Diffraction Gratings and Resolution Flashcards

1
Q

what is a diffraction grating

A

a slab with a periodic modulation on one of its surfaces

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2
Q

what are the three types of diffraction grating

A

transmission, reflection or phase

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3
Q

How do diffraction gratings let us measure spectra

A

they diffract different wavelengths in different directions

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4
Q

What is the significance that the modulation of the transmission from a diffraction grating is periodic

A

we can use a fourier series for it
A(x0,y0)=A0+A1cos( 2πœ‹π‘₯0/π‘Ž) + 𝐴2cos( 4πœ‹π‘₯0/π‘Ž) + 𝐴3 cos(6πœ‹π‘₯0/π‘Ž ) +… (only the x integral)

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5
Q

What is the wavelength dependence at order zero diffraction

A

none

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6
Q

what happens to different wavelengths of light at the +1 diffraction order

A

because x1 depends on wavelength, the wavelengths are separated x1=zlambda/a
z=distance from grating to screen
a = grating separation

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7
Q

In diffraction, the longer the wavelength

A

the larger its diffraction angle in nonzero orders

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8
Q

What is the transmission diffraction grating equation

A

π‘Ž (sin πœƒ βˆ’ sin πœƒπ‘–) = π‘šπœ†

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9
Q

How do we understand a transmission diffraction grating from fourier arguments

A

it is a convolution of a single slit with a comb function so a spectrum is a series of delta functions for each incident wavelength

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10
Q

Describe a blazed diffraction grating

A
  • tilting the facets of the grating so that the desired diffraction order coincides with the specular reflection from the facets, grating efficiency can be increased
  • while both diffracted beams would satisfy the grating equation, one is more intense than the other
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11
Q

what does specular mean

A

angle of incidence = angle of reflection

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12
Q

What happens if two diffraction gratings are superimposed perpendicularly

A

they form a 2d periodic array of apertures
the observed diffraction pattern isn’t the sum or the product of the individual gratings, the separate patterns repeat to form a 2d array

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13
Q

what are laguerre-gaussian modes

A

forked patterns due to phase dislocation in spiral phase fronts - donut beams

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14
Q

What is the total intensity for N randomly-distributed apertures

A

N times the intensity due to a single aperture

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15
Q

What will the diffraction pattern be of randomly places indentical holes

A

the gross features of the pattern will reveal the shape of the holes

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16
Q

What is Babinet’s Principle

A

The diffraction pattern of an array of holes is the same as that of its opposite

17
Q

What is the tendancy of diffraction to expand the smallest structure into the largest pattern key for

A

x-ray crystallography to diffract rays off atomic nuclei and reveal the crystal molecular structure

18
Q

explain particle detection and measurement by diffraction

A

a flow of particles passes through a laser beam
by the fraunhofer diffraction of the laser beam, a cross section of the diffraction ring pattern is captured using a photodiode array

19
Q

Describe how moon coronas form

A

moonlight passes through clouds, and diffracts when it passes between water droplets in the atmosphere - produces a coloured ring structure

20
Q

what is the ultimate limit on image quality

A

the spreading out of light around each point in an image

21
Q

As we bring 2 point sources closer and closer, eventually they will overlap - what is the rayleigh criterion

A

it tells us if we have resolvable images
the sources are just resolved when the centre of one airy pattern falls on the first minimum of the other airy pattern

22
Q

what is the minimum resolvable angular separation of two objects

A

Ξ”πœƒ = 1.22 πœ†/D

23
Q

if f is the focal length of the lens and D is the diameter of the aperture, what is the radius of the airy disc

A

1.22 fπœ†/𝐷

24
Q

what are two ways to better resolve an image

A

decrease the aperture diameter or increase the viewing distance

25
Q

How can diffraction effects be minimised

A

keeping the aperture sizes large comared to the wavelengths

26
Q

Why do astronomical telescopes have such huge apertures

A

to limit diffraction effects

27
Q

Why do we replace the objective lens in large reflecting telescopes with a concave mirror

A

because mirrors are free from chromatic and spherical aberrations and they are easier to correct than a lens

28
Q

How is modern scanning near-field microscopy able to avoid the rayleigh limit

A

by sampling the evanescent wave transmitted by the sample through a narrow aperture, the resolution can get to a hundredth of a wavelength

29
Q

what does sted stand for

A

stimulated emission depletion microscopy

30
Q

How does sted work to improve the resolution over a regular microscope

A

it adds a second laser beam to the scanning process of the image compared to confocal imaging
the normal pulse is followed by a donut shaped pulse (laguerre gaussian beam) which bleaches molecules back to ground state, only molecules in the hole of the donut can emit fluorescence, limiting the point spread function and improving the resolution

31
Q

What is the abbe limit

A

NA = nsintheta

32
Q

what is the dispersion of a diffraction grating

A

π‘‘πœƒπ‘š/π‘‘πœ† = π‘š/π‘Ž π‘π‘œπ‘ πœƒ

33
Q

what is the diffraction grating spectrometer resolution

A

π›Ώπœ† = 4πœ†/π‘šπœ‹π‘ where N = no. grating lines = a/d

34
Q

In a 2 slit experiment, if the spatial coherence length is less than the slit separation, what will happen

A

the relative phase of light from each slit will vary randomly and fine scale fringes wash out so only a one slit pattern will be observed

35
Q

What happens if the slit width is period/N

A

the minima of the slit diffraction correspond to the maxima N, 2N, 3N, of the grating diffraction resulting in missing maxima