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
Example Problem
An electron (q=1.6×10⁻¹⁹ C) has acceleration a=10²⁰ m/s². Find the radiated power using Larmor formula.
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.
Exercises
7 problemsAn electron with a=5×10¹⁹ m/s². Find the Larmor radiated power in mW.
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.
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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Upgrade to Pro →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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Upgrade to Pro →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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Upgrade to Pro →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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Upgrade to Pro →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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Upgrade to Pro →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