Moving Charges and Magnetism - Comprehensive Study Notes

Historical Context and Oersted’s Discovery

  • Long-standing Knowledge: Both electricity and magnetism have been recognized for over 2000 years. However, it was not until 1820 that they were realized to be fundamentally connected.
  • Hans Christian Oersted (1820): During a lecture demonstration in the summer of 1820, the Danish physicist Oersted observed that a current in a straight wire caused a deflection in a nearby magnetic compass needle.
    • Needle Alignment: He found that the needle aligns tangentially to an imaginary circle centered on the wire, with the plane of the circle perpendicular to the wire.
    • Current and Proximity: The deflection becomes noticeable when the current is large or when the needle is sufficiently close to the wire, allowing the observer to neglect the Earth’s magnetic field.
    • Reversal and Magnitude: Reversing the current direction reverses the orientation of the needle. The deflection increases with higher current or reduced distance from the wire.
    • Iron Filings: When sprinkled around the wire, iron filings arrange themselves in concentric circles centered on the wire.
  • Conclusion: Oersted concluded that moving charges or currents produce a magnetic field in the surrounding space.
  • Scientific Advancement:
    • 1864: James Maxwell unified the laws of electricity and magnetism, realizing light consists of electromagnetic waves.
    • Late 19th Century: Radio waves were discovered by Hertz and produced by J.C. Bose and G. Marconi.
    • 20th Century: Progress accelerated due to understanding electromagnetism and inventions for the production, amplification, transmission, and detection of electromagnetic waves.

The Lorentz Force and Sources of Fields

  • Electric Field (E) Recap:
    • A source charge QQ produces an electric field EE:
    • E = \frac{Q \times \text{̒{r}}}{4̒̒̒̒_0 \times r^2}
    • A charge qq interacting with this field experiences a force: F=q×EF = q \times E.
    • The field is a physical entity that conveys energy and momentum, propagating at a finite speed.
  • Magnetic Field (B): Like the electric field, current or moving charges produce a magnetic field denoted by B(r)B(r).
    • It is a vector field defined at each point in space and time.
    • Principle of Superposition: The magnetic field of several sources is the vector sum of the fields from each individual source.
  • Lorentz Force Equation: The total force on a charge qq moving with velocity vv in the presence of both electric and magnetic fields is given by:
    • F=q[E(r)+v×B(r)]=Felectric+FmagneticF = q [ E(r) + v \times B(r)] = F_{electric} + F_{magnetic}
  • Features of Magnetic Force (Fmagnetic=q[v×B]F_{magnetic} = q [ v \times B ]):
    • It depends on the charge qq, velocity vv, and magnetic field BB. The force on a negative charge is opposite to that on a positive charge.
    • Vector Product: The force vanishes if the velocity and magnetic field are parallel or anti-parallel (angle is 0° or 180°).
    • Direction: The force acts perpendicularly to both the velocity and the magnetic field. Its direction is determined by the Right-Hand Rule or the Screw Rule.
    • Static Charges: The magnetic force is zero if the charge is not moving (∣v∣=0|v| = 0). Only moving charges experience magnetic force.

Magnetic Field Units and Constants

  • Magnitude Definition: The magnitude of magnetic field BB is 1 SI unit when the force on 1 Coulomb (1‐C1‐C) moving perpendicular to BB at 1‐m/s1‐m/s is 1 Newton (1‐N1‐N).
  • Dimensional Formula: [B]=[F/(q×v)][B] = [F / (q \times v)]
  • Units:
    • SI Unit: Tesla (TT), named after Nikola Tesla (1856–1943). Also expressed as Newton•second / (coulomb•meter).
    • CGS Unit: Gauss (GG). 1‐G=10−4‐T1‐G = 10^{-4}‐T.
    • Earth’s Magnetic Field: Approximately 3.6×10−5‐T3.6 \times 10^{-5}‐T or 0.36‐G0.36‐G.
  • Permeability of Free Space (̒_0):
    • \frac{̒_0}{4̒} = 10^{-7}‐T \times m/A.
  • Relation to Light Speed: The speed of light in vacuum cc is related to permittivity (̒_0) and permeability (̒_0) by:
    • ̒_0 \times ̒_0 = \frac{1}{c^2}

Magnetic Force on a Current-Carrying Conductor

  • Derivation: Consider a rod of cross-sectional area AA, length ll, and number density of mobile carriers nn.
    • Total charge carriers: (n×l×A)(n \times l \times A).
    • Force on carriers in field BB: F=(n×l×A)×q×vd×BF = (n \times l \times A) \times q \times v_d \times B, where vdv_d is the drift velocity.
    • Since current density j=n×q×vdj = n \times q \times v_d and current I=∣j∣×AI = |j| \times A, the force simplifies to:
    • F=I×l×BF = I \times l \times B
    • Here, ll is a vector with magnitude equal to the length of the rod and direction matching the current flow.
  • Arbitrary Shapes: If a wire has an irregular shape, the total force is the integral of infantisimal elements: F=∑I×dlj×B→∫I×dl×BF = ∑ I \times dl_j \times B \rightarrow ∫ I \times dl \times B.
  • Example 4.1: A straight wire (200‐g200‐g, 1.5‐m1.5‐m) carrying 2‐A2‐A is suspended in mid-air by a horizontal magnetic field BB.
    • Force balance: m×g=I×l×Bm \times g = I \times l \times B
    • B=m×gI×l=0.2×9.82×1.5=0.65‐TB = \frac{m \times g}{I \times l} = \frac{0.2 \times 9.8}{2 \times 1.5} = 0.65‐T.

