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Question 37 of 57

Q.Using an expression for energy of electron, obtain the Bohr's formula for hydrogen spectral lines. OR State the law of radioactive decay. Hence derive the relation N=N0e−λtN = N_0 e^{-\lambda t}. Represent it graphically.

Maharashtra MsbshseMaharashtra HSC (MSBSHSE) Board 2019Subjective· 3mImportance★★★★★
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Bohr's energy expression for the H atom gives the Rydberg/spectral-line formula; separately, radioactive decay follows an exponential law derived from dN/dt∝−NdN/dt \propto -N.

Option — Bohr's formula for hydrogen spectral lines

For the hydrogen atom, the total energy of the electron in the nn-th orbit is

En=−me48ε02h2n2=−13.6n2 eVE_n = -\frac{me^4}{8\varepsilon_0^2h^2n^2} = -\frac{13.6}{n^2}\ \text{eV}

When an electron makes a transition from a higher orbit n2n_2 to a lower orbit n1n_1 (n2>n1n_2>n_1), a photon is emitted with energy equal to the difference:

hν=En2−En1=−me48ε02h2(1n22−1n12)=me48ε02h2(1n12−1n22)h\nu = E_{n_2}-E_{n_1} = -\frac{me^4}{8\varepsilon_0^2h^2}\left(\frac{1}{n_2^2}-\frac{1}{n_1^2}\right) = \frac{me^4}{8\varepsilon_0^2h^2}\left(\frac{1}{n_1^2}-\frac{1}{n_2^2}\right)

Since ν=c/λ\nu = c/\lambda,

1λ=me48ε02h3c(1n12−1n22)=R(1n12−1n22)\frac{1}{\lambda} = \frac{me^4}{8\varepsilon_0^2h^3c}\left(\frac{1}{n_1^2}-\frac{1}{n_2^2}\right) = R\left(\frac{1}{n_1^2}-\frac{1}{n_2^2}\right)

where R=me48ε02h3cR = \dfrac{me^4}{8\varepsilon_0^2h^3c} is the Rydberg constant. This is Bohr's formula for the hydrogen spectral lines: for fixed n1n_1 and varying n2=n1+1,n1+2,…n_2 = n_1+1, n_1+2,\dots, it generates a whole series of spectral lines (Lyman for n1=1n_1=1, Balmer for n1=2n_1=2, etc.).

— OR (alternative) —

Law of radioactive decay: The number of undecayed radioactive nuclei decreases with time such that the rate of decay (−dN/dt-dN/dt) at any instant is directly proportional to the number of undecayed nuclei NN present at that instant:

−dNdt∝N⇒−dNdt=λN-\frac{dN}{dt} \propto N \quad\Rightarrow\quad -\frac{dN}{dt} = \lambda N

where λ\lambda is the decay constant (a characteristic of the radioactive nuclide).

Derivation of N=N0e−λtN=N_0e^{-\lambda t}:

dNN=−λ dt\frac{dN}{N} = -\lambda\,dt

…

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