DC pole | Wartość | Język |
dc.contributor.author | Liao, Kai | - |
dc.contributor.author | Biesiada, Marek | - |
dc.contributor.author | Fan, Xi-Long | - |
dc.date.accessioned | 2019-06-06T09:30:01Z | - |
dc.date.available | 2019-06-06T09:30:01Z | - |
dc.date.issued | 2019 | - |
dc.identifier.citation | Astrophysical Journal, Vol. 875 (2019), Art. No. 139 | pl_PL |
dc.identifier.issn | 0004-637X | - |
dc.identifier.issn | 1538-4357 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12128/9390 | - |
dc.description.abstract | Gravitational wave predicted by general relativity is the transverse wave of spatial strain. Several gravitational
waveform signals from binary black holes and from a binary neutron star system accompanied by electromagnetic
counterparts have been recorded by the advanced Laser Interferometer Gravitational-Wave Observatory (LIGO)
and the advanced Virgo. In analogy to light, the spatial fringes of diffraction and interference should also exist as
the important features of gravitational waves (GWs). We propose that observational detection of such fringes could
be achieved through gravitational lensing of continuous GWs. The lenses would play the role of the diffraction
barriers. Considering peculiar motions of the observer, the lens, and the source, the spatial amplitude variation of
diffraction or interference fringes should be detectable as an amplitude modulation of a monochromatic
gravitational signal. | pl_PL |
dc.language.iso | en | pl_PL |
dc.rights | Uznanie autorstwa 3.0 Polska | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/pl/ | * |
dc.subject | gravitational lensing | pl_PL |
dc.subject | micro - gravitational waves | pl_PL |
dc.title | The Wave Nature of Continuous Gravitational Waves from Microlensing | pl_PL |
dc.type | info:eu-repo/semantics/article | pl_PL |
dc.identifier.doi | 10.3847/1538-4357/ab1087 | - |
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