Question
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 1st and 2nd lines of Lyman series in H-like atom to difference in wavelength for 2nd and 3rd lines of same series is:
A. 2.5:1
B. 3.5:1
C. 4.5:1
D. 5.5:1
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 2πh 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 level to n1 level. Let the light wavelength it emits while doing so be, λ. Let R be Rydberg constant.So from definition of transition we get,
λ1=R(n121−n221)→(i)
For Lyman series transition, n1=1 as electrons in this case transit from higher state to first energy state.So equation (i) become,
λ1=R(1−n221)
So for 1st order transition we have, n2=2
Putting values we get,
λ11=R(1−221)
⇒λ11=R43
⇒λ1=3R4
So for 2nd order transition we have, n2=3
Putting values we get,
λ21=R(1−321)
⇒λ21=R98
⇒λ2=8R9
Similarly, for 3rd order transition we have, n2=4
Putting values we get,
λ31=R(1−421)
⇒λ31=R1615
⇒λ3=15R16
So the difference of 1st&2nd lines of Lyman series is, λ=λ1−λ2
Putting values we get,
λ=3R4−8R9
⇒λ=24R32−27
⇒λ=24R5
So the difference of 2nd&3rd lines of Lyman series is, λ′=λ2−λ3
Putting values we get,
λ′=8R9−15R16
⇒λ′=120R135−128
⇒λ′=120R7
So the required ratio is,
λ′λ=(120R7)(24R5)
⇒λ′λ=725
∴λ:λ′=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.