lecture 10 light ii phys 420-spring 2006 dennis papadopoulos...

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LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos http://physics.berea.edu/~king/Teaching/ModPhys/QM/ Photoelectric/Photoelectric.html http://physics.berea.edu/~king/Teaching/ModPhys/QM/ Blackbody/BlackBody.html http://www.student.nada.kth.se/~f93-jhu/phys_sim/ compton/Compton.htm

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Page 1: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

LECTURE 10

LIGHT II

PHYS 420-SPRING 2006

Dennis Papadopoulos

http://physics.berea.edu/~king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html

http://physics.berea.edu/~king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

http://www.student.nada.kth.se/~f93-jhu/phys_sim/compton/Compton.htm

Page 2: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

• Hertz showed that light is an electromagnetic phenomenon, and that electromagnetic waves behave much like any other wave-- they can be reflected, refracted, diffracted and polarized.

• Heated solids emit a continuous spectrum of radiation whose intensity and spectral form depends only on their temperature (blackbody radiation)

• Planck realized that the emission is caused by electrons oscillating on the surface of the body and emitting radiation att the frequency of their oscillation (little antennas)

• However, unless energy is quantized, the radiation of a blackbody will continue to increase with frequency—a dilemma dubbed the ultraviolet catastrophe—forcing Planck to theorize that light comes in lumps and “oscillators” atomic walls must have quantized energy.

Page 3: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Black Body Radiation

Page 4: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

ATJe ),(

0

4Tdee vtotal

just a measure of the area

under the curve

Page 5: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

ENERGY PER UNIT VOLUME PER UNIT FREQUENCY(J/m3Hz) uT) orPOWER PER UNIT AREA PER UNIT FREQUENCY J T)

JT)=(c/4)u(,T)

u(,T)= (average Energy per mode)(number of modes per unit volume)

)/8)((),( 32 ckTTu

UV catastrophe. To save it average energy per mode <E> must be a function of .<E>= kT F(,T)

Page 6: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

]/[ kTExpE

Wien

hJ

kTExpE

Planck

sec106.6

1]/[

34

ENTuc

N

)(),(

8)(

3

2

Page 7: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Particles have identical physical properties…but can be

distinguished by following their(well defined) classical paths.

In equilibrium, the energy distribution of the particles will converge

to the most probable allowed.

In principle, there is no limit on the number of particles

occupying each state.

ASSUMPTIONSASSUMPTIONS

See Ch.10, section 10.1

]/[)( kTEAExpEP

Page 8: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Imagine 6 particles with 9 units of energy that can be distributed among nine states. The system has total energy 9E.

•If the particles are indistinguishable, we only care about how many particles are in each state, and there are 26 unique ways to distribute the energy among them—26 unique combinations.

Page 9: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

To find the average number of particles in each state

2211 pnpnn jjjaverage number

of particles in the jth energy level count the

number of particles in

each state for this

distribution

multiply by the number of permutations that can produce this distribution divided by the total number of permutation for all distributions

Page 10: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Energylevel

Averagenumber

0 2.143

1 1.484

2 0.989

3 0.629

4 0.378

5 0.210

6 0.105

7 0.045

8 0.015

9 0.003

Page 11: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

0

2

0

)(]/[

]/[

kTdEkTEEExp

kTdEkTEExp

Average Energy-Continuous case

0 00

)/()/1()(/)( kTdEkTEEExpkTdEEPdEEEPE

Average Energy – Discrete case

1]/[]/[

]/[

0

0

kTExp

kTnExp

kTnExpnE

hE

replace

n

n

Page 12: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-11, p. 78

Page 13: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-9, p. 74

Page 14: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-10, p. 75

Page 15: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

• Inconsistency in Planck’s thinking in that he

• Quantized the oscillators emitting radiation in the walls of the cavity

• Insisted that the cavity radiation was composed of classical waves

• Concluded that radiation must be composed of lumps ( quantas) consstent with the quantas emitted by the cavity walls

Page 16: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

The observation that electromagnetic waves could eject electrons from the surface of a metal was first made by Hertz.

