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Today Ch.36 (Diffraction) Next week, Dec.6, Review This week off. hours: Th: 2:00-3:15pm; F: 1:00-3:00pm Next week off. hours: Tu:2-3:15pm,W:1-3pm,Th:1-3pm Webct homework is due by Dec.12. Check your Midterm Exams Grades on elearning! Final Exam: (Ch.21-25, 27-29, 32,33,35,36) Secs.511-515: December 9, Friday: 12:30-2:30 pm Secs.521-525, 528: December 12,

Today Ch.36 (Diffraction) Next week, Dec.6, Review This week off. hours: Th: 2:00-3:15pm; F: 1:00-3:00pm Next week off. hours: Tu:2-3:15pm,W:1-3pm,Th:1-3pm

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Page 1: Today Ch.36 (Diffraction) Next week, Dec.6, Review This week off. hours: Th: 2:00-3:15pm; F: 1:00-3:00pm Next week off. hours: Tu:2-3:15pm,W:1-3pm,Th:1-3pm

Today Ch.36 (Diffraction) Next week, Dec.6, ReviewThis week off. hours: Th: 2:00-3:15pm; F: 1:00-3:00pmNext week off. hours:Tu:2-3:15pm,W:1-3pm,Th:1-3pmWebct homework is due by Dec.12.Check your Midterm Exams Grades on elearning!

Final Exam: (Ch.21-25, 27-29, 32,33,35,36)

Secs.511-515: December 9, Friday: 12:30-2:30 pmSecs.521-525, 528: December 12, Monday, 8-10 am

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Lecture 24 (Ch. 36)

Diffraction1. Huygen’s principle, bending of the rays2. Fraunhofer’s diffraction3. Single slit4.Two slits with a finite width5. Resolution of the lens6. Diffraction grating7.Spectroscopy8. x-ray diffraction9. e diffraction

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Huygen’s principle and bending of the rays

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1788 – 1827

Augustin-Jean Fresnel

Joseph von Fraunhofer (1787 – 1826)

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Single slit diffraction

How to describe the real picture?

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Single slit diffraction

ma

xy

x

ysmallfor

axistoparallelraysallm

mNBmma

asta

m

:min,tansin;

)max!00(

!0:,...)2,1(sin:min

sinmin)1(2

sin2

r

sinar

Page 7: Today Ch.36 (Diffraction) Next week, Dec.6, Review This week off. hours: Th: 2:00-3:15pm; F: 1:00-3:00pm Next week off. hours: Tu:2-3:15pm,W:1-3pm,Th:1-3pm
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Intensity distribution

1st max 0

sin

2ark

)12(:max

)0(sin2:min

}

2

2sin

{,

2

2sin

,,2

sin2

200

0

m

mmam

IIEER

ER

E

R=

E

21st min: 1st max: 3

E

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)0(sin2:min;}

2

2sin

{ 20 mmamII

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a

1

Narrowing of the first fringe with increase of the slit width

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Circular hole diffraction

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The photographs of four very small sources of light taken made with a circular aperture in front of the lens

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)7.4(650:

)7.0(780:

gigabytesnmDVD

gigabytesnmCD

Rayleigh’s criterion for resolution of two point objects: Two objects are barely resolved if the center of one diffraction pattern coincides with the first minimum if the other.

L

DLS

22.1sin

For a microscop

1842 – 1919John William Strutt, 3rd Baron Rayleigh

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Hubble vs Arecibo

Hubble: D=2.4m, nm500Arecibo: D=300m, cm75

kmDkmS

kmss

myearcly

CentaurystarnearestlyL

sizecraterkmSmS

moonthetomL

DLS

JupiterH

AH

57

1378

8

10,10

101010311

),(4

)(1000,77

)(108.3

22.1sin

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Giant Magellan Telescope (2016)

D1=8.5m, Deq=24m nm500

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Interferometry: Arrays of telescopes

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Two slits with a finite width

2cos}

2

2sin

{4

sin,

2

2sin

)(:

sin,2

cos)(2:

220

00

0

II

kaEEfactorDifraction

kdEEfactornceInterefere

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Diffraction grating

mdm sin2:max

!02

0 ININEE otot

tE0

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N-1 minima

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With increase of N principal maxima becomes narrower

and their amplitude grows as 2N

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Grating spectroscopySpectrum of sunlight produced by a diffraction grating has dark absorption lines due to absorption of the corresponding wavelength by the solar atmosphere. It allows to find out a chemical composition of the solar atmosphere.

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x-ray diffraction

Wilhelm Röntgen (1845 – 1923)The 1st Nobel Prize,1901

nm101.0~

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Bragg condition

nd sin2

An x-ray scattering pattern of DNA recorded by Rosalind Franklin led Watson and Crick to discovery of the DNA double helix structure

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Louis de Broglie (1892 – 1987)

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Electromagnetically induced transparency (EIT)

Two undistinguishable absorption passes for light result in cancellation of absorption (transparency).An electron has the wave property. It may be in a superposition of states 1 and 1’. Monohromatic light with a frequency resonant either to one or another atomic transition is absorbed.Bichromatic light containing two resonant frequencies goes through.

11’

1 2

O.K., Y.I.Khanin, JETP, 1986; O.K., P. Mandel, Phys. Rev. A. 1990. theory S.E. Harris, PRL, 1991. experiment

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Electromagnetically induced transparency (EIT)Two undistinguishable absorption passes for light result in cancellation of absorption (transparency).An electron has the wave property. It may be in a superposition of states 1 and 1’. A circular polarized light interacts only with 1-2 (or 1’-2) state and absorbed. A linear polarized light interacts with both 1-2 and 1-2’ states and goes through the medium without absorption. To make medium transparent for light with given circular polarization send through the medium simultaneously light with another circular polarization.

The same is true for two beams of different frequenciesWhen the frequency difference coincides with the frequency of the atomic transition 1-1’.

1

1’

2

1

1’

1 2

O.K., Y.I.Khanin, JETP, 1986; O.K., P. Mandel, Phys. Rev. A. 1990. theory S.E. Harris, PRL, 1991. experiment

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