MIT OpenCourseWare http://ocw.mit.edu 3.23 Electrical, Optical, and Magnetic Properties of Materials Fall 2007 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 3.23 Fall 2007 – Lecture 17 FERMAT’s FIRST THEOREM Image removed due to copyright restrictions. Please see: http://en.wikipedia.org/wiki/ Image:Ibn_haithem_portrait.jpg Abū ʿAlī al-Ḥasan ibn al-Ḥasan ibn al-Haytham Pierre-Louis Moreau de Maupertuis Hero 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Last time 1. 2. 3. 4. 5. Electric field, polarization, displacement, susceptibility M Maxwell’s ll’ equations ti Potentials and gauges Electromagnetic waves (no free charges, currents) Refractive index, phase and group velocity 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 1 Study • (mostly read) Fox, Fox Optical Properties of Solids: 1.1 to 1.4, 2.1 to 2.2.3, 3.1 to 3.3 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Polarization, transversality of EM fields 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 2 Boundary conditions (Gauss theorem) ∫ r r ∇ ⋅ Bdv = ∫ r r ∇ ⋅ Ddv = volume ∫ r ˆ =0 B ⋅ ndS ∫ r ˆ = 4π D ⋅ ndS surface volume surface ∫ ρ dv volume 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Boundary conditions r r nˆ ⋅ B2 − B1 = 0 ( ) r r ˆn ⋅ D2 − D1 = σ (σ = surface charge g densityy )) ( ) 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 3 Boundary conditions (Stokes theorem) r r ˆ = ∇ × E ⋅ ndS ∫ surface ∫ r r E ⋅ dr line 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Boundary conditions r r n̂ × E2 − E1 = 0 r r r nˆ × H 2 − H1 = K r K = surface current density ( ( ( ) ) ) 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 4 Snell’s law r r r Ei eωt −iki ⋅r incident wave r r r Er eωt −ikr ⋅r reflected wave r r r Et eωt −ikt ⋅r transmitted wave Image from Wikimedia Commons, http://commons.wikimedia.org 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Snell’s law r r ωn ki = k r = 1 c r ωn kt = 2 c Image from Wikimedia Commons, http://commons.wikimedia.org 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 5 Snell’s law r ( k ⋅ rr ) 1 (k 1y x=0 r r = k1′ ⋅ r ( ) x=0 r r = k2 ⋅ r ( ) x=0 y + k1z z ) = ( k1y′ y + k1z′ z ) = ( k2 y y + k2 z z ) → k1y = k1y′ = k2 y and k1z = k1′z = k2 z ( r r r r r r k1t ⋅ rt = k1t′ ⋅ rt = k2t ⋅ rt ) ( ) ( ) 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Snell’s law r r ω k1 = k1′ = n1 c r ω k2 = n2 c kiz = ktz → ki sin θ1 = kt sin θ 2 ω n1 c sin θ1 = ω n2 c sin θ 2 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 6 Snell’s law r ω ⎫ k1z = k1 sin θ1 = n1 sin θ1 ⎪ ⎪ c ⎬ n1 sin θ1 = n2 sin θ 2 r ω k2 z = k2 sin θ 2 = n2 sin θ 2 ⎪ ⎪⎭ c 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Principle of least action 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 7 Energy law r r r r r r r r 4π r r 1 r ∂D 1 r ∂B E ⋅∇ × H − H ⋅∇ × E = J ⋅E + E⋅ + H⋅ c c ∂t c ∂t r r r r r r r r r E ⋅∇ × H − H ⋅∇ × E = −∇ ⋅ E × H r r 4π r r 1 r ∂D 1 r ∂B r r r → J ⋅E + E⋅ + H⋅ +∇⋅ E× H = 0 c c ∂t c ∂t Apply Gauss's theorem r r r r ⎛ 1 r ∂D 1 r ∂B ⎞ 4π r r ⋅ + ⋅ + ⋅ + J Edv E H dv E ∫c ∫ ⎜⎝ c ∂t c ∂t ⎟⎠ ∫ × H ⋅ nˆdS = 0 ( ) ( ) ( ) 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Energy law 1 4π 1 4π r r r r r2 r ∂D 1 r ∂ε E 1 ∂ε E 1 ∂ E⋅D E⋅ = E⋅ = = ∂t 4π ∂t ∂t 8π ∂t 8π r r r r ∂B 1 ∂ H ⋅ B = H⋅ ∂t 8π ∂t ( ( ) ) 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 8 Energy conservation r