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A photon of 300 nm is absorbed by a gas ...

A photon of `300` nm is absorbed by a gas and then emits two photons. One photon has a wavelength `496` nm then the wavelength of second photon in nm is :

A

959

B

859

C

759

D

659

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The correct Answer is:
To solve the problem, we need to use the conservation of energy principle for the absorption and emission of photons. Here’s a step-by-step solution: ### Step 1: Calculate the energy of the absorbed photon The energy of a photon can be calculated using the formula: \[ E = \frac{hc}{\lambda} \] where: - \( E \) is the energy of the photon, - \( h \) is Planck's constant (\( 6.626 \times 10^{-34} \, \text{J s} \)), - \( c \) is the speed of light (\( 3.00 \times 10^8 \, \text{m/s} \)), - \( \lambda \) is the wavelength of the photon in meters. For the absorbed photon with a wavelength of \( 300 \, \text{nm} \) (which is \( 300 \times 10^{-9} \, \text{m} \)): \[ E_{absorbed} = \frac{(6.626 \times 10^{-34} \, \text{J s})(3.00 \times 10^8 \, \text{m/s})}{300 \times 10^{-9} \, \text{m}} \] ### Step 2: Calculate the energy of the emitted photon The energy of the emitted photon with a wavelength of \( 496 \, \text{nm} \) (which is \( 496 \times 10^{-9} \, \text{m} \)) can be calculated similarly: \[ E_{emitted1} = \frac{hc}{\lambda_1} = \frac{(6.626 \times 10^{-34} \, \text{J s})(3.00 \times 10^8 \, \text{m/s})}{496 \times 10^{-9} \, \text{m}} \] ### Step 3: Use conservation of energy According to the conservation of energy, the energy of the absorbed photon is equal to the sum of the energies of the emitted photons: \[ E_{absorbed} = E_{emitted1} + E_{emitted2} \] Thus, we can express it as: \[ E_{absorbed} = E_{emitted1} + E_{emitted2} \] ### Step 4: Solve for the second emitted photon Rearranging the equation gives: \[ E_{emitted2} = E_{absorbed} - E_{emitted1} \] ### Step 5: Calculate the wavelength of the second emitted photon Using the energy of the second emitted photon, we can find its wavelength using: \[ E_{emitted2} = \frac{hc}{\lambda_2} \] Rearranging gives: \[ \lambda_2 = \frac{hc}{E_{emitted2}} \] ### Step 6: Substitute and calculate Now we can substitute the values to find \( \lambda_2 \). ### Final Calculation 1. Calculate \( E_{absorbed} \) using \( \lambda = 300 \, \text{nm} \). 2. Calculate \( E_{emitted1} \) using \( \lambda_1 = 496 \, \text{nm} \). 3. Find \( E_{emitted2} \) using the conservation of energy. 4. Finally, calculate \( \lambda_2 \).

To solve the problem, we need to use the conservation of energy principle for the absorption and emission of photons. Here’s a step-by-step solution: ### Step 1: Calculate the energy of the absorbed photon The energy of a photon can be calculated using the formula: \[ E = \frac{hc}{\lambda} \] where: - \( E \) is the energy of the photon, - \( h \) is Planck's constant (\( 6.626 \times 10^{-34} \, \text{J s} \)), ...
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