Coherence in Beams
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Coherence in Beams Jörg Rossbach University of Hamburg & DESY CERN Accelerator School (CAS) on Free-Electron Laser and Energy Recovery Linac 31 May – 10 June, 2016, Hamburg Contents This lecture will address some basic issues -- details and solutions will be given in later lectures --- or (even better) in your own studies • Why coherence ? • Basics on wave propagation • Interference • Transverse coherence • Longitudinal coherence • Correlation functions • Coherent matter waves 0 p o s itio n / m m CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 2 Why coherence? Electro-magnetic radiation comes in waves: amplitudes and phases -- and we have to cope with it ! Structure of biological macromolecule reconstructed from diffraction pattern of protein crystal: LYSOZYME , MW=19,806 Images courtesy Janos Hajdu CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 3 Coherence of a single photon pulse from an FEL courtesy Janos Hajdu SINGLE MACROMOLECULE simulated image Needs very high radiation power @ λ ≈1Å CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 4 CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 4 Why Coherence ? Diffraction from LCLS X-ray FEL/Stanford: D. Li, et al., DOI: 10.1038/ncomms10140 (2016) CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 5 Basics on wave propagation 1. At some distance from the source, a wave front propagates indepentently Huygens Principle: Each point on the wave front can be considered the origin of a spherical wave, the new wave front being the envelope of these wavelets applicable for e.m., water, acoustic, matter waves Basics for diffraction 2. The e.m. wave equation is linear If two waves , are solutions, then will be a solution as well ! Basics for interference CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 6 Diffraction from a slit ˆ Consider a plane wave (complex amplitude E 0 ) to screen of arriving from the left at slit of width a observation We use Huygens principle and consider the radiation field consisting of wavelets from tiny areas of size ∆y . We observe under an angle θ from a “very far distance”. We call the complex electric wave vector of the first wavelet ˆ . E1 ∆δ ∆y sin θ The next wavelet is: ˆ ⋅ i with ∆δ = 2 π E1 e λ δ a ⋅sin θ And the last wavelet: ˆ ⋅ i N with δ= 2 π E1 e N λ 2 ∆δ δ 2 ∝ˆˆˆ =++in ++ ˆ i N The intensity at the screen is IEsum E1KK Ee 1 Ee 1 ∆y λ The amplitude of each wavelet is E ˆ = E ˆ = E ˆ ∆ δ 1a 0 0 2π a sin θ CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 7 Diffraction from a slit Intensity at the screen: 2 2 λ 2 ∆δ iδ IE∝ˆ = E ˆ ∆++++δ ()1 KK eein N sum 2πa sin θ 0 δ= δ 2 2 N 2 λδ λ δ 2 ⇒ Eedˆi δ = − Eie ˆ ()i N − 1 πθ0 ∫ πθ 0 2sinaδ =0 2sin a λ2 λ 2 iδ∗ − i δ I∝ EeEeˆ()()N −−=1 ˆ N 1 21cos E 2 () −=δ 2πθa sin0 0 2 πθ a sin 0 N π θ 2 asin 2 sin λ δ λ π θ =2 2 N = 2 ∝ 2 asin 4 E0 sin E0 sinc 2sinπa θ 2 πasin θ 2 λ λ Can be interpreted as a Fourier transform of the transmission function of the slit (note δ ≈ 2πyθ/λ is a linear function of y): δ= δ = N iδ y y 2 2πθ+∞ 2 πθ e iy iy dδ∝ eλ dy = τ() ye λ dyFT = () τ () y ∫θ ∫ ∫ slit δ = = −∞ 0 y y 1 CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 8 Diffraction from two narrow slits Makes it simple to calculate more complicated slit systems: e.g. Young’s double slit experiment (1801) τ Fourier transform of two delta functions at ±a/2: 2δ +∞ 2πθ a ai y πθλ− πθλ π a θ δy++− δ y edyeλ =+ia/ e ia / = 2cos ∫ λ −∞ 1444244432 2 τ 2δ θ∝ () τ 2 I() FT2δ () y 2 πθa 2 πθ a ∝cos =1 1 + cos : λ 2 λ CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 9 Diffraction from two real slits We can even take into account the finite width of the slits: τ= τ′ − ⋅ τ ′ ′ realistic()y∫ 2δ ( yy ) slit () ydy The Fourier transform of such a convolution integral is just the product of the Fourier transforms: θτ∝() 2 = ττ ⋅ 2 I() FTrealistic () y FT ()():2δ FT slit Note 1: “diffraction from two slits” (or of a finite number of separated waves) is mostly called “ interference ”. Interference from a continuum of waves is called “diffraction ”. There is no fundamental difference ! Note 2: Due to interference of two waves, there are suddenly locations of permanently ZERO intensity (energy density) where each individual wave did generate intensity. Energy density is re-distributed in space due to interference ! CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 10 Far field condition We have assumed a plane wave arriving at the slits. Typically realized by a point source in very far distance L. How far is “far”? There should be no significant phase difference of the wave between the two slits (or the illuminated object) Compare the optical path lengths ! a2 L− L = << λ 1 2 8L Point source a2 L >> distance should be 8λ The same condition holds for the distance from object to observation screen ! Fraunhofer diffraction Otherwise: Fresnel diffraction (no fun) 11 CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH transverse coherence What matters for interference is the superposition of (two) e.m. waves. So far we assumed they both come from the same source. This is not realistic. Let’s now drop this assumption but let’s still consider monochromatic waves. iδ i δ =+=1 + 2 (Let’s assume A 1 = A 2) E E121 E Ae Ae 1 Intensity: 2 2 ? ∝ =+()δ − δ I E2 A 1 1 cos( 2 1 ) period =() + ∆ δ ⇒ I I 0 1 cos asin θ ∆=δ2 π +const ∝⋅+ a x const λ ? ? ? Such radiation from slits is called transversely coherent CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbachsely, Univ HH 12 transverse coherence =( + ∆ δ ) I I 0 1 cos Moving along the screen, the cos ∆δ - term oscillates between +1 and -1 (see page 9) The interference contrast (=“visibility”) is then V=1: I− I V ≡max min →1 (perfect coherence and A =A ) + 1 2 Imax I min 2πa θ 2 π c Phase difference ∆δ can be expressed as time delay, e.g.: ∆=δ = τωτ = λ λ 0 Imagine, the two fields E1 and E2 do NOT stem from the same point source. We can still calculate the intensity on the screen according to p.9, but the phase difference on the screen does NOT only stem from the time delay τ (due to the observation angle), but there may be a further time difference τ’ between E1 and E2 : ∆δ ωτ′ ωττ+ ′ =i i0 = i 0 ( ) E2 Eee 1 Ee 1 E() tE⋅∗ ( t − τ ) O,1 O ,2 T ≡ γc τ 12 (a , ) normalized complex correlation function 2⋅ 2 EO,1 E O ,2 We consider intensities need to average over osc. period CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 13 transverse coherence E() tE⋅∗ ( t − τ ) O,1 O ,2 ≡ γc τ 12 (a , ) 2 2 normalized complex correlation function E⋅ E 2πa θ a θ O,1 O 2 - depends on observation angle through τ = = λω 0 c In our simple case A 1 = A 2: =( + ∆δ) +ℜ γc =( + γ ) II01 cos⇒ I 0( 1 12) I 0 1 12 ω∗ − ωττ +′ − it0 it 0 ( ) Ae1 Ae 1 −ω τ′ − τ Indeed: γc τ = = i 0 ( ) 12 (a , ) 2 e A1 ω τ ∆δ γc τ 0 = 12 (a , ) ⇒ e e γ=ℜ γc =ℜ∆δ = ∆ δ 12 12 e cos γ c The visibility of interference is determined by: 12 =γ c = In this case (A 1 = A 2): V 12 1 q.e.d. CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 14 transverse coherence E() tE⋅∗ ( t − τ ) O,1 O ,2 ≡ γc τ 12 (a , ) 2 normalized complex correlation function ⋅ 2 EO,1 E O 2 ≠ If I 1 I 2 2 ω ωττ+′ − 2 ωττ′− − ωττ ′ − ∝=+i0 t i 0 () t =++2 2 i0 ()() + i 0 Itotal E sum Ae1 Ae 2 AAAAe 1212 ( e ) =++()ωττ′ − + + ℜ γ c ⇒ IIIIItotal 12 12cos 0 ( ) ⇒ IIII 12 1212 I− I 2 I I V ≡max min =1 2 γc ≡ γ eff + + 12 12 Imax I min II 1 2 CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 15 transverse coherence ∗ 2 E( y ,0)⋅ E ( y ,0) dy dy This is a single number describing the entire beam ς ≡ ∫ 11 22 12 2 from slit (object), independent of angle of observation. ()E( y ,0) dy ∫ 1 1 1 ς →1 for perfectly coherent radiation. Example from FLASH FEL: From: A. Singer, et. al: Opt.Express 20, No.16 (2012) ς = ± x 0.59 0.1 ς = ± y 0.72 0.08 CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 16 Transverse coherence S. Reiche Z=25 m Z=37.5 m Z=50 m Z=62.5 m Z=75 m Z=87.5 m m Single mode dominates close to 100% transverse coherence CAS on FELs and ERLs, Hamburg Jörg Rossbach, Univ HH 17 2016 impact of focusing (needed for most experiments) CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 18 transverse coherence Why are the phases in 1 and 2 uncorrelated? Probably because the source is extended ! Consider a ray arriving at double slit at an angle ϕ and with intensity I(ϕ ) It contributes a phase difference π ϕ to double slit of: ∆δ = 2 a ϕ λ The averaged phase difference between the ω∗ − ωττ +′ − it0 it 0 ( ) Ae1 Ae 1 −ω τ′ − τ γc τ = = i 0 ( ) extended source to the double slit is: 12 (a , ) 2 e A1 +∞ 2πa ϕ 1−i I (ϕ ) a a Van Zitter-Zernicke-Theorem: IedFT(ϕ ) λ ϕ = ≡ I⇒ VI= Visibility of interference pattern corresponds to ∫ λ λ Fourier Transform of source distribution function Itotal −∞ I total CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 19 temporal coherence 2 2 −π t − π t ()∆τ 2 πν ()∆ τ 2 =i2 0 t ℜ = πν EtEe( )0 e ; EtEe( )0 cos(2 0 t ) ν− ν 2 −π (0 ) −∆−πτνν()()22 ∆ ν 2 FT( E ( t )) ∝ e(0 ) = e Phase information will be lost after longitudinal coherence time: τ ≈ 1 c ∆ν CAS on FELs and ERLs, Hamburg 2016 Jörg Rossbach, Univ HH 20 .