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QJEEAdv23Ch64c4: JEE Advanced 2023 Chemistry - Class 11 JEEAdv23Ch64c4 Solution: For , a transition takes place from the orbit of radius to the…

For He+\mathrm{He}^{+} , a transition takes place from the orbit of radius 105.8pm105.8 \mathrm{pm} to the orbit of radius 26.45pm26.45 \mathrm{pm} . The wavelength (in nm) of the emitted photon during the transition is _______.

[Use :

Bohr radius, a=52.9pm\mathrm{a}=52.9 \mathrm{pm}

Rydberg constant, RH=2.2×10−18 JR_{\mathrm{H}}=2.2 \times 10^{-18} \mathrm{~J}

Planck's constant, h=6.6×10−34 J s\mathrm{h}=6.6 \times 10^{-34} \mathrm{~J} \mathrm{~s}

Speed of light, c=3×108 m s−1\mathrm{c}=3 \times 10^8 \mathrm{~m} \mathrm{~s}^{-1} ]

Step-by-Step Verified Solution

1. The radius of the nth orbit in a single-electron system is given by the equation:

r=52.9×n2Zr = \frac{52.9 \times n^2}{Z}

where rr is in pm, nn is the principal quantum number, and ZZ is the atomic number.

2. For a He+\mathrm{He}^{+} ion, Z=2Z=2 .

3. We are given the initial radius r2=105.8r_2 = 105.8 pm and the final radius r1=26.45r_1 = 26.45 pm.

4. We can substitute these radii into the equation for rr to find the corresponding quantum numbers.

For r2=105.8r_2 = 105.8 pm, we get :

105.8=52.9×n222105.8 = \frac{52.9 \times n_2^2}{2}

which gives n2=2n_2 = 2 .

Similarly, for r1=26.45r_1 = 26.45 pm, we get :

26.45=52.9×n12226.45 = \frac{52.9 \times n_1^2}{2}

which gives n1=1n_1 = 1 .

5. Therefore, the transition is from n2=2n_2 = 2 to n1=1n_1 = 1 .

6. The energy difference during this transition is equal to the energy of the emitted photon, which is given by :

E=hcλ=RHZ2(1n12−1n22)E = \frac{hc}{\lambda} = R_H Z^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)

where hh is the Planck's constant, cc is the speed of light, RHR_H is the Rydberg constant, and λ\lambda is the wavelength of the photon.

7. Substituting all known values into this equation gives :

6.6×10−34 J s×3×108 m/sλ=2.2×10−18 J×22(112−122)\frac{6.6 \times 10^{-34} \, \mathrm{J} \, \mathrm{s} \times 3 \times 10^8 \, \mathrm{m/s}}{\lambda} = 2.2 \times 10^{-18} \, \mathrm{J} \times 2^2 \left( \frac{1}{1^2} - \frac{1}{2^2} \right)

Solving this equation yields λ=30×10−9\lambda = 30 \times 10^{-9} m, or 30 nm.

8. So, the wavelength of the emitted photon during the transition is 30 nm.

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