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Overview: Atoms

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Estimated time: 28 minutes
CBSE: Class 12

Formula: Coulomb Force between α-particle and Nucleus

\[F=\frac{1}{4\pi\varepsilon_0}\frac{(2e)(Ze)}{r^2}\]

Where:

  • Z = atomic number

  • r = distance between α-particle and nucleus

CBSE: Class 12

Formula: Distance of Closest Approach

\[d=\frac{1}{4\pi\varepsilon_0}\frac{2Ze^2}{K}\]

CBSE: Class 12

Formula: Electron in Circular Orbit

Centripetal Force = Electrostatic Force

\[\frac{1}{4\pi\varepsilon_0}\frac{e^2}{r^2}=\frac{mv^2}{r}\]

CBSE: Class 12

Formula: Relation between Radius and velocity

\[r=\frac{e^2}{4\pi\varepsilon_0mv^2}\]

CBSE: Class 12

Formula: Energies

Kinetic Energy:

\[K=\frac{1}{2}mv^2\]

Potential Energy:

\[U=-\frac{e^2}{4\pi\varepsilon_0r}\]

Total Energy:

\[E=-\frac{e^2}{8\pi\varepsilon_0r}\]

CBSE: Class 12

Key Points: Bohr’s Model – Three Postulates

Postulate 1:

An atom could revolve in certain stable orbits without the emission of radiant energy.

Postulate 2:

The electron revolves around the nucleus only in those orbits for which the angular momentum is some integral multiple of h/2π, where h is Planck’s constant (= 6.6 × 10–34 J s). Thus, the angular momentum (L) of the orbiting electron is quantised. That is

\[L=\frac{nh}{2\pi}\]

Postulate 3:

An electron might make a transition from one of its specified non-radiating orbits to another of lower energy. 

\[h\nu=E_i-E_f\]

CBSE: Class 12

Formula: Radius of nth Orbit

\[r_n=\frac{\varepsilon_0n^2h^2}{\pi me^2}\]

CBSE: Class 12

Formula: Energy of nth Orbit

\[E_n=-\frac{13.6}{n^2}\mathrm{~eV}\]

CBSE: Class 12

Formula: Frequency of Emitted Radiation

\[h\nu=E_{n_i}-E_{n_f}\]

Since ni and nf are integers → Discrete line spectrum

CBSE: Class 12

Key Points: Rutherford’s Nuclear Model

Based on the experiment, Rutherford proposed that:

  • An atom has a small, dense, positively charged nucleus at its centre.

  • Almost all the mass of the atom is concentrated in the nucleus.

  • Electrons revolve around the nucleus.

  • Most of the atom is empty space.

CBSE: Class 12

Definition: Impact parameter

The impact parameter is the perpendicular distance of the initial velocity vector of the a-particle from the centre of the nucleus.

CBSE: Class 12

Definition: Emission Spectrum

When an excited gas emits radiation of specific discrete wavelengths, it produces bright lines on a dark background called an emission line spectrum.

CBSE: Class 12

Definition: Absorption Spectrum

When white light passes through a gas, some wavelengths are absorbed and appear as dark lines in the continuous spectrum, called the absorption spectrum

CBSE: Class 12

Key Points: Important Constants

Quantity Value
Planck’s constant (h) \[6.6\times10^{-34}\mathrm{Js}\]
Electron charge (e) \[1.6\times10^{-19}\mathrm{C}\]
1 eV \[1.6\times10^{-19}\mathrm{」}\]
Bohr radius \[5.3\times10^{-11}\mathrm{m}\]
Ground state energy –13.6 eV
CBSE: Class 12

Formula: De Broglie Theory and Bohr’s Quantisation

Formula Meaning
\[\lambda=\frac{h}{mv}\] de Broglie wavelength
\[2\pi r_n=n\lambda\] Standing wave condition
\[mvr_n=\frac{nh}{2\pi}\] Bohr quantisation
CBSE: Class 12

Key Points: Limitations of Bohr Model

  1. Applicable only to hydrogenic atoms

  2. Cannot explain multi-electron atoms

  3. Cannot explain the relative intensity of spectral lines

  4. Does not include electron–electron interaction

CBSE: Class 12

Key Points: Limitations of Rutherford Model

1. An atom should be unstable

  • Electron is accelerating
  • Accelerating charge radiates energy
  • Electron should spiral into the nucleus

2. Cannot explain the line spectrum of hydrogen

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