Solution
Related Formula
The energy of an electron in the n-th state of a hydrogen atom is:
Eₙ = -(13.6)/(n²) eVCore Logic
At T = 0 K, all hydrogen atoms are in their ground state (n = 1). To observe any lines in the Balmer series emission spectrum:
- The emission lines must result from a transition terminating in the state n = 2.
- This requires the hydrogen electron to first be excited to at least the state n = 3.
Thus, the bombarding electrons must have enough kinetic energy to excite the ground-state electron (n = 1) to the n = 3 state.
Step 1: Calculate the Required Energy and Potential
The required energy difference is:
Δ E = E₃ - E₁ = -(13.6)/(3²) - (-(13.6)/(1²)) eV Δ E = 13.6 (1 - (1)/(9)) eV = 13.6 × (8)/(9) eV ≈ 12.09 eVSince the excitation energy is provided by electrons accelerated through potential V, the minimum potential difference required is:
V ≈ 12.09 V ≈ 12.1 VStep 2: Solve for Alpha
Comparing to the given form (α)/(10) V:
12.1 = (α)/(10) α = 121Pattern Recognition
Balmer series emission requires excitation of the electron to at least n=3. Ground state n=1 to n=3 excitation energy is 12.09 eV ≈ 12.1 eV, matching α = 121 when multiplied by 10.
Chapter Mix
Class 12 Physics: Atoms