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Light rays of wavelength 6000A^(@) and o...

Light rays of wavelength `6000A^(@)` and of photon intensity `39.6Wm^-2` is incident on a metal surface. If only one percent of photons incident on the surface of electrons emitted per second unit area from the surface will be [Planck constant =`6.64xx10^(-34) J-S`,Velocity of light =`3xx10^(8) ms^(-1)`]

A

`12 xx10^(18)`

B

` 10 xx 10^(18)`

C

` 12 xx 10^(17)`

D

`12 xx 10^(19)`

Text Solution

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The correct Answer is:
To solve the problem, we need to determine the number of electrons emitted per second per unit area from a metal surface when light of a specific wavelength and intensity is incident on it. Here's a step-by-step solution: ### Step 1: Understand the relationship between intensity, number of photons, and energy of photons The intensity \( I \) of the light is defined as the energy falling per unit area per unit time. The energy of a single photon can be calculated using the formula: \[ E = \frac{hc}{\lambda} \] where: - \( h \) is Planck's constant (\( 6.64 \times 10^{-34} \, \text{J s} \)), - \( c \) is the speed of light (\( 3 \times 10^8 \, \text{m/s} \)), - \( \lambda \) is the wavelength of the light. ### Step 2: Calculate the energy of a single photon Given the wavelength \( \lambda = 6000 \, \text{Å} = 6000 \times 10^{-10} \, \text{m} \): \[ E = \frac{(6.64 \times 10^{-34} \, \text{J s})(3 \times 10^8 \, \text{m/s})}{6000 \times 10^{-10} \, \text{m}} \] Calculating this gives: \[ E = \frac{(6.64 \times 3) \times 10^{-26}}{6000} = \frac{19.92 \times 10^{-26}}{6000} = 3.32 \times 10^{-29} \, \text{J} \] ### Step 3: Relate intensity to the number of photons The intensity \( I \) can also be expressed in terms of the number of photons \( N \) incident per unit area per second: \[ I = \frac{N \cdot E}{A} \] where \( A \) is the area (which we can consider as 1 m² for simplicity). Rearranging gives: \[ N = \frac{I \cdot A}{E} \] Substituting \( A = 1 \, \text{m}^2 \): \[ N = \frac{I}{E} \] ### Step 4: Substitute the values Given \( I = 39.6 \, \text{W/m}^2 \): \[ N = \frac{39.6 \, \text{W/m}^2}{3.32 \times 10^{-29} \, \text{J}} \approx 1.19 \times 10^{30} \, \text{photons/m}^2 \text{s} \] ### Step 5: Calculate the number of emitted electrons Since only 1% of the incident photons lead to the emission of electrons: \[ \text{Electrons emitted} = 0.01 \times N = 0.01 \times 1.19 \times 10^{30} \approx 1.19 \times 10^{28} \, \text{electrons/m}^2 \text{s} \] ### Step 6: Final result Thus, the number of electrons emitted per second per unit area from the surface is: \[ \text{Electrons emitted} = 1.19 \times 10^{28} \, \text{electrons/m}^2 \text{s} \]
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