Calculating the Period of Fringe Pattern for Michelson Interferometer

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In a Michelson Interferometer, moving Mirror 1 by a distance Δd=λ0/2 results in a path difference of λ0, causing each fringe to shift to the position of an adjacent fringe. The relationship Δd=m(λ0/2) is crucial for understanding fringe movement. The intensity equation I0=2I0 - 2I0 cos(2kdL or 2wt) indicates that fringes shift by a phase of 2kdL or 2wt. The discussion highlights a need for clarity on how to apply the given wavelength and mirror displacement to calculate the period of the fringe pattern. Understanding these principles is essential for accurate calculations in interferometry.
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Homework Statement
Given the wavelength of the beam of light, and the displacement of one of the mirrors, how would one go about finding the fraction of a period the fringe pattern will move as a result of the mirror displacement?
Relevant Equations
Δ𝑑=𝑚(𝜆0/2), I0=2I0 - 2I0 cos (2kdL or 2wt), dL=L1-L2
In a Michelson Interferometer when Mirror 1 is moved a distance Δ𝑑=𝜆0/2Δ, this path difference changes by 𝜆0, and each fringe moves to the position previously occupied by an adjacent fringe. Δ𝑑=𝑚(𝜆0/2)

I also know from the equation for I0=2I0 - 2I0 cos (2kdL or 2wt) that the fringes shift by a phase 2kdL or 2wt(omega tau). I'm unsure what to do , though, given that I am only provided the beam's wavelength and mirror 1's displacement. I'd appreciate any help!
 
So is there some elegant way to do this or am I just supposed to follow my nose and sub the Taylor expansions for terms in the two boost matrices under the assumption ##v,w\ll 1##, then do three ugly matrix multiplications and get some horrifying kludge for ##R## and show that the product of ##R## and its transpose is the identity matrix with det(R)=1? Without loss of generality I made ##\mathbf{v}## point along the x-axis and since ##\mathbf{v}\cdot\mathbf{w} = 0## I set ##w_1 = 0## to...

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