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Question: The ratio of difference of \(1st\) and \(2nd\) lines of Lyman series in H-like atom to difference in...

The ratio of difference of 1st1st and 2nd2nd lines of Lyman series in H-like atom to difference in wavelength for 2nd2nd and 3rd3rd lines of same series is:
A. 2.5:12.5:1
B. 3.5:13.5:1
C. 4.5:14.5:1
D. 5.5:15.5:1

Explanation

Solution

In order to solve this question we need to understand the spectrum of hydrogen. So atoms configuration as suggested by Bohr is that the electrons revolve around the nucleus in shells such that their angular momentum is integral multiple of h2π\dfrac{h}{{2\pi }} in that shell. So when electrons at higher state or shell transits to lower state then it emits light of a certain wavelength. Collection of all those wavelengths are known as spectrum. Based on order of transitions, they are named as Lyman series transitions, Balmer, Paschen, Brackett, and Pfund series transitions.

Complete step by step answer:
Let the electron transit from n2{n_2} level to n1{n_1} level. Let the light wavelength it emits while doing so be, λ\lambda . Let RR be Rydberg constant.So from definition of transition we get,
1λ=R(1n121n22)(i)\dfrac{1}{\lambda } = R(\dfrac{1}{{{n_1}^2}} - \dfrac{1}{{{n_2}^2}}) \to (i)

For Lyman series transition, n1=1{n_1} = 1 as electrons in this case transit from higher state to first energy state.So equation (i) become,
1λ=R(11n22)\dfrac{1}{\lambda } = R(1 - \dfrac{1}{{{n_2}^2}})
So for 1st1st order transition we have, n2=2{n_2} = 2
Putting values we get,
1λ1=R(1122)\dfrac{1}{{{\lambda _1}}} = R(1 - \dfrac{1}{{{2^2}}})
1λ1=R34\Rightarrow \dfrac{1}{{{\lambda _1}}} = R\dfrac{3}{4}
λ1=43R\Rightarrow {\lambda _1} = \dfrac{4}{{3R}}
So for 2nd2nd order transition we have, n2=3{n_2} = 3
Putting values we get,
1λ2=R(1132)\dfrac{1}{{{\lambda _2}}} = R(1 - \dfrac{1}{{{3^2}}})
1λ2=R89\Rightarrow \dfrac{1}{{{\lambda _2}}} = R\dfrac{8}{9}
λ2=98R\Rightarrow {\lambda _2} = \dfrac{9}{{8R}}

Similarly, for 3rd3rd order transition we have, n2=4{n_2} = 4
Putting values we get,
1λ3=R(1142)\dfrac{1}{{{\lambda _3}}} = R(1 - \dfrac{1}{{{4^2}}})
1λ3=R1516\Rightarrow \dfrac{1}{{{\lambda _3}}} = R\dfrac{{15}}{{16}}
λ3=1615R\Rightarrow {\lambda _3} = \dfrac{{16}}{{15R}}
So the difference of 1st&2nd1st{\kern 1pt} \& {\kern 1pt} {\kern 1pt} 2nd lines of Lyman series is, λ=λ1λ2\lambda = {\lambda _1} - {\lambda _2}
Putting values we get,
λ=43R98R\lambda = \dfrac{4}{{3R}} - \dfrac{9}{{8R}}
λ=322724R\Rightarrow \lambda = \dfrac{{32 - 27}}{{24R}}
λ=524R\Rightarrow \lambda = \dfrac{5}{{24R}}

So the difference of 2nd&3rd2nd{\kern 1pt} \& {\kern 1pt} {\kern 1pt} 3rd lines of Lyman series is, λ=λ2λ3\lambda ' = {\lambda _2} - {\lambda _3}
Putting values we get,
λ=98R1615R\lambda ' = \dfrac{9}{{8R}} - \dfrac{{16}}{{15R}}
λ=135128120R\Rightarrow \lambda ' = \dfrac{{135 - 128}}{{120R}}
λ=7120R\Rightarrow \lambda ' = \dfrac{7}{{120R}}
So the required ratio is,
λλ=(524R)(7120R)\dfrac{\lambda }{{\lambda '}} = \dfrac{{(\dfrac{5}{{24R}})}}{{(\dfrac{7}{{120R}})}}
λλ=257\Rightarrow \dfrac{\lambda }{{\lambda '}} = \dfrac{{25}}{7}
λ:λ=3.5:1\therefore \lambda :\lambda ' = 3.5:1

The correct option is B.

Note: It should be remembered that, when the electron is at higher level it de-excites in microseconds because of time-energy Heisenberg uncertainty principle, according to which if energy is fixed or perfectly defined then uncertainty in time is maximum, this clearly depicts why electrons at higher excited level de-excites in microseconds.