CH8: coherence theory Flashcards

1
Q

Temporal coherence

A

fields offset in time
E(r,t) E(t,t-tau)

Mich int is sensitive ot spectral content of wave

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2
Q

Spatial coherence

A

fields at difference spatial locations

E(r,t) E(r+delta r,t)

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3
Q

HOw do we detect coherence effects

A

Interference
Temportal, michaelson interefeormeter
Spatial - yongs two slit interferometer

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4
Q

If high degree of coherence then we see

A

HIGH COHERENCE

  • The light consistently interferes either constructively or destructively at the detection point,
  • Time avg intensity signal shows the interference
  • ocilllates wihtou diminisihing as time delay or spatial something is introduced/adjusted

LOW COHERENCE
-NO INTERFERENCE SEEN

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5
Q

What dspecial about PW and coherence

A

MONOCHROMATIC PW is temporatlly coherence (i.e. in miachealson int.)

-any change of tau not affect intereference pattern at detector,
-PW must have 1 frequence, 1 wavelngth 1 k,
a continous band of freqyuencies we get a degree of incoherenceincoherence

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6
Q

What makes a light source temporally incoherent

A

when it has a continous band of frequencies (i.e. not a monochromatic anymore)
we get fast fringe cisibibility diminishes as a delay is introduced in the michealson int

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7
Q

Fluence

A

Sig(tau)
time integrated intensity
units” energy per area
integral of Itot(t,tau) (over dt from -inf,inf)

sort of like total energy, not useful for CW sourses of light

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8
Q

Does the mich int depend on phase

A

no
The signal out of the int does not dep on E(w)
it depends only on the amount of light associated wiht each frequency thorgh I(w)

since the degree of coherence function only has I(w) in

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9
Q

D.o.coherence functoion

A

gamma(Tau)

describes the oscillations in intensity at the detector as the mirror arm is moved

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10
Q

What happens for large Tau in temporal coherence

A

If not coherent (not monochormatic light)
then the oscillations die of as the diff freq get out of sync
some interfere dest, others constructively

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11
Q

Is narrow band light more coherent than boradband

A

Yes because there is less opportunity for freq to get out of sunc
for larger Tau the osciallations will still die off

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12
Q

Define coherence time

A

The amount of delay needed to cause gamma(tau) to quit oscillating (amplitude approach 0)
arb. vanishsing pt givin in tau_c formula

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13
Q

Define fringe visibility

A

depends only on freq of light not whether these freq are organised into a long or very short pulse

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14
Q

How can we determine pulse length by looking at intereference pattern on mich. in

A

We look at the detectorl signal - focus on getting coherence time since

If long pulse -> T_c is long
since T_c = sqrt (2pi) T
where T is a measure of the length of a gaussian pulse

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15
Q

Diff between youhng and michealson

A

two beams of light travel different paths and then interfere

Mich: one path delay wrt ot he other so that temporal effects studied
Young: two laterally separate points of the same wave are compared as they are sent through two slits

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16
Q

If mich is sensitive to ___ then young is sensitive to __________

A

mich: spectral content of the light
young: spatial extent of the light source illuminating the two slits

17
Q

How did oyoung use to measure star width

A

wide angular width of stars -» poor finge visibilitit -> very wide spatial extent

18
Q

Partial spatial coherence

A

Collection of point sources distrib over a finite lateral extent, only slighlty diminished finged pattern that is washed out.

We assume the poiunt sources vary only in the y dimension

19
Q

The more extended the source the mroe___

A

Wahsed out the fringe pattern.

less contrast in fringe patten

20
Q

When are the approximations valid for youngs

A

We taylor expanded d1(y) and d2(y) and these are validwhen
D»y, D»h
i.e. only true in the middle of the finger pattern, only true when the distance between the screena dn the slit&raquo_space; the slit width

21
Q

Tau in temporal is what in spatial

A

h

slit separation

22
Q

What is the stochastic assumption

A

Used in derivation of Itot(h) in young’s two slit exp

Assume that the phase of the emission (phi(yj)) varies in time independently at every point on the source

23
Q

Where is the stochastic assumption valoid/not

A

Valid in stars, glowing filaments spontaneous emission from excited gas or plasma, not coherent sources (coherent in the tyoic sense not really spatial or temporally here)
Not valid: lasers which are coherent sources

24
Q

simplyfying arpporximation reuslt of tay series

A

d1(y) - d2(y) approx = hy/D

25
Q

In the degree of coherence function fro spatial we have

A

gamma(h)

depeneding on I(y’) wjocj jas imots pf omtemsotu [er ;emgtj pf tje spirce

26
Q

in the defree of coh. func spatial what does the exp(-ikhy/D) define

A

The locations ofthe periodic fringes on the screen

depth of such fringes are dep on the rest pf the docoh. function

27
Q

wehn h increases what happens to gamma(h)

A

amplitude of Gamma(h) diminises until the intensity becomes uniform

larger slit separation -> poorer spatial coherence

28
Q

When do we get very good spatial coherence

A

|When gamma(h)|=1

the two slits have very small spearation h

29
Q

What is hc

A

Analogous with Tc

it is the slit spearation h that will cause th finge patterns to totally wash our (here bcome totally uniform)