Question:medium

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.

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Use the formula for the energy levels of a hydrogen atom and the energy of the emitted photon during a transition between energy levels. Identify the initial and final energy levels based on the given information. Set up the equation relating the photon energy to the initial and final quantum numbers and solve for the unknown final quantum number \( n \).
Updated On: Jan 14, 2026
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Correct Answer: 2

Solution and Explanation

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.

Concept Used:

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-by-Step Solution:

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.

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