Width of Principal Maxima
The direction of the nth principal maximum is given by
(a + b) sin θn = nλ (i)
Let θn + dθ and θn – dθ give the directions of the first secondary minima on the two sides of the nth primary maxima.
Then,
(a + b) sin [θn ± dθ] = nλ ± λ/N (ii)
where N is the total number of lines on the grating surface.
Dividing (ii) by (i)
Expanding this equation
For small values of dθ; cos dθ = 1 and sin dθ = dθ.
∴ 1 ± cot θn.dθ = 1 ± (1/Nn) (iv)
cot θn.dθ = (1/Nn)
In equation (iv), dθ refers to half the angular width of the principal maximum. The half width dθ is (i) inversely proportional to N the total number of lines and (ii) inversely proportional to n cot θn. The value of n cot θn is more for higher orders because the increase in the value of cot θn is less than the increase in the order. Thus, the half width of the principal maximum is less for higher orders. Also, the larger the number of lines on the grating surface, the smaller is the value of dθ. Further, the value of θn is higher for longer wavelengths and hence the spectral lines are more sharp towards the violet than the red end of the spectrum.
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