r r r r r r r ∂ ˆ =0 E ⋅ D + H ⋅ B dv + ∫ E × H ⋅ ndS ∫ J ⋅ Edv + ∂t ∫ 14 4244 3 1 424 3 ( ) total energy stored in electrical and magnetic field per volume ( ) energy surface flux per unit area r c r r S= E×H 4π 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Optical processes • • • • Reflection and refraction Absorption Luminescence Scattering 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 9 Optical coefficients T: ratio of transmitted vs incident power R+T=1 (no absorption, scattering) Absorption: Transmission: 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Complex refractive index n% = n + ik k 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 10 Complex refractive index Image removed due to copyright restrictions. Please see any image of the structure of amorphous silica, such as http://www.research.ibm.com/amorphous/figure1.gif. Courtesy of Elsevier, Inc., http://www.sciencedirect.com. Used with permission. 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Modeling Optical Constants with a Damped Harmonic Oscillator d 2 X dX + m0γ + m0ω02 X = −eE ( t ) m0 2 1 424 3 123 2 dt dt { 1 424 3 harmonic restoring time dependent acceleration dissipation force electric field 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 11 Modeling Optical Constants with a Damped Harmonic Oscillator X0 = Presonant = Np = −NeX = −eE0 m0 (ω − ω 2 − iγω ) 2 0 Ne 2 E m0 (ω02 − ω 2 − iγω ) 14442444 3 α Ne 2 E =εE m0 (ω02 − ω 2 − iγω ) 144424443 D = E + 4π P + 4π Presonantt = E + 4πχ E + 4π α Atomic polarizability = α 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Modeling Optical Constants with a Damped Harmonic Oscillator ε = 1 + 4πχ + 4π ( Ne 2 (ω02 − ω 2 ) ) m0 (ω02 − ω 2 ) + γ 2ω 2 144444424444443 2 ε1 − i 4π ( Ne 2γω γ ) m0 (ω02 − ω 2 ) + γ 2ω 2 14444244443 2 ε2 2 ε = ( n + ik ) = n12 −3 k 2 + i 2{ nk 123 2 ε1 ε2 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 12 Amorphous silica ε' ε" Figure by MIT OpenCourseWare. Courtesy of Elsevier, Inc., http://www.sciencedirect.com. Used with permission. 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Optical materials Image removed . due to copyright restrictions Please see: Fig. 1.4 in Fox, Mark. Optical Properties of Solids. Oxford, England: Oxford University Press, 2001. 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 13 Infrared active modes Image removed due to copyright restrictions. Please see Fig. 1a and 2a in Giannozzi, Paolo, et al. "Ab initio Calculation of Phonon Dispersions in Semiconductors." Physical Review B 43 (March 15, 1991): 7231-7242. 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Optical materials Image removed due to copyright restrictions. Please see: Fig. 1.7 in Fox, Mark. Optical Properties of Solids. Oxford, England: Oxford University Press, 2001. 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 14 Optical materials Image removed due to copyright restrictions. Please see: Fig. 1.5 in Fox, Mark. Optical Properties of Solids. Oxford, England: Oxford University Press, 2001. 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) Transition rate for direct absorption Image removed due to copyright restrictions. Please see any diagram of GaAs energy bands, such as http://ecee.colorado.edu/~bart/book/book/chapter2/gif/fig2_3_6.gif. 3.23 Electronic, Optical and Magnetic Properties of Materials - Nicola Marzari (MIT, Fall 2007) 15