Govt. Exams
Entrance Exams
sin(θc) = n_cladding/n_core = 1.48/1.5 ≈ 0.9867. Therefore θc = arcsin(0.9867) ≈ 83.4°.
At u = 30 cm: m = -f/(u-f) = -15/15 = -1. At u = 20 cm: m = -15/5 = -3. Magnification increases in magnitude from 1 to 3.
At minimum deviation: A = r₁ + r₂ = 2r (by symmetry). Also, sin(A/2) = n·sin(r/2). sin(30°) = √3·sin(30°), which checks out. δ_m = 2i - A where i = A/2 + δ_m/2. Solving: δ_m = 30°.
Using Snell's law: sin(60°) = √3 × sin(r). √3/2 = √3 × sin(r). sin(r) = 1/2, therefore r = 30°.
For Newton's rings: D_m ∝ √m. Therefore D₅/D₁₀ = √5/√10 = √(1/2). D₅ = 0.5 × √(5/10) = 0.5 × √0.5 ≈ 0.354 cm.
For concave lens, images are always virtual, erect, and diminished regardless of object position. Using 1/v = 1/f - 1/u = -1/20 - 1/10 = -3/20, v = -20/3 ≈ -6.67 cm (virtual).
At critical angle: sin(θc) = 1/n = 1/√2. Therefore θc = 45°. This occurs when light travels from denser to less dense (rarer) medium.
For bright fringes: y = (m·λ·D)/d. For 5th bright fringe: 2.5 × 10⁻³ = (5 × λ × 1)/(1 × 10⁻³). Therefore λ = 500 nm.
Magnification m = -v/u = -2, so v = 2u. Using lens equation: 1/f = 1/u + 1/v = 1/u + 1/(2u) = 3/(2u). Therefore u = 3f/2.
Maximum intensity occurs for constructive interference when phase difference = 0 or 2π. I_max = (√I₁ + √I₂)²