C, ISBN 978-981-238-171-2
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Gravitational Wave Astronomy, Max Planck Institute for Gravitational Physics, diarkibkan daripada yang asal pada 6 February 2013, dicapai pada 24 January 2013
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LIGO Magazine, LIGO Scientific Collaboration