A gravitational wave detector like LIGO or Virgo has two orthogonal arms with laser beams bouncing off mirrors that are made to interfere destructively in the intersection of the arms. A gravitational wave will shrink one arm by a (tiny) amount delta(t) and stretch the other by delta(t). The shrink and stretch  vary periodically with a frequency of the order of kHz to be detectable. One would (naively) expect to get a signal varying like

sin(4delta(t)/lambda_{laser})  = ~ 4delta(t)/lambda       

(the factor 4 comes from the two arms each giving a contribution delta and and the two armlength the light travels as it bounces back from the mirror).

However, what one really measures is the difference in wavenumber (i.e the difference between the two arms of the number of wavelength between  twice  the intersection and the mirror modulo one i.e. phase difference ) between the standing light waves in the two arms.  My problem is that the gravitational wave also changes the propagation of electromagnetic waves, and I don't see why the wavelength of the laser light in the two directions is not shrunk and stretched by the same proportion (at least to first order which is the only thing one might hope to measure) so that if we continue this line of thought, the wave numbers in the two directions of the beam line should actually be the same (to first order) with or without the GW and no interference signal would be detected. Note that in the kHz band the wavelength of the GW is of the order of 300 km so is essentially constant over the whole (km's sized) detector. 

It seems more than likely that something is wrong in my mental picture but I'd like to know what. 

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