Gravitational Wave detection through microlensing?

Details Gravitational Wave detection through microlensing? Gravitational Wave detection through microlensing?

2003-07-04

arxiv.org/abs/astro-ph/0307089v1

Mon.Not.Roy.Astron.Soc.345:100-110,2003

Astronomy and Astrophysics

Astrophysics

12 pages, 7 figures, to appear in Mon. Not. R. Astron. Soc

Scientific paper

10.1046/j.1365-8711.2003.06959.x

It is shown that accurate photometric observations of a relatively high--magnification microlensing event ($A\gg 1$), occurring close to the line of sight of a gravitational wave (GW) source, represented by a binary star, can allow the detection of subtle gravitational effects. After reviewing the physical nature of such effects, it is discussed to what extent these phenomena can actually be due to GWs. Expressions for the amplitude of the phenomena and the detection probability are supplied.

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