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| <math>A^2 _{12} / A^2 = C _1 + C _2 + 2 C _1 C _2 \cos ( \frac{4 \pi \tau}{\lambda} ) </math> | | <math>A^2 _{12} / A^2 = C _1 + C _2 + 2 C _1 C _2 \cos ( \frac{4 \pi \tau}{\lambda} ) </math> |
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− | == Calculating the Shape == | + | == Ideal Shape Calculation == |
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| Of course, thickness is not the only thing we need. After calculating <math> \tau </math> and uncovering the mirror, we will also detect the third laser reflection. We can calculate that the amplitude of this new combined wave will be | | Of course, thickness is not the only thing we need. After calculating <math> \tau </math> and uncovering the mirror, we will also detect the third laser reflection. We can calculate that the amplitude of this new combined wave will be |
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| Although this equation looks very complicated, we know that | | Although this equation looks very complicated, we know that |
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− | <math>( d _2 - d _1 ) = \frac{4 \pi \tau}{\gamma}</math> | + | <math>( d _2 - d _1 ) = \frac{4 \pi \tau}{\lambda}</math> |
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| so | | so |
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− | <math>d _2 = \frac{4 \pi \tau}{\gamma} + d _1</math> | + | <math>d _2 = \frac{4 \pi \tau}{\lambda} + d _1</math> |
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− | To further simplify, we need a "shape term". This term will represent the difference in the distance traveled by waves 1 and 3. If the phase-shift between 1 and 3 is constant, the diamond is flat; otherwise, it is deformed by some distance expressed by s. | + | To further simplify, we need a "shape term". This term will represent the difference in the distance traveled by waves 0 and 1. If the phase-shift between 0 and 1 is constant, the diamond is flat; otherwise, it is deformed by some distance expressed by s. |
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− | <math>s = d _1 \frac{v _a}{2}</math> | + | <math>s = \frac{d _1 \lambda}{4 \pi}</math> |
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− | where <math> v _a </math> is the speed of light in air. We can rewrite this in terms of <math> d _1 </math>:
| + | We can rewrite this in terms of <math> d _1 </math>: |
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− | <math>d _1 = 2 s / v _a</math> | + | <math>d _1 = \frac{4 \pi s}{\lambda}</math> |
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| Simplifying our initial equation, we find that | | Simplifying our initial equation, we find that |
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− | <math>\frac{A^2 _{123}}{A^2} = C^2 _1 + C^2 _2 + C^2 _3 + 2 C _1 C _2 \cos ( 2 \tau / V _d ) + 2 C _1 \cos ( - 2 s / v _a ) + 2 C _2 \cos ( - 2 \tau / v _d - 2 s / v _a ) </math> | + | <math>\frac{A^2 _{012}}{A^2} = C^2 _0 + C^2 _1 + C^2 _2 + 2 C _1 C _2 \cos ( \frac{4 \pi \tau}{\lambda} ) + 2 C _0 C _1 \cos ( - \frac{4 \pi s}{\lambda} ) + 2 C _0 C _2 \cos ( - \frac{4 \pi (\tau + s)}{\lambda} ) </math> |
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| Because the cosine is an even function, we can slightly simplify this further. | | Because the cosine is an even function, we can slightly simplify this further. |
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− | <math>\frac{A^2 _{123}}{A^2} = C^2 _1 + C^2 _2 + C^2 _3 + 2 C _1 C _2 \cos ( 2 \tau / V _d ) + 2 C _1 \cos ( 2 s / v _a ) + 2 C _2 \cos ( 2 \tau / v _d + 2 s / v _a )</math> | + | <math>\frac{A^2 _{012}}{A^2} = C^2 _0 + C^2 _1 + C^2 _2 + 2 C _1 C _2 \cos ( \frac{4 \pi \tau}{\lambda} ) + 2 C _0 C _1 \cos ( \frac{4 \pi s}{\lambda} ) + 2 C _0 C _2 \cos ( \frac{4 \pi (\tau + s)}{\lambda} ) </math> |
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| This equation, athough complicated, is completely solvable, as the only unknown is the s-term. | | This equation, athough complicated, is completely solvable, as the only unknown is the s-term. |