Solveeit Logo

Question

Question: The energies of three consecutive energy levels \({L_3}\), \({L_2}\) and \({L_1}\) of hydrogen atom ...

The energies of three consecutive energy levels L3{L_3}, L2{L_2} and L1{L_1} of hydrogen atom E0{E_0}, 4E09\dfrac{{4{E_0}}}{9} and E14\dfrac{{{E_1}}}{4} respectively. A photon of wavelength λ\lambda is emitted for a transition L3{L_3} to L1{L_1}. What will be the wavelength of emission for transition L2{L_2} to L1{L_1}?

Explanation

Solution

In the solution, we will use the Planck’s equation for the energy of the radiation emitted. Using the Planck’s equation, we will derive the expression for the difference in energies of two consecutive levels to obtain the wavelength.

Complete step by step answer:
Given:
The energy of level L3{L_3}, EL3=E0{E_{{L_3}}} = {E_0}
The energy of level L2{L_2}, EL2=4E09{E_{{L_2}}} = \dfrac{{4{E_0}}}{9}
The energy of level L1{L_1}, EL1=E04{E_{{L_1}}} = \dfrac{{{E_0}}}{4}
Now, the relation for the change in the energy of the radiation emitted during transition from one energy level to the other can be written as,
ΔE=hυ EnEn1=hυ\Delta E = h\upsilon \\\ \Rightarrow {E_n} - {E_{n - 1}} = h\upsilon
Here ΔE\Delta E is the change in energy, hh is the Planck’s constant, υ\upsilon is the frequency of the photon of radiation emitted, En{E_n} is the upper energy level and En1{E_{n - 1}} is the lower energy level.

Since c=υλc = \upsilon \lambda , we can write
υ=cλ\upsilon = \dfrac{c}{\lambda }.
Here cc is the velocity of light and λ\lambda is the wavelength of the photon emitted.
We now use the relation υ=cλ\upsilon = \dfrac{c}{\lambda } in EnEn1=hυ{E_n} - {E_{n - 1}} = h\upsilon to get,
EnEn1=hcλ{E_n} - {E_{n - 1}} = h\dfrac{c}{\lambda }
Hence, the relation for the change in energy during a transition from energy level L3{L_3} to L1{L_1} is,
EL3EL1=hcλ{E_{{L_3}}} - {E_{{L_1}}} = h\dfrac{c}{\lambda }
Here λ\lambda is the wavelength of the photon emitted during a transition from energy level L3{L_3} to L1{L_1}.

Since EL3=E0{E_{{L_3}}} = {E_0} and EL1=E04{E_{{L_1}}} = \dfrac{{{E_0}}}{4} we can substitute the values of E0{E_0} andEL1{E_{{L_1}}} in the above equation. Hence,
E0E04=hcλ 4E0E04=hcλ 3E04=hcλ E0=4hc3λ{E_0} - \dfrac{{{E_0}}}{4} = h\dfrac{c}{\lambda }\\\ \Rightarrow \dfrac{{4{E_0} - {E_0}}}{4} = h\dfrac{c}{\lambda }\\\ \Rightarrow \dfrac{{3{E_0}}}{4} = h\dfrac{c}{\lambda }\\\ \Rightarrow {E_0} = \dfrac{{4hc}}{{3\lambda }}

Now, let’s express the relation for the change in energy during a transition from energy level L2{L_2} to L1{L_1}.The relation is written as,
EL2EL1=hcλ2{E_{{L_2}}} - {E_{{L_1}}} = h\dfrac{c}{{{\lambda _2}}}
Here λ2{\lambda _2} is the wavelength of the photon emitted during a transition from the energy level L2{L_2} to L1{L_1}.
Since EL2=4E09{E_{{L_2}}} = \dfrac{{4{E_0}}}{9} and EL1=E04{E_{{L_1}}} = \dfrac{{{E_0}}}{4}, we can substitute 4E09\dfrac{{4{E_0}}}{9} for and E04\dfrac{{{E_0}}}{4} for EL1{E_{{L_1}}} in the above equation. So, the equation becomes
4E09E04=hcλ2 4E0×49E09×4=hcλ2 16E09E036=hcλ2 7E036=hcλ2\dfrac{{4{E_0}}}{9} - \dfrac{{{E_0}}}{4} = h\dfrac{c}{{{\lambda _2}}}\\\ \Rightarrow \dfrac{{4{E_0} \times 4 - 9{E_0}}}{{9 \times 4}} = h\dfrac{c}{{{\lambda _2}}}\\\ \Rightarrow \dfrac{{16{E_0} - 9{E_0}}}{{36}} = h\dfrac{c}{{{\lambda _2}}}\\\ \Rightarrow \dfrac{{7{E_0}}}{{36}} = h\dfrac{c}{{{\lambda _2}}}

Rewriting the equation, we get
λ2=36hc7E0{\lambda _2} = \dfrac{{36hc}}{{7{E_0}}}
Since E0=4hc3λ{E_0} = \dfrac{{4hc}}{{3\lambda }}, we can substitute 4hc3λ\dfrac{{4hc}}{{3\lambda }} for E0{E_0} in λ2=36hc7E0{\lambda _2} = \dfrac{{36hc}}{{7{E_0}}}.
λ2=36hc7×4hc3λ λ2=9×3λ7 λ2=27λ7{\lambda _2} = \dfrac{{36hc}}{{7 \times \dfrac{{4hc}}{{3\lambda }}}}\\\ \Rightarrow {\lambda _2} = \dfrac{{9 \times 3\lambda }}{7}\\\ \therefore {\lambda _2} = \dfrac{{27\lambda }}{7}

Hence, we obtained the wavelength of the photon emitted during a transition from L2{L_2} to L1{L_1} as 27λ7\dfrac{{27\lambda }}{7}.

Note: Planck’ equation generally helps in calculating the energy changes involving light radiations. Hence, we can obtain the frequency and the wavelength of the radiation emitted if the energy of the radiation is known.