Optics - Double Slit Irradiance of Fringes

peppies
Messages
15
Reaction score
1
[Solved] Optics - Double Slit Irradiance of Fringes

Homework Statement


A double slit diffraction pattern is formed using mercury green light at 546.1nm. Each slit has a width of 0.100mm (= b), slit separation is 0.400mm (=a). The pattern reveals that the fourth-order interference maxima are missing from pattern.

What is the irradiance of the first three orders of interference fringes, relative to the zeroth-order maximum?


Homework Equations


I = 4Io (sin(\beta)/\beta))^2 * (cos(\alpha))^2
\beta = 0.5kbsin(\theta)
\alpha = 0.5kasin(\theta)
k = (2(pi)/\lambda)


The Attempt at a Solution


I've been trying to figure this one out for days and the book never gave any practice problems or simple explanation on what to do here.

First I tried to solve for the first order interference fringe (m=1):

sin(\theta) = (m\lambda/a), then use this result to solve for alpha and beta in the two equations above and then finally solve for the sinc and cos^2 functions in the irradiance to find the ratio to the zeroth order fringe.

The answers in the back of the book for the first three orders are (0.8106, 0.4053, 0.09006) but I am not getting these.

The book I'm using is "Introduction to Opitics 3rd edition by Pedrotti"

Thanks
Best
 
Last edited:
Physics news on Phys.org
Nevermind, I solved it by using the RAD mode on my calculator rather than DEG.
 
Hello everyone, I’m considering a point charge q that oscillates harmonically about the origin along the z-axis, e.g. $$z_{q}(t)= A\sin(wt)$$ In a strongly simplified / quasi-instantaneous approximation I ignore retardation and take the electric field at the position ##r=(x,y,z)## simply to be the “Coulomb field at the charge’s instantaneous position”: $$E(r,t)=\frac{q}{4\pi\varepsilon_{0}}\frac{r-r_{q}(t)}{||r-r_{q}(t)||^{3}}$$ with $$r_{q}(t)=(0,0,z_{q}(t))$$ (I’m aware this isn’t...
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
Back
Top