The magnetic force The Right-hand rule Magnetic field is the analogous field to the electric field for magnetism ultimately electric and magnetic field is just different mirror image of the same thing. magnetic field have no ends—there is no magnetic monopole magnetic goes from north magnetic pole to south magnetic pole we have not found an isolated north or south pole: they are always found in pairs. A moving charge feels a force in a magnetic field ~ B = q~v × B ~ F Make sure your coordinate system is right-handed, then: x̂ × ŷ = ẑ , Magnetism ŷ × ẑ = x̂ , ẑ × x̂ = ŷ . Use any even permutation of the equation. Thumb: first variable. Index: second variable. Middle/Rest: third variable. FB = qvB sin θ N·s unit of magnetic field is Tesla: 1 T = C·m The force is always perpendicular to both the magnetic field and the direction of motion. magnetic force do no work. just like electric field, magnetic field also have energy LMZ (UCSD) Let algebra takes care of everything SS-I ’09 Why the right-hand rule? 1 / 10 Cyclotron motion LMZ (UCSD) Magnetism SS-I ’09 2 / 10 The Hall effect Electromagnetic (Lorentz) force: A particle of charge q and velocity v enter a region of uniform magnetic field B perpendicular to the velocity would under go circular motion. called cyclotron motion. mv cyclotron radius: r = qB qB cyclotron frequency: f = 2πm ~ = qE ~ + q~v × B ~ F A conductor driven by an electric field is placed in a uniform perpendicular magnetic field. Charges is bend toward the edge of the conductor and accumulates there. The accumulated charge creates a cross electric field and potential difference. At equilibrium, the Lorentz force of the cross field cancels the magnetic force. The corresponding potential difference Hall Potential: Cyclotron frequency do not depend on radius. The cyclotron exploit this fact to accelerate charge particles. Modern particle accelerators are descendants of the cyclotron In general there can be also be drift in the direction of magnetic field Magnetic field can “freeze” or “trap” charged particle with potentially very useful application. Magnetic mirroring: gradient in magnetic field tends to prevent particle from entering region of strong magnetic field. Responsible for Aurora Borealis. Protects earth from solar wind. LMZ (UCSD) Magnetism SS-I ’09 VH = What are the directions of current density and total electric field? The integer and fractional quantum Hall effect. One Nobel prize each since 1980 (fractional effect unexplained). Quantum mechanics at macroscopic level—correlated electron effect. Current standard for measuring the value of e. 3 / 10 More magnetic force LMZ (UCSD) Magnetism SS-I ’09 4 / 10 What creates magnetic field? Since magnetic force affects moving charge, an current carrying wire also experience it: Uniform current carried by straight wire in uniform magnetic field: Moving charges or electric current according to the Biot-Savart Law: ~ = dB ~ = I~l × B ~ F ~ = Id~l × B ~ dF Since magnetic monopole do not exist1 , dipolar field is the simplest kind of magnetic field. Natural magnetic field of stars and planet are not well understood due to the exceedingly complex dynamics. Earth’s magnetic field: A current loop constitutes a magnetic dipole: ~ µ ~ =NIA roughly equal to that of a magnetic dipole with dipole moment µ = 8.0 × 1022 A · m2 . due to motion its iron-rich core through not completely understood mechanism. periodic reversal about once every million years that last about 10,000 years. Torque on a magnetic dipole: ~ ~τ = µ ~ ×B with potential energy: ~ U = −~ µ·B Magnetism µ0 Id~l × r̂ 4π r 2 A current loop not only responds to magnetic field like a magnetic dipole, but also creates a dipolar magnetic field. Arbitrarily shaped conductor in non-uniform magnetic field: LMZ (UCSD) IB nql 1 as SS-I ’09 5 / 10 far as we know LMZ (UCSD) Magnetism SS-I ’09 6 / 10 Magnetic force between wires Ampère’s Law Amère’s Law: The line integral of magnetic field along any closed loop is proportional to the steady current penetrating an (any) area bounded by that loop. I ~ · ~l = µ0 Ienclosed B Magnetic field due to a straight wire: B= µ0 I 2πr Magnetic analogue of Gauss’s Law. Magnetic field is not conservative. Eq. above only applies to steady current that do not change with time. Allows trivial calculation of magnetic field in few highly symmetric cases. Direction dictated by the r.h.r. Line current and cyliner: The force between two parallel wire: 1 µ0 I B= × rr 2π R2 µ0 I1 I2 l F= 2πd Parallel current attract; anti-parallel currents repel. Sheet current: B= outside inside 1 µ0 J s 2 Solenoid: B= LMZ (UCSD) Magnetism SS-I ’09 7 / 10 Magnetic material Ferromagnetism: material that can have permanent magnetic moment magnetic domain: quantum-mechanical interaction induced region of aligned magnetic momentum. Usually transition or rare earth metal with many unpaired electron: Fe, Co, Nb. Curie temperature: temperature above which ferromagnetism ceases. Hysteresis: magnetization of a ferromagnet depends on the history of magnetization. A lot of application everywhere and extremely interesting study of thermodynamic. Paramagnetism: has intrinsic magnetic moment that become aligned under magnetic field. Magnetic moment is induced and temporary. Attracts weakly to magnet. Diamagnetism: No intrinsic magnetic moment Describes most material. LMZ (UCSD) Magnetism SS-I ’09 9 / 10 LMZ (UCSD) µ0 nI 0 Magnetism inside outside SS-I ’09 8 / 10