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Fields

Fields

Fields describe the region of space around an object where another object experiences a force without physical contact. This section covers gravitational fields, electric fields, and magnetic fields — and their unification through electromagnetic induction.

Topics Covered

Gravitational Fields

  • Newton’s law of gravitationF=GMmr2F = \frac{GMm}{r^2}; inverse square law
  • Gravitational field strengthg=GMr2g = \frac{GM}{r^2}; radial fields around point masses; uniform fields near Earth’s surface (g9.81N/kgg \approx 9.81\,\text{N/kg})
  • Gravitational potentialVg=GMrV_g = -\frac{GM}{r}; potential energy Ep=GMmrE_p = -\frac{GMm}{r}; work done moving mass in a field
  • Orbits — circular orbits: F=mv2rF = \frac{mv^2}{r}; geostationary and polar orbits; escape velocity vesc=2GMrv_{\text{esc}} = \sqrt{\frac{2GM}{r}}

Electric Fields

  • Coulomb’s lawF=Q1Q24πε0r2F = \frac{Q_1 Q_2}{4\pi\varepsilon_0 r^2}; similarity to gravitational force but with charge
  • Electric field strengthE=FQ=Q4πε0r2E = \frac{F}{Q} = \frac{Q}{4\pi\varepsilon_0 r^2} (radial); E=VdE = \frac{V}{d} (uniform between plates)
  • Electric potentialVe=Q4πε0rV_e = \frac{Q}{4\pi\varepsilon_0 r}; potential energy Ep=Q1Q24πε0rE_p = \frac{Q_1 Q_2}{4\pi\varepsilon_0 r}
  • Uniform fields — between parallel plates; force on charge F=QEF = QE; motion of charged particles (parabolic paths analogous to projectile motion)
  • Comparison: gravitational vs. electric fields — both follow inverse square laws, but gravity is always attractive while electric fields can be attractive or repulsive

Magnetic Fields

  • Magnetic flux densityBB; the tesla; F=BIlsinθF = BIl\sin\theta for current-carrying conductors
  • Fleming’s left-hand rule — determining force direction on a current in a magnetic field
  • Charged particles in magnetic fields — circular motion with radius r=mvBQr = \frac{mv}{BQ}; frequency independent of speed
  • Magnetic flux and flux linkageΦ=BAcosθ\Phi = BA\cos\theta; NΦ=BANcosθN\Phi = BAN\cos\theta

Electromagnetic Induction

  • Faraday’s lawε=d(NΦ)dt\varepsilon = -\frac{d(N\Phi)}{dt}; induced EMF equals rate of change of flux linkage
  • Lenz’s law — the induced current opposes the change producing it; conservation of energy
  • AC generatorε=BANωsin(ωt)\varepsilon = BAN\omega\sin(\omega t); peak EMF and RMS values
  • TransformersVsVp=NsNp\frac{V_s}{V_p} = \frac{N_s}{N_p}; efficiency and power transmission

Study Tips

  1. Compare gravitational and electric fields explicitly — learn the parallels (inverse square laws, potential equations) and the differences (attractive only vs. attractive/repulsive, mass vs. charge).
  2. Use Fleming’s left-hand rule physically — actually hold your left hand in the correct orientation. Practise until it’s automatic.
  3. Derive orbital velocity from combining GMmr2\frac{GMm}{r^2} with mv2r\frac{mv^2}{r} — this derivation appears frequently.
  4. Practise Lenz’s law — for any situation, ask “what change is happening?” and then “what current would oppose this change?”
  5. Sketch field lines — radial (point mass/charge), uniform (between plates), and the combined fields.

How to Use These Notes

Follow the sidebar order. Each page provides physical principles, derivations from first principles, worked examples, and exam-style problems. Start with gravitational fields, then electric fields, then magnetic fields and electromagnetic induction.