Scattering of light Physics 123 7/24/2016 Lecture XI 1 Test #1 • March 8- in lecture class (12:30-1:45pm) • Equation sheet will be provided with the test – Review it in advance – available on the web • HW#6 is based on Chapters 33-37 to help you prepare for the test • Lecture #14 – review, send requests (e.g. homework problems) • HW#7 – light and conceptual, but more work after spring break 7/24/2016 Lecture XI 2 Electron and EM wave • Prediction from classical EM • Electric field exerts a force on an electron acceleration electron radiates EM wave • Oscillating electric field (frequency f) on electron forced oscillator with the same frequency radiation at the same frequency f • An electron will scatter EM wave frequency f, wavelength l in all directions without changing its frequency and wavelength. • Rayleigh scattering 1 E - l4 • Blue-violet light gets scattered more than redorange than is why the sky is blue 7/24/2016 Lecture XI 3 Photons – particles of light • Photon= particle of light = quantum of light = gamma(g)-quant • Each photon carries energy proportional to the frequency of the EM wave: Eg=hf=hc/l • Photon has zero mass m0=0, it is always (and in any inertial frame of reference) moving at the speed of light v=c • Photon’s momentum can be calculated from relativistic formula pg=h/l E p c m c p c 2 2 2 2 4 0 2 2 E pc p E/c h/l 7/24/2016 Lecture XI 4 Collisions: Compton effect • EM wave – collection of photons • Light particle – photon scatters of electron at rest: Eg=Eg’+KEe • Electron gets some energy photon looses energy • Eg goes down f goes down wave length l goes up: l’>l • Expect maximum change (longest l) for back scattering (fp) 7/24/2016 Lecture XI KEe Eg Eg’ 5 Compton effect • Calculate wavelength of scattered photon as a function of angle with respect to its initial direction f • Energy and momentum is conserved Eg Ee me c Eg ' Energy-momentum pg pe p'g conservation Ee Eg 2 E pe c me c 2 e 2 2 Eg pg c 7/24/2016 2 4 Eg’ “Dispersion” equations Relate energy, momentum and mass Lecture XI 6 Compton effect Ee Eg me c 2 Eg ' pe pg p'g Ee Eg E pe c me c 2 e 2 2 2 4 Eg pg c hc / l Eg’ ( Ee Eg me c 2 Eg ' ) 2 Ee Eg me c 4 Eg '2 2( Eg Eg ' )me c 2 2 Eg Eg ' 2 2 2 2 ( pe pg p'g ) c pe c 2 Eg Eg '2 2 Eg Eg ' cos 2 2 2 Ee pe c 2 me c 4 2( Eg Eg ' )me c 2 2 Eg Eg ' (1 cos ) 2 2 2 me c 4 me c 4 2( Eg Eg ' )me c 2 2 Eg Eg ' (1 cos ) 2 2 ( Eg Eg ' )me c 2 Eg Eg ' (1 cos ) 7/24/2016 Lecture XI 7 Compton effect Eg pg c hc / l Ee Eg ( Eg Eg ' )me c 2 Eg Eg ' (1 cos ) hc hc (hc) 2 1 ll ' (1 cos ) 2 l l ' me c ll ' hc h l 'l (1 cos ) me c Eg’ h l' l (1 cos ) me c 7/24/2016 Lecture XI 8 Compton effect h l' l (1 cos ) Always positive change me c Ee Eg f 0 cos 1 l ' l No change ~no interaction 2h Max change f p cos 1 l ' l me c Back scattering h f p / 2 cos 0 l ' l me c Compton wavelength Eg’ Note how small! h hc 1243eV nm 3 lC 1 . 4 10 nm 1.4 pm 2 6 me c me c 0.5 10 eV 7/24/2016 Lecture XI 9 Pair production • A piece of antimatter Positron – antipartner of electron – same Emass, opposite charge • When matter and antimatter meet Eg (positron and electron collide) they annihilate – produce light • It can go in the opposite direction e+ after as well collision • A photon can create matter, such as the production of a positron E+ and electron pair. • Minimum energy of the photon for pair production from energy hc 1243eV nm conservation: 12 l 1 . 2 10 m 6 2 Eg=2mec =2 0.5MeV=1MeV E 110 eV 7/24/2016 Lecture XI 10 Light interaction with matter Eg • Rayleigh scattering • Photoelectric effect – photon is absorbed and an electron is knocked out • Excitation – absorbed by atoms that go to an excited state. Atom goes to ground state and emits a photon. • Compton scattering – wavelength is increased • Electron-positron pair production 7/24/2016 l 1-100 eV 500-10nm ~1-10 eV ~500nm 1-20 eV 500-100nm 0.5MeV 2.43pm >1MeV <1.2pm Lecture XI 11 Light interaction with matter 7/24/2016 Lecture XI 12