To solve the problem, we need to evaluate the resultant intensities at points A and B where two light beams interfere. The given intensities are 4I and 9I; these represent the intensities of the individual light beams.
Step 1: Calculate Resultant Intensity at Point A
At point A, the phase difference ϕ = 0, meaning the waves are in phase. The formula for resultant intensity Ires when two coherent beams interfere is: Ires = I1 + I2 + 2√(I1 I2) cos ϕ.
Substituting I1 = 4I, I2 = 9I, and cos(ϕ) = cos(0) = 1:
Ires,A = 4I + 9I + 2√(4I * 9I)
= 13I + 12I = 25I.
Step 2: Calculate Resultant Intensity at Point B
At point B, the phase difference ϕ = π, meaning the waves are out of phase. Use the same formula but with cos(ϕ) = cos(π) = -1:
Ires,B = 4I + 9I + 2√(4I * 9I) * (-1)
= 13I - 12I = 1I.
Step 3: Determine the Difference of Resultant Intensities
The difference between the intensities at points A and B is:
ΔI = Ires,A - Ires,B = 25I - 1I = 24I.
The computed intensity difference ΔI = 24I fits within the expected range of 24,24. Hence, the difference of resultant intensities, at points A and B, is 24I.
\(I_A = (\sqrt{I_1} + \sqrt{I_2})^2 = 25I\)
\(I_B = (\sqrt{I_1} - \sqrt{I_2})^2 = I\)
So,\(I_A - I_B = 25I - I\)
\(= 24I\)
So, the answer is 24.
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,


What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)
When light shines on a metal, electrons can be ejected from the surface of the metal in a phenomenon known as the photoelectric effect. This process is also often referred to as photoemission, and the electrons that are ejected from the metal are called photoelectrons.
According to Einstein’s explanation of the photoelectric effect :
The energy of photon = energy needed to remove an electron + kinetic energy of the emitted electron
i.e. hν = W + E
Where,