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A 2.0 -MeV X-ray photon is scattered off a free electron at rest and deflected by an angle of \(53^{\circ}\). What is the wavelength of the scattered photon?

Short Answer

Expert verified
Answer: The wavelength of the scattered photon is approximately \(7.92 \times 10^{-12} \text{ m}\).

Step by step solution

01

Convert the given energy into initial photon wavelength

First, we need to convert the given energy (2.0 MeV) into the initial photon wavelength using the formula: \(E = \frac{h c}{\lambda}\) Where \(E\) is the energy, \(h\) is the Planck's constant, \(c\) is the speed of light, and \(\lambda\) is the wavelength. We are given \(E = 2.0 \times 10^6 \text{ eV}\), so we can rewrite the formula as: \(\lambda = \frac{h c}{E}\) Remember to convert the energy from eV to Joules: \(E_\text{J} = E \times e = 2.0 \times 10^6 \text{ eV} \times 1.6 \times 10^{-19} \text{ J/eV} = 3.2 \times 10^{-13} \text{ J}\) Then, plug in the values for \(h\) and \(c\): \(\lambda_i = \frac{6.626 \times 10^{-34} \text{ J s} \times 3.0 \times 10^8 \text{ m/s}}{3.2 \times 10^{-13} \text{ J}} = 6.20 \times 10^{-12} \text{ m}\)
02

Use the Compton scattering formula to find the change in wavelength

The Compton scattering formula relates the initial photon wavelength (\(\lambda_i\)), final photon wavelength (\(\lambda_f\)), electron's rest mass, and the scattering angle (\(\theta\)). It is given by: \(\lambda_f - \lambda_i = \frac{h}{m_e c} (1 - \cos{\theta})\) Where \(\frac{h}{m_e c}\) is the Compton wavelength and is approximately equal to \(2.43 \times 10^{-12} \text{ m}\). The scattering angle is given in degrees, so we need to convert it to radians: \(\theta_\text{rad} = 53^{\circ} \times \frac{\pi}{180} \approx 0.925 \text{ rad}\) Now, plug in the initial wavelength, Compton wavelength, and the scattering angle: \(\Delta\lambda = \lambda_f - \lambda_i = 2.43 \times 10^{-12} \text{ m} \times (1 - \cos{0.925}) = 1.72 \times 10^{-12} \text{ m}\)
03

Find the final photon wavelength

Now that we have the change in wavelength, we can find the final photon wavelength: \(\lambda_f = \lambda_i + \Delta\lambda = 6.20 \times 10^{-12} \text{ m} + 1.72 \times 10^{-12} \text{ m} = 7.92 \times 10^{-12} \text{ m}\) So, the wavelength of the scattered photon is approximately \(7.92 \times 10^{-12} \text{ m}\).

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