Introduction Particle Properties of Light

Introduction Particle Properties of Light Introduction Particle Properties of Light

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Introduction Until the early 20 th century physicists used to explain the phenomena in the physical world around them using theories such a mechanics, electromagnetism, thermodynamics and statistical physics that are now known as classical theories. At the turn of the 19 th century more and more experiments did show effects that could not be explained by these classical theories. This indicated a need for a new theory that we now know as quantum mechanics. Here we discuss a set of early experiments indicating the need for a new theory: particle properties of light • photoelectric effect, Compton effect, x-ray generation emission of light from atoms • discrete line spectra - energy levels, Franck-Hertz experiment wave properties of particles Particle Properties of Light • Until the beginning of the 1900’s all known properties of light (and in fact any type of electromagnetic radiation) were thought to only wave-like. • In the early years of the 20 th century experimental observations did hint at the fact that light might also posses particle properties. I.e. that any radiation transports energy in quanta of energy that we now are used to call photons. • These observations were important in the early days of the developments of quantum mechanics. Now quantum mechanics is one of the best tested theories describing the physical world on the microscopic scale. • The knowledge of quantum mechanics is crucial for the understanding of basic physical phenomena on the microscopic (but increasingly also on the mesoscopic and macroscopic scale). • Here we discuss a number of phenomena and experiments in which the particle properties of light become apparent.

<strong>Introduction</strong><br />

Until the early 20 th century physicists used to explain the phenomena in the physical<br />

world around them using theories such a mechanics, electromagnetism,<br />

thermodynamics and statistical physics that are now known as classical theories.<br />

At the turn <strong>of</strong> the 19 th century more and more experiments did show effects that could<br />

not be explained by these classical theories. This indicated a need for a new theory<br />

that we now know as quantum mechanics.<br />

Here we discuss a set <strong>of</strong> early experiments indicating the need for a new theory:<br />

particle properties <strong>of</strong> light<br />

• photoelectric effect, Compton effect, x-ray generation<br />

emission <strong>of</strong> light from atoms<br />

• discrete line spectra - energy levels, Franck-Hertz experiment<br />

wave properties <strong>of</strong> particles<br />

<strong>Particle</strong> <strong>Properties</strong> <strong>of</strong> <strong>Light</strong><br />

• Until the beginning <strong>of</strong> the 1900’s all known properties <strong>of</strong> light (and in fact any<br />

type <strong>of</strong> electromagnetic radiation) were thought to only wave-like.<br />

• In the early years <strong>of</strong> the 20 th century experimental observations did hint at the<br />

fact that light might also posses particle properties. I.e. that any radiation<br />

transports energy in quanta <strong>of</strong> energy that we now are used to call photons.<br />

• These observations were important in the early days <strong>of</strong> the developments <strong>of</strong><br />

quantum mechanics. Now quantum mechanics is one <strong>of</strong> the best tested theories<br />

describing the physical world on the microscopic scale.<br />

• The knowledge <strong>of</strong> quantum mechanics is crucial for the understanding <strong>of</strong> basic<br />

physical phenomena on the microscopic (but increasingly also on the mesoscopic<br />

and macroscopic scale).<br />

• Here we discuss a number <strong>of</strong> phenomena and experiments in which the particle<br />

properties <strong>of</strong> light become apparent.


Photoelectric Effect<br />

• light <strong>of</strong> sufficiently high frequency (ultraviolet: λ ~ 1 – 400 nm) impinging on<br />

an Alkali metal surface leads to emission <strong>of</strong> electrons<br />

Sodium (Na)<br />

Observation:<br />

• Electrons are emitted immediately (a few nanoseconds (10-9 s)) after light is<br />

switched on .<br />

Time for emission: try to explain it classically<br />

How to analyze effect in more detail? Measure the energy distribution <strong>of</strong> electrons.


Photoelectric Effect<br />

• light <strong>of</strong> sufficiently high frequency (ultraviolet: λ ~ 1 – 400 nm) impinging on<br />

an Alkali metal surface leads to emission <strong>of</strong> electrons<br />

Sodium (Na)<br />

Observation:<br />

• Electrons are emitted immediately (a few nanoseconds (10-9 s)) after light is<br />

switched on .<br />

Photo Effect: Measurement <strong>of</strong> Photo Current<br />

• dependence <strong>of</strong> stopping potential U 0<br />

on<br />

frequency <strong>of</strong> light<br />

• dependence <strong>of</strong><br />

stopping potential<br />

U 0<br />

on intensity <strong>of</strong><br />

light<br />

Observations:<br />

• energy distribution is independent <strong>of</strong> intensity <strong>of</strong> light<br />

• intensity <strong>of</strong> light only changes the number <strong>of</strong> emitted electrons<br />

• maximum kinetic energy <strong>of</strong> measured electrons depends only <strong>of</strong> frequency <strong>of</strong> light


Maximum Kinetic Energy <strong>of</strong> Photoelectron<br />

• maximum photo electron<br />

energy in dependence on<br />

frequency <strong>of</strong> light<br />

• threshold frequency for emission <strong>of</strong> electrons ν 0<br />

• dependence <strong>of</strong> maximum kinetic energy <strong>of</strong> electrons is linear in frequency ν <strong>of</strong> light<br />

• the proportionality constant is Planck’s constant h = 6.63 10 -34 Js<br />

• the proportionality constant is independent <strong>of</strong> the metal used for the experiment<br />

Explanation <strong>of</strong> Photoelectric effect<br />

• note: Electrons can also be emitted from metal surface by heating up the metal, e.g.<br />

by running a large current through it. This process is called thermal emission. It is<br />

used, for example, in vacuum tubes for generating free electrons. In this case the heat<br />

(thermal energy) is providing the energy to extract the electron from the metal. The<br />

value <strong>of</strong> the work function can be determined this way as well and usually agrees<br />

well with the one that can be determined from the photoelectric effect.<br />

• exercise: Calculate the maximum kinetic energy <strong>of</strong> electrons emitted by the photo<br />

electric effect from a Potassium (Ka) metal surface with work function <strong>of</strong> 2.0 eV by<br />

ultraviolet photons with wavelength 350 nm.


Nobel Prize in Physics (1906): Einstein<br />

"for his services to Theoretical Physics, and especially for his<br />

discovery <strong>of</strong> the law <strong>of</strong> the photoelectric effect"<br />

• Einstein’s explanation for the<br />

photoelectric effect: <strong>Light</strong> is composed <strong>of</strong><br />

individual quanta <strