1992
DOI: 10.1088/0264-9381/9/5/019
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Effect of a weak plane GW on a light beam

Abstract: The effect of a weak plane gravitational wave on a beam of light is analysed by solving Maxwell's electromagnetic equations in a curved background geometry. The results are applied to the consideration of the function of laser-interferometric GW antennae.

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Cited by 30 publications
(46 citation statements)
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“…It can however be made precise by the following considerations, which are studied in depth in references [22] and [23].…”
Section: Interferometric Gw Detectorsmentioning
confidence: 99%
See 1 more Smart Citation
“…It can however be made precise by the following considerations, which are studied in depth in references [22] and [23].…”
Section: Interferometric Gw Detectorsmentioning
confidence: 99%
“…As shown in reference [22], we need not worry about either ε 0 (ωt) or ε 1 (ωt) at this stage because the longitudinal component of the electric field (i.e., E x ) is an order of approximation smaller than the transverse components, which are given by…”
Section: Test Light Beams In a Gw-warped Space-timementioning
confidence: 99%
“…Provided that the wave length of the GW is large compared to the wave length of the light signal, we will use the eikonal or geometrical optics approximation to describe the interaction of the light in gravitational waves. The propagation of the electromagnetic waves in the field of gravitational waves was considered many times and we can refer the reader to several papers dealing with this questions in the geometrical optics approximation [7,21,22,23,24,25]. Our subsequent analysis of this problem will be carried out in close analogy with the paper of Sazhin and Maslova [25], where they have considered the structure of electromagnetic field in Fabry-Perot resonator in the field of gravitational waves.…”
Section: Propagation Of Light Near the Localized Source Of Gravitatiomentioning
confidence: 99%
“…For example, as stressed in reference [22], its range of validity is not limited to interferometer arms short compared to the GW wavelength. Therefore, according to the formula, a null effect (signal cancellation) happens if the round trip time τ equals the period of the GW, 2π/ω.…”
Section: Test Light Beams In a Gw-warped Space-timementioning
confidence: 99%
“…If incidence is instead oblique then a significant damping factor of sin 4 θ comes in, where θ is the angle between the GW direction and the cylinder's axis [24] 8 . This is a severe penalty, and it also happens in interferometric detectors not optimally oriented [22,31].…”
Section: Cylindersmentioning
confidence: 99%