Motion of Charged Particles in Magnetic Fields

  • Work Done: Since the magnetic force is always perpendicular to velocity (F∕vF ∕ v), the work done by the magnetic field on a charge is zero (W=0W = 0). The magnitude of velocity (kinetic energy) remains constant, but the direction changes.
  • Circular Motion (v∕Bv ∕ B):
    • The magnetic force acts as a centripetal force: m×v2r=q×v×B\frac{m \times v^2}{r} = q \times v \times B.
    • Radius: r=m×vq×Br = \frac{m \times v}{q \times B}.
    • Angular Frequency (̒): ̒ = \frac{v}{r} = \frac{q \times B}{m}.
    • Frequency (̒): ̒ = \frac{q \times B}{2̒ \times m}.
    • Time Period (TT): T = \frac{2̒ \times m}{q \times B}.
    • Crucially, frequency and period are independent of the particle’s speed and radius.
  • Helical Motion: If the velocity has a component parallel to the magnetic field (v_{||} = v \times \text{cos}(̒)), the particle moves along the field lines while rotating, creating a helix.
    • Pitch (pp): The distance moved along the field in one rotation:
    • p = v_{||} \times T = \frac{2̒ \times m \times v_{||}}{q \times B}.

Biot-Savart Law

  • Definition: This law relates the magnetic field dBdB at a point PP to an infinitesimal current element I×dlI \times dl at distance rr.
    • dB = \frac{̒_0}{4̒} \times \frac{I \times dl \times r}{r^3}
    • Vector Form Magnitude: dB = \frac{̒_0}{4̒} \times \frac{I \times dl \times \text{sin}(̒)}{r^2}.
  • Comparison to Coulomb’s Law:
    1. Similarities: Both are long-range (1/r21/r^2 dependence) and obey the principle of superposition.
    2. Source: Electric field is produced by a scalar (charge); magnetic field is produced by a vector (current element I×dlI \times dl).
    3. Direction: Electric field is along the displacement vector; magnetic field is perpendicular to the plane of dldl and rr.
    4. Angle Dependence: Biot-Savart law depends on the angle ̒ between dldl and rr; the field is zero along the line of the current element.

Magnetic Field of a Circular Current Loop

  • On-Axis Calculation: For a loop of radius RR carrying current II, at distance xx from the center along the axis:
    • B = \frac{̒_0 \times I \times R^2}{2(x^2 + R^2)^{3/2}}
  • At the Center (x=0x = 0):
    • B = \frac{̒_0 \times I}{2 \times R}
  • Field Lines: The field lines form closed loops. The direction is given by the Right-Hand Thumb Rule: Curl fingers in the direction of the current, and the thumb indicates the direction of the magnetic field.
  • Example 4.6: A 100-turn coil of radius 10‐cm10‐cm carrying 1‐A1‐A current:
    • B = \frac{100 \times ̒_0 \times I}{2 \times R} = 6.28 \times 10^{-4}‐T.

Ampere’s Circuital Law

  • Statement: The line integral of the magnetic field BB around a closed loop is equal to ̒_0 times the total current II passing through the surface enclosed by the loop:
    • ∮ B ⋅ dl = ̒_0 \times I
  • Right-Hand Rule for Signs: Curl fingers in the direction of the integral traversal; the thumb indicates the positive direction for current.
  • Solenoid Field: A solenoid is a long wire wound into a helix. Inside a long solenoid, the field is uniform and parallel to the axis; reaching outside, the field is nearly zero.
    • B = ̒_0 \times n \times I
    • Here, nn is the number of turns per unit length.
  • Straight Infinite Wire: Applying Ampere's Law to a circle of radius rr surrounding a wire:
    • B \times (2̒ \times r) = ̒_0 \times I \rightarrow B = \frac{̒_0 \times I}{2̒ \times r}.

Force Between Two Parallel Currents

  • Parallel Currents: Two long parallel conductors separated by distance dd carrying currents IaI_a and IbI_b.
    • Field due to 'a' at 'b': B_a = \frac{̒_0 \times I_a}{2̒ \times d}.
    • Force on length LL of 'b': F_{ba} = I_b \times L \times B_a = \frac{̒_0 \times I_a \times I_b \times L}{2̒ \times d}.
  • Directional Strength:
    • Parallel currents attract.
    • Anti-parallel currents repel.
  • Definition of the Ampere (SI Unit): One Ampere is the steady current which, when maintained in two infinitely long parallel conductors 1 meter apart in vacuum, produces a force of 2×10−7‐N/m2 \times 10^{-7}‐N/m on each conductor.

Torque on Current Loops and Galvanometers

  • Torque Calculation: A rectangular loop of area AA carrying current II in a uniform field BB experiences a torque:
    • ̒ = m \times B
    • Where mm is the magnetic moment: m=N×I×Am = N \times I \times A.
    • Magnitude: ̒ = N \times I \times A \times B \times \text{sin}(̒).
  • Moving Coil Galvanometer (MCG):
    • Principle: A current-carrying coil in a magnetic field experiences a torque that is balanced by a spring's restoring torque.
    • Equilibrium: k \times ̒ = N \times I \times A \times B, where kk is the torsional constant of the spring.
    • Deflection: ̒ = (\frac{N \times A \times B}{k}) \times I.
    • Radial Field: Achieved via a cylindrical soft iron core, ensuring \text{sin}(̒) = 1.
  • Instrument Conversions:
    • Ammeter: Connect a small shunt resistance (rsr_s) in parallel with the galvanometer.
    • Voltmeter: Connect a large resistance (RR) in series with the galvanometer.
  • Sensitivity:
    • Current Sensitivity: \frac{̒}{I} = \frac{N \times A \times B}{k}.
    • Voltage Sensitivity: \frac{̒}{V} = \frac{N \times A \times B}{k \times R_{galvanometer}}.
    • Note: Doubling the number of turns doubles current sensitivity but might not change voltage sensitivity as the resistance also increases.