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A radiation of energy E falls normally o...

A radiation of energy `E` falls normally on a perfectly reflecting surface . The momentum transferred to the surface is

A

`E/C`

B

`(2E)/(C )`

C

`(2E)/(C^(2))`

D

`E/(C^(2))`

Text Solution

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The correct Answer is:
To solve the problem of calculating the momentum transferred to a perfectly reflecting surface when radiation of energy \( E \) falls normally on it, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding the Energy of Radiation:** The energy \( E \) of the radiation can be expressed in terms of its frequency \( f \) using the equation: \[ E = h \cdot f \] where \( h \) is Planck's constant. 2. **Relating Energy to Momentum:** The momentum \( p \) of a photon (which is a quantum of radiation) can be expressed as: \[ p = \frac{E}{c} \] where \( c \) is the speed of light. This can also be derived from the relationship: \[ p = \frac{h}{\lambda} \] where \( \lambda \) is the wavelength of the radiation. 3. **Calculating Initial Momentum:** When the radiation falls on the surface, it has an initial momentum \( p_i \): \[ p_i = \frac{E}{c} \] 4. **Reflection of Radiation:** Since the surface is perfectly reflecting, the radiation will reflect back with the same magnitude of momentum but in the opposite direction. Thus, the final momentum \( p_f \) after reflection is: \[ p_f = -\frac{E}{c} \] 5. **Calculating Change in Momentum:** The change in momentum \( \Delta p \) (which is the momentum transferred to the surface) can be calculated as: \[ \Delta p = p_f - p_i \] Substituting the values of \( p_f \) and \( p_i \): \[ \Delta p = -\frac{E}{c} - \frac{E}{c} = -\frac{2E}{c} \] 6. **Final Result:** The magnitude of the momentum transferred to the surface is: \[ |\Delta p| = \frac{2E}{c} \] ### Conclusion: The momentum transferred to the perfectly reflecting surface is \( \frac{2E}{c} \).
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