To find the wavelength of light emitted in the visible region by the He+ ions, we proceed with the following steps:
1. Energy Transferred by the Hydrogen Atoms
The energy levels of a hydrogen atom (Z=1) are given by:
En(H)=−n213.6 eV
Initially, the hydrogen atoms are in their first excited state (n=2). The total excitation energy of an excited hydrogen atom is the energy required to excite it from its ground state (n=1) to n=2:
ΔEexc(H)=E2−E1=−2213.6−(−1213.6)=−3.4−(−13.6)=10.2 eV
2. State of the He+ Ions After Collision
The energy levels of a singly ionized helium atom He+ (Z=2) are:
En(He+)=−13.6×n2Z2=−n254.4 eV
Initially, the He+ ions are also in their first excited state (n=2):
E2(He+)=−2254.4=−13.6 eV
When the hydrogen atom transfers its total excitation energy of 10.2 eV to a He+ ion via collision, the new energy of the He+ ion becomes:
Efinal(He+)=E2(He+)+ΔEexc(H)=−13.6 eV+10.2 eV=−3.4 eV
Let the principal quantum number of this final state be n. Then:
−n254.4=−3.4⟹n2=3.454.4=16⟹n=4
Thus, the He+ ions are excited to the state n=4.
3. Transitions and Identification of Visible Light Emission
From the state n=4, the possible radiative transitions for He+ are:
- 4→1: UV region (λ≈24.3 nm)
- 4→2: UV region (λ≈121.5 nm)
- 3→1: UV region (λ≈25.6 nm)
- 3→2: UV region (λ≈164.1 nm)
- 2→1: Extreme UV region (λ≈30.4 nm)
- 4→3: Visible region (wavelength lying between 380 nm and 750 nm)
Thus, the only transition that emits radiation in the visible spectrum is from n=4 to n=3.
4. Calculation of the Emitted Wavelength
Using the Rydberg formula for a hydrogen-like ion with Z=2:
λ1=RZ2(n121−n221)
Substituting Z=2, n1=3, n2=4, and the Rydberg constant R≈1.097×107 m−1:
λ1=R×22×(321−421)=4R(91−161)=4R×1447=367R
Therefore:
λ=7R36=7×1.097×107 m−136≈4.69×10−7 m≈4.8×10−7 m
Hence, the correct option is (C).