Important
Closest Distance of Approach (α-particle)
\[ R = \frac{4KZe^2}{m_\alpha V_\alpha^2} \]
K = Coulomb's constant, Z = atomic number, e = charge, m_α = mass of α-particle
Radius of Nucleus
\[ R = R_0 A^{1/3} \text{ cm} \]
R₀ ≈ 1.2 × 10⁻¹³ cm; A = mass number
Key
Planck's Quantum Theory — Energy of Photon
\[ E = h\nu = \frac{hc}{\lambda} \]
h = 6.626×10⁻³⁴ J·s; c = 3×10⁸ m/s
Photoelectric Effect
\[ h\nu = h\nu_0 + \frac{1}{2}m_e v^2 \]
ν₀ = threshold frequency; ½mₑv² = kinetic energy of ejected electron
Key
Bohr's Model — Quantization of Angular Momentum
\[ mvr = n\frac{h}{2\pi} \]
n = principal quantum number (1,2,3…)
Important
Energy of Electron (Bohr Model)
\[ E_n = -\frac{E_1 z^2}{n^2} = -2.178\times10^{-18}\frac{z^2}{n^2}\ \text{J/atom} = -13.6\frac{z^2}{n^2}\ \text{eV} \]
E₁ = −13.6 eV for hydrogen; z = atomic number; n = orbit number
Radius of nth Orbit (Bohr)
\[ r_n = \frac{n^2}{Z} \times \frac{h^2}{4\pi^2 e^2 m} = \frac{0.529\,n^2}{Z}\ \text{Å} \]
Velocity of Electron (Bohr)
\[ v = \frac{2\pi ze^2}{nh} = \frac{2.18\times10^6\,z}{n}\ \text{m/s} \]
Key
de-Broglie Wavelength
\[ \lambda = \frac{h}{mc} = \frac{h}{p} \]
p = momentum; for particles: λ = h/mv
Rydberg Formula (Spectral Lines)
\[ \frac{1}{\lambda} = \bar{\nu} = Rz^2\!\left(\frac{1}{n_1^2} - \frac{1}{n_2^2}\right) \]
R = Rydberg constant = 1.097×10⁷ m⁻¹
No. of Spectral Lines (from level n)
\[ \text{Lines} = \frac{n(n-1)}{2} \quad\text{(or }\ \frac{\Delta n(\Delta n+1)}{2}\text{)} \]
Heisenberg's Uncertainty Principle
\[ \Delta x \cdot \Delta p \geq \frac{h}{4\pi} \quad;\quad m\Delta x\cdot\Delta v \geq \frac{h}{4\pi} \]
NEET Key
Orbital Angular Momentum
\[ L = \frac{h}{2\pi}\sqrt{\ell(\ell+1)} = \hbar\sqrt{\ell(\ell+1)} \]
ℓ = azimuthal quantum number (0,1,…,n−1)
Quantum Numbers Summary
Orbitals in subshell: \(2\ell+1\)
Max electrons in subshell: \(2(2\ell+1)\)
n: 1,2,3,… | ℓ: 0 to n−1 | mₗ: −ℓ to +ℓ | mₛ: ±½