A simple experiment can be designed to measure the energy and intensity of the electrons ejected.

•Light shines on a metal plate emitting electrons

•The voltage on a battery can be gradually turned up until the electric field just stop the electrons from reaching the collector plate, thereby giving a measure of the kinetic energy.

Page 17: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

•The energy in the light wave is spread out uniformly and continuously over the wavefront.

CIAtKmaxThe maximum kinetic energy of an ejected electron is therefore

timelight intensity

cross sectional area of atom

work function

absorption coefficient

which depends on the light intensity and the time over which it is exposed.

•The intensity of a light wave is proportional to the square of the amplitude of the electric field.

•The energy in the light wave is spread out uniformly and continuously over the wavefront.

…and therefore does not depend on frequency.

Page 18: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

•The number of photoelectrons ejected depended on the intensity (as expected) but their maximum kinetic energy did not!

•The maximum kinetic energy depended only on the frequency, the slope of the linear relationship between the energy and the frequency gives “Planck’s constant”, h.

•The electrons were ejected immediately after the light started shining—the electron instantaneously absorbed enough energy to escape-provided there was enough energy to overcome the binding energy or “work function”.

•Even a high intensity source of low frequency light cannot liberate electrons.

Page 19: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

We have to change our way of thinking about this picture:

Instead of continuous waves we have to

think of the energy as being localized in

quanta.

In the photoelectric effect, these discrete localized quanta of

energy, hv, are transferred entirely to

the electron

hvKmax

Page 20: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html
Page 21: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-16, p. 84

Page 22: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Table 3-1, p. 84

Page 23: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-17, p. 84

Kmax varies linearly with f

Page 24: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Part 2: Compton scattering: when you have a higher energy photon

Photoelectric effect- all of the incident photon’sEnergy is transferred to an electron, ejecting it.

Compton scattering-electron is ejected, but photon retains someenergy.

Pair-production-the photon’s energy is consumed to producean electron and a positron.

Page 25: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-18, p. 87

Page 26: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-19, p. 87

Page 27: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-23a, p. 91

Page 28: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-22a, p. 90

Page 29: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-23b, p. 91

Page 30: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-23, p. 91

Page 31: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Fig. 3-22b, p. 90

Page 32: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html
Page 33: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

The unshifted peak comes from tightly bound electrons

Contrast, classical scattering:

Electrons would shake with the frequency of the incident wave

The incident and scattered wavelengths would be the same

Page 34: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

Bragg spectroscopyBragg spectroscopy

,...3,2,1sin2 ndn

(a) Constructive interference occurs when:

(b) At other angles the waves do not interfere constructively

This is an important tool in crystallography as it is a sensitive measure of the spacing of the crystalline planes.

Page 35: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html
Page 36: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

…and the answer is…drumroll please…

If light, which was previously thought of as a wave, has characteristics of particles, could it be true that particles must also be thought of as waves in some contexts in

order to fully describe their behavior?

Light:

•Interferes like a wave

•Diffracts like a wave

•Can be polarized like a wave

•Scatters like a particle

Page 37: LECTURE 10 LIGHT II PHYS 420-SPRING 2006 Dennis Papadopoulos king/Teaching/ModPhys/QM/Photoelectric/Photoelectric.html king/Teaching/ModPhys/QM/Blackbody/BlackBody.html

If you are making choices from n objects, then on your first pick you have n choices. On your second pick, you have n-1 choices, n-2 for your third choice

and so forth. As illustrated before for 5 objects, the number of ways to pick from 5 objects is 5! .

Suppose you are going to pick a subset r out of the total number of objects n, like drawing 5 cards from a deck of 52. For the first pick, you have n choices,

then n-1 and so on down to n-r+1 for the last pick. The number of ways you can do it is:

rnPrn

nrnnnn

)!(

!)1)...(2)(1(