14. 1. Poynting’s Theorem
14. 1. Poynting’s Theorem (Gri ths 8.1.2) ... To understand radiation pressure classically let’s go back to the example of an xpolarised wave propagating in ezdirection: the electric eld moves charges, on the surface the radiation ... radiation" = light bouncing around in all directions; this gives instead p rad= hu
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Quantum Electrodynamics
www2.ph.ed.ac.ukQuantum Electrodynamics Quantum Theory (QED) of Electromagnetic Interactions Classical Electromagnetism Forces arise from Potentials V(r) act instantaneously at a distance QED Picture Forces described by exchange of virtual field quanta - photons Matrix element Full derivation in 2nd order perturbation theory Gives propagator term 1/(q2-m2)
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www2.ph.ed.ac.ukThe spherical harmonics satisfy an orthogonality relation: * 2π 0 dφ * π 0 dθ sinθ, Ym1 l1 (θ,φ)-∗ Ym2 l2 (θ,φ)=δ l1,l2 δ m1,m2. Note that they are orthonormal, not just orthogonal, as the constant multiplying the product of Kronecker deltas is unity. 6.3.1 Completeness and the …
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www2.ph.ed.ac.uk(10) is an important result and is used frequently in electromagnetism, uid mechanics, and other ‘ eld theories’. Finally, when a scalar eld ˚depends only on the magnitude of the position vector r= jrj, we have r2 ˚(r) = ˚00(r) + 2˚0(r) r where the prime denotes di erentiation with respect to r. Proof of this relation is left to the ...
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