I Correct Formula for "No Fringe Condition" (Michelson Interferometer)

AI Thread Summary
Two textbooks present different formulas for the "No Fringe Formation" condition in a Michelson interferometer, leading to confusion. The first formula, derived from combining bright and dark fringe conditions for two wavelengths, results in d = λ(1)λ(2)/(4∆λ). The second formula, based on nth and (n+1)th order bright fringes, yields d = λ(1)λ(2)/(2∆λ). The first formula is deemed correct for determining mirror separation where no fringes are observed, while the second indicates the distance for maximum fringe visibility. Despite the differences, the first formula is preferred for clarity in similar problem types.
warhammer
Messages
164
Reaction score
33
In two different textbooks, there are two different formulas with different derivation styles for the "No Fringe Formation" Condition.

In approach (a), they use an amalgamation of bright and dark for 2 wavelengths having very minute difference in the following manner:

2dcostheta=n*λ(1) -------- (1)

2dcostheta= (n+1/2)*λ(2) ----------- (2)

Subtracting both the equations we get, n=λ(2)/(2(∆λ))

Now using this value of 'n' for small angles in (1) we get d= λ(1)λ(2)/(4∆λ)

This is one formula.

In the other textbook they have used another approach to calculate the separation 'd' in order to gauge after what distance fringe vanishes. Here they considered a bright of nth order and another bright for (n+1)th order. So proceeding in similar fashion as above (for small angles etc.)

2d=nλ(1)=n'λ(2) where n'=n+1

Thus n=λ(2)/{(λ(1)-λ(2)}

Using above value of n, we eventually get

d= λ(1)λ(2)/(2∆λ).

This is the other formula.

Now I would greatly appreciate if someone would help me understand which is the correct one because I used both of them and they apply for different questions which are of the type- "find separation of mirrors for which there is no fringe observed".

Both have a distinction of 1/2.
 
Science news on Phys.org
The first one is the correct one as far as I can tell. The second one gives the distance for which you will observe the maximum amount of fringes with two closely spaced wavelengths.
This phenomenon will be cyclical, in that you can have ## 2d=n \lambda_a=(n+3/2) \lambda_b ##, and I think that will give ## d=(3/4)(\lambda_a \lambda_b)/\Delta \lambda ##, etc. (Edit: Yes, I did the algebra=it does indeed give this result).
In college we did this with the 5890 and 5896 (angstroms) lines of sodium, and the fringes come and go periodically as one of the mirrors is moved.
 
Last edited:
Charles Link said:
The first one is the correct one as far as I can tell. The second one gives the distance for which you will observe the maximum amount of fringes with two closely spaced wavelengths.
This phenomenon will be cyclical, in that you can have ## 2d=n \lambda_a=(n+3/2) \lambda_b ##, and I think that will give ## d=(3/4)(\lambda_a \lambda_b)/\Delta \lambda ##, etc. (Edit: Yes, I did the algebra=it does indeed give this result).
In college we did this with the 5890 and 5896 (angstroms) lines of sodium, and the fringes come and go periodically as one of the mirrors is moved.
Thank you so much for your response sir. I was also inclined towards the first one but in both the textbooks I am still unable to understand/gauge why the authors have used the distinct formulae in same type of questions 😕 But I guess I will stick with the first one only
 
  • Like
Likes Charles Link
Thread 'A quartet of epi-illumination methods'
Well, it took almost 20 years (!!!), but I finally obtained a set of epi-phase microscope objectives (Zeiss). The principles of epi-phase contrast is nearly identical to transillumination phase contrast, but the phase ring is a 1/8 wave retarder rather than a 1/4 wave retarder (because with epi-illumination, the light passes through the ring twice). This method was popular only for a very short period of time before epi-DIC (differential interference contrast) became widely available. So...
I am currently undertaking a research internship where I am modelling the heating of silicon wafers with a 515 nm femtosecond laser. In order to increase the absorption of the laser into the oxide layer on top of the wafer it was suggested we use gold nanoparticles. I was tasked with modelling the optical properties of a 5nm gold nanoparticle, in particular the absorption cross section, using COMSOL Multiphysics. My model seems to be getting correct values for the absorption coefficient and...
Back
Top