期刊
LIVING REVIEWS IN RELATIVITY
卷 26, 期 1, 页码 -出版社
SPRINGER INT PUBL AG
DOI: 10.1007/s41114-023-00044-3
关键词
Gravitational waves; Gravitational-wave detectors; Gravitational-wave sources
As the detection of gravitational wave signals from the merger of compact binary stars in other galaxies has become routine, it is interesting to explore other potential gravitational wave signatures. This article examines the possibilities of discovering continuous gravitational waves from fast-spinning neutron stars in our own galaxy and from more exotic sources. It reviews potential continuous wave sources, presents search methodologies and results, and discusses the prospects of imminent discovery.
Now that detection of gravitational-wave signals from the coalescence of extra-galactic compact binary star mergers has become nearly routine, it is intriguing to consider other potential gravitational-wave signatures. Here we examine the prospects for discovery of continuous gravitational waves from fast-spinning neutron stars in our own galaxy and from more exotic sources. Potential continuous-wave sources are reviewed, search methodologies and results presented and prospects for imminent discovery discussed.
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