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Question: When a Hydrogen atom emits a photon of energy \( 12.09eV \) , what will be the change in its orbit’s...

When a Hydrogen atom emits a photon of energy 12.09eV12.09eV , what will be the change in its orbit’s angular momentum?
A. 3hπ\dfrac{{3h}}{\pi }
B. 2hπ\dfrac{{2h}}{\pi }
C. hπ\dfrac{h}{\pi }
D. 4hπ\dfrac{{4h}}{\pi }

Explanation

Solution

Hint : Find the separation between the orbits, Δn\Delta n using the energy equation of electron in Hydrogen atoms for nth{n^{th}} orbit, En=13.6n2eV{E_n} = \dfrac{{ - 13.6}}{{{n^2}}}eV .Using the formula for the energy of an electron in nth{n^{th}} orbit, En=13.6n2eV{E_n} = \dfrac{{ - 13.6}}{{{n^2}}}eV .
1eV=1.60218×1019J1eV = {\text{1}}{\text{.60218}} \times {10^{ - 19}}J ,Where, nn is positive integer 1,2,3....1,2,3.... .Angular momentum of an electron at nth{n^{th}} orbit,
Ln=n  =nh2π{L_n} = n\;\hbar = \dfrac{{nh}}{{2\pi }}
where, h  = 6.63 × 1034  Jsh\; = {\text{ }}6.63{\text{ }} \times {\text{ }}{10^ - }^{34}\;J \cdot s is Planck’s constant.

Complete Step By Step Answer:
We know, the energy of an electron at nth{n^{th}} orbit in terms of nn ,
En=13.6n2eV{E_n} = \dfrac{{ - 13.6}}{{{n^2}}}eV .
Where, nn is a positive integer 1,2,3....1,2,3.... and nn is called principal quantum number
and 1eV=1.60218×1019J1eV = {\text{1}}{\text{.60218}} \times {10^{ - 19}}J
Now we know, the energy separation between two orbits is equal to the energy of the photon, ΔE=hν=Ep\Delta E = h\nu = {E_p}
where, Ep{E_p} is the energy of the photon, ν\nu is the frequency of the photon and h  = 6.63 × 1034  Jsh\; = {\text{ }}6.63{\text{ }} \times {\text{ }}{10^ - }^{34}\;J \cdot s , Planck’s constant.
Now, here a photon has been released that means the electron has jumped from a higher orbit to lower orbit.
Let’s say, the electron jumps from n2{n_2} orbit to n1{n_1} orbit .Therefore energy separation between these two orbit is, ΔE=En2En1=(13.6n2213.6n12)eV\Delta E = {E_{{n_2}}} - {E_{{n_1}}} = \left( {\dfrac{{ - 13.6}}{{{n_2}^2}} - \dfrac{{ - 13.6}}{{{n_1}^2}}} \right)eV which is equal to the photon energy of Ep=12.09eV{E_p} = 12.09eV .
So, you can see that with one equation we obviously cannot find the value of n2{n_2} and n1{n_1} both, but you can find the energy separation just by observing the energy of each orbit.
Here, the photon energy is 12.09eV12.09eV so separation ΔE=(13.6n22+13.6n12)eV\Delta E = \left( {\dfrac{{ - 13.6}}{{{n_2}^2}} + \dfrac{{13.6}}{{{n_1}^2}}} \right)eV must be greater than 12eV12eV .
Now, the energy of the electron in the H-atom at first orbit is 13.6eV- 13.6eV . Therefore, ΔE=(13.6n22+13.6)eV\Delta E = \left( {\dfrac{{ - 13.6}}{{{n_2}^2}} + 13.6} \right)eV for n1=1{n_1} = 1 , Which only can be greater than 12eV12eV for a value of n2{n_2} and must be n2>1{n_2} > 1 . So, the electron must have jumped to the first orbit since at first the electron has the highest energy separation in energy.
Now, we just have to find n2{n_2} using the photon energy. So, equating photon energy and the energy separation of the orbits we get,
ΔE=(13.6n22+13.6)eV=12.09eV\Delta E = \left( {\dfrac{{ - 13.6}}{{{n_2}^2}} + 13.6} \right)eV = 12.09eV
Deducing the relation we get,
(13.6n22)=12.0913.6=1.51\Rightarrow \left( {\dfrac{{ - 13.6}}{{{n_2}^2}}} \right) = 12.09 - 13.6 = - 1.51
n22=13.61.519.00\Rightarrow {n_2}^2 = \dfrac{{ - 13.6}}{{ - 1.51}} \approx 9.00
Therefore solving for n2{n_2} we get,
n2=9=3\Rightarrow {n_2} = \sqrt 9 = 3
Therefore, the electron jumps from 3rd{3^{rd}} orbit to 1st{1^{st}} orbit.
Therefore, Δn=31=2\Delta n = 3 - 1 = 2
Now, angular momentum of electron at nth{n^{th}} is,
Ln=n  =nh2π{L_n} = n\;\hbar = \dfrac{{nh}}{{2\pi }}
Hence, change in angular momentum,
ΔL=Ln2Ln1=(n2  n1)=(n2  n1)h2π\Delta L = {L_{{n_2}}} - {L_{{n_1}}} = ({n_2}\; - {n_1})\hbar = \dfrac{{({n_2}\; - {n_1})h}}{{2\pi }}
ΔL=Δnh2π\therefore \Delta L = \dfrac{{\Delta nh}}{{2\pi }}
Here, Δn=2\Delta n = 2
Therefore, change in angular momentum will be,
ΔL=2h2π=hπ\Delta L = \dfrac{{2h}}{{2\pi }} = \dfrac{h}{\pi }
Hence, the answer is hπ\dfrac{h}{\pi }
Hence , option ( C) is correct.

Note :
To find the difference between the states, you have to observe the photon energy and choose the correct range for the energy gap between the orbits/states. If, observing the photon energy is not possible you can solve for the wavelength of the photon using the relation, Ep=hν=hcλ{E_p} = h\nu = \dfrac{{hc}}{\lambda }
and choose the correct H-spectrum. Here, we will get Lyman series of hydrogen spectrum since the electron jumps from first orbit to nth{n^{th}} orbit, for Lyman series the minimum wavelength is 1216A1216{\mathop A\limits^\circ}
Also, please keep in mind that, for the same value of photon energy you can get multiple jumps between different orbits.