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PC20312 Wave Optics Section 3: Interference
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Interference fringes I 1 + I 2 Image adapted from Wikipedia
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Temporal coherence Phase relationship changes over a characteristic time Coherence time: Image adapted from Wikipedia
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Spatial coherence Wave with infinite temporal and spatial coherence Wave with infinite temporal coherence but finite spatial coherence Wave with finite temporal and spatial coherence A pinhole isolates part of the wavefront and thus increases spatial coherence. Coherence length is unaffected. Images adapted from Wikipedia
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Types of interference Wavefront division e.g. Young’s slits Amplitude division e.g. Michelson interferometer
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Thomas Young Thomas Young (1773-1829) “The Last Man Who Knew Everything “ Learned 13 languages by age 14 Comparative study of 400 languages Translated the Rosetta stone PhD in physics & medical doctor Young’s slits Young’s modulus Founded physiological optics: colour vision astigmatism accommodation of the eye Seminal work on haemodynamics Secretary to the Board of Longitude Superintendent of the HM Nautical Almanac Office. Image from Wikipedia
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Young’s slits 1 Poor spatial coherence Good spatial coherence Single slit isolates part of wavefront Double slits act as two coherent sources To distant screen
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Young’s slits 1 Young’s original diagram presented to Royal Society in 1803 Image from Wikipedia http://www.acoustics.salford.ac.uk/feschools/waves/diffract3.htm
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Young’s slits 3 a y r2r2 r1r1 rr s s >> a
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Lloyd’s mirror ii y r1r1 l1l1 l2l2 Phase change on reflection source image of source r 2 = l 1 +l 2 tt Rev. Humphrey Lloyd (1800-1881) Trinity College Dublin
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Multiple slits S0S0 S3S3 S4S4 S5S5 S6S6 S1S1 S2S2 a rr 2r2r 3r3r s>>a P
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Interference pattern for multiple slits
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Michelson Interferometer Albert Abraham Michelson (1852-1931) d1d1 d2d2 beamsplitter Mirror, M 1 Mirror, M 2 compensator plate lens screen light source d = 2(d 1 - d 2 ) Image from Wikipedia
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The compensator plate Without compensator: Unequal paths thru glass path length diff. = f( ) With compensator: Equal paths thru glass path length diff. f( ) Rays to M 1 pass thru BS once Rays to M 2 pass thru BS three times NB n glass = f( )
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Equivalent diagram for Michelson interferometer source plane M 1 plane M 2 plane d d cos( ) S S1S1 S2S2 Images of S in M 1 and M 2 lens f focal plane
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Fringe patterns Sodium lamp Images from http://hyperphysics.phy-astr.gsu.edu/hbase/phyopt/michel.html#c1 White light
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Fourier Transform Spectroscopy d1d1 d2d2 beamsplitter compensator plate lens detector Movable mirror d I(d) monochromatic d I(d) polychromatic
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Thin films ntnt nini nini B D C A s source lens ii tt A C D ii ii A C B s tt tt
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Thin film applications Dichroic mirrors – high reflectivity for narrow bandwidth only Anti-reflection coatings – reduces glare from lenses Images from Wikipedia
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Thin films in nature Oil on water – oil layer thickness varies giving a rainbow effect in white light Soap bubbles – thickness and angle of film varies to give rainbow The ‘Tapetum lucidum’ is found behind the retina of many animals (not humans) – it enhances night vision The tapetum lucidium in a calf’s eye Images from Wikipedia and Google Image
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Multibeam interference ErEr s source E t0 E t1 E t3 E t2 E t5 E t4 E r0 E r1 E r3 E r2 E r5 E r4 E r6 lens EtEt
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Stokes’ relations Sir George Gabriel Stokes (1819-1903) r 2 E+ttE E rE tE E rE tE rE tE rtE+trE A) B) C) B) is time-reverse of A) Comparing B) and C): r 2 + tt=1 r = -r Images from Wikipedia
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The Airy function Sir George Biddell Airy (1801-1892) Finesse, F = Free Spectral Range, Resolution, Image from Wikipedia
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Fabry-Pérot Etalons 1 Potrait images from http://www-obs.cnrs-mrs.fr/tricent/astronomes/fabry.htm &Wikipediahttp://www-obs.cnrs-mrs.fr/tricent/astronomes/fabry.htm Charles Fabry (1867-1945) Alfred Pérot (1863-1925) s r source lens f 2 highly reflecting parallel surfaces Outer surfaces are non-parallel
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Images from Google imageData from D. Binks PhD thesis Fabry-Pérot Etalons 2
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