An electron in the hydrogen atom initially in the fourth excited state makes a transition to \( n^{th} \) energy state by emitting a photon of energy 2.86 eV. The integer value of n will be 1cm.
This task involves determining the final principal quantum number (\(n\)) of an electron in a hydrogen atom following a transition from a higher energy level, accompanied by the emission of a photon with a specified energy.
The energy of an electron within the \(k^{th}\) energy level (or orbit) of a hydrogen atom is defined by the following equation:
\[ E_k = -\frac{13.6}{k^2} \text{ eV} \]The "ground state" is designated by \(k=1\). The "first excited state" is at \(k=2\), the "second excited state" at \(k=3\), and so forth. Consequently, the \(m^{th}\) excited state corresponds to the principal quantum number \(k = m+1\).
Upon transitioning from a higher initial energy state \(E_i\) (characterized by quantum number \(k_i\)) to a lower final energy state \(E_f\) (characterized by quantum number \(k_f\)), an electron emits a photon. The energy of this emitted photon (\(\Delta E\)) is equivalent to the difference between these energy levels.
\[ \Delta E = E_i - E_f \]Step 1: Identify the initial principal quantum number (\(k_i\)) of the electron.
The problem specifies that the electron begins in the "fourth excited state". Applying the established relationship where the \(m^{th}\) excited state corresponds to \(k = m+1\), for the fourth excited state (\(m=4\)), the principal quantum number is calculated as:
\[ k_i = 4 + 1 = 5 \]Step 2: Compute the energy of the electron in its initial state (\(E_i\)).
Using the energy formula with the initial quantum number \(k_i = 5\):
\[ E_i = E_5 = -\frac{13.6}{5^2} \text{ eV} = -\frac{13.6}{25} \text{ eV} \] \[ E_i = -0.544 \text{ eV} \]Step 3: Utilize the energy of the emitted photon to determine the energy of the final state (\(E_n\)).
The energy of the emitted photon is provided as \(\Delta E = 2.86\) eV. The electron transitions to the \(n^{th}\) energy state, with energy \(E_n\). The governing equation is:
\[ \Delta E = E_i - E_n \]To solve for \(E_n\), the equation is rearranged as follows:
\[ E_n = E_i - \Delta E \]Substituting the known values yields:
\[ E_n = -0.544 \text{ eV} - 2.86 \text{ eV} \] \[ E_n = -3.404 \text{ eV} \]Step 4: Ascertain the principal quantum number (\(n\)) for the final energy state.
The energy formula is applied once more, this time using the final energy \(E_n\):
\[ E_n = -\frac{13.6}{n^2} \text{ eV} \]Inserting the calculated value of \(E_n\):
\[ -3.404 = -\frac{13.6}{n^2} \]Solving for \(n^2\):
\[ n^2 = \frac{13.6}{3.404} \] \[ n^2 \approx 3.995 \]Given that the principal quantum number \(n\) must be an integer, \(n^2\) is rounded to the nearest integer.
\[ n^2 = 4 \] \[ n = \sqrt{4} = 2 \]Therefore, the integer value of n corresponding to the final energy state is 2.
