← Electrodynamics
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Electromagnetic Radiation

An accelerating charge radiates electromagnetic energy. For non-relativistic motion, the radiated power is given by the Larmor formula. Oscillating electric dipoles are the simplest radiating systems and form the basis of antenna theory.

Key Concepts

  • Larmor formula: P = q²a²/(6πε₀c³)
  • Electric dipole radiation: P = ω⁴p₀²/(12πε₀c³)
  • Radiation pattern: dipole has sin²θ angular dependence
  • Radiation resistance of antenna: P = I²R_rad
  • Cyclotron radiation from circular motion in magnetic field

Key Equations

Larmor formula
P=q2a26πε0c3P = \frac{q^2 a^2}{6\pi\varepsilon_0 c^3}
Dipole radiated power
P=μ0ω4p0212πcP = \frac{\mu_0 \omega^4 p_0^2}{12\pi c}
Radiation intensity
dPdΩ=μ0q2a216π2csin2θ\frac{dP}{d\Omega} = \frac{\mu_0 q^2 a^2}{16\pi^2 c}\sin^2\theta
Cyclotron frequency
ωc=qBm\omega_c = \frac{qB}{m}
Worked Example

Example Problem

Problem

An electron (q=1.6×10⁻¹⁹ C) has acceleration a=10²⁰ m/s². Find the radiated power using Larmor formula.

Solution

P = q²a²/(6πε₀c³) = (1.6×10⁻¹⁹)²×(10²⁰)²/(6π×8.854×10⁻¹²×(3×10⁸)³) = 2.56×10⁻³⁸×10⁴⁰/(5.093×10¹¹) = 1.52 W.

Practice

Exercises

7 problems
1 of 7

An electron with a=5×10¹⁹ m/s². Find the Larmor radiated power in mW.

mW
2 of 7

A dipole antenna (p₀=10⁻²⁹ C·m) oscillates at f=100 MHz (ω=6.28×10⁸ rad/s). Find total radiated power in pW.

pW
3 of 7

An electron moves in a circle (r=0.5 cm) in B=0.01 T. Find the cyclotron frequency f_c in GHz.

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4 of 7

Synchrotron radiation: a proton (γ=100, m=1.67×10⁻²⁷ kg) in B=1.0 T. Find the cyclotron frequency (non-relativistic formula f_c = qB/(2πm)) in MHz.

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5 of 7

The radiation resistance of a short dipole (L≪λ) is R_rad = 80π²(L/λ)². For L/λ = 0.1, find R_rad in Ω.

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6 of 7

Total radiated power from a half-wave dipole with I₀=1.0 A and R_rad=73.1 Ω in W.

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7 of 7

The angular power distribution from a dipole: dP/dΩ = P_total×(3/8π)sin²θ. At θ=90°, find dP/dΩ in W/sr for P_total=10 mW.

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Key Takeaways

  • The Larmor formula P = q²a²/(6πε₀c³) governs non-relativistic radiation
  • Dipole radiation power scales as ω⁴, strongly favoring high frequencies
  • The radiation pattern of a dipole has sin²θ angular dependence
  • Cyclotron and synchrotron radiation arise from magnetic deflection of charges