A hydrogen atom is in its fifth excited state, with principal quantum number \(n=6 .\) The atom emits a photon with a wavelength of \(410 \mathrm{nm}\). Determine the maximum possible orbital angular momentum of the electron after emission.

Short Answer

Expert verified
Answer: The maximum possible orbital angular momentum of the electron after the photon emission is approximately \(1.49 \times 10^{-34} \mathrm{Js}\).

Step by step solution

01

Calculate the energy of the emitted photon.

The energy of a photon can be calculated using its wavelength and the Planck's constant, with the formula \(E = \frac{hc}{\lambda}\), where \(E\) is the energy, \(h\) is the Planck's constant (\(6.626 \times 10^{-34} \mathrm{Js}\)), \(c\) is the speed of light (\(2.998 \times 10^{8} \mathrm{m/s}\)), and \(\lambda\) is the wavelength of the photon (\(410 \mathrm{nm}\)). Converting the wavelength to meters, we get \(\lambda = 410 \times 10^{-9} \mathrm{m}\). Now, we can calculate the energy of the photon: \(E = \frac{(6.626 \times 10^{-34} \mathrm{Js})(2.998 \times 10^{8} \mathrm{m/s})}{410 \times 10^{-9} \mathrm{m}} \approx 4.839 \times 10^{-19} \mathrm{J}\).
02

Calculate the initial energy level of the hydrogen atom.

The energy of a hydrogen atom with a principal quantum number \(n\) is given by the formula \(E_n = -\frac{13.6 \mathrm{eV}}{n^2}\). Since the atom is initially in its fifth excited state (with \(n = 6\)), its initial energy can be calculated as: \(E_6 = -\frac{13.6 \mathrm{eV}}{6^2} \approx -0.377 \mathrm{eV}\). Converting the energy to joules, we get \(E_6 \approx -6.044 \times 10^{-20} \mathrm{J}\).
03

Calculate the final energy level of the hydrogen atom.

Since the energy of a photon is equal to the difference in energy levels between the initial and final states, we can calculate the final energy level (\(E_f\)) after photon emission as follows: \(E_f = E_6 - E_{photon} \approx -6.044 \times 10^{-20} \mathrm{J} - 4.839 \times 10^{-19} \mathrm{J} \approx -5.443 \times 10^{-19} \mathrm{J}\). Converting the energy back to electron volts, we get \(E_f \approx -3.39 \mathrm{eV}\).
04

Determine the maximum value of the azimuthal quantum number (l).

To find the final principal quantum number \(n_f\), we can compare the obtained energy to the energy levels of the hydrogen atom: \(E_{n_f} = -\frac{13.6 \mathrm{eV}}{n_f^2}\). Setting \(E_{n_f} = -3.39 \mathrm{eV}\), we can solve for \(n_f\): \(n_f \approx \sqrt{\frac{13.6 \mathrm{eV}}{3.39 \mathrm{eV}}} \approx 2\). The maximum possible value of the azimuthal quantum number (\(l\)) is \(n_f - 1\) for a given energy level. Therefore, the maximum value of \(l\) for the final state is: \(l_{max} = n_f - 1 = 2 - 1 = 1\).
05

Calculate the maximum possible orbital angular momentum.

The orbital angular momentum (\(L\)) can be calculated using the formula \(L = \sqrt{l(l+1)}\hbar\), where \(\hbar\) is the reduced Planck's constant (\(1.054 \times 10^{-34} \mathrm{Js}\)). Using the maximum value of \(l\), we can calculate the maximum possible orbital angular momentum: \(L = \sqrt{1(1+1)}(1.054 \times 10^{-34} \mathrm{Js}) \approx 1.49 \times 10^{-34} \mathrm{Js}\). The maximum possible orbital angular momentum of the electron after the photon emission is approximately \(1.49 \times 10^{-34} \mathrm{Js}\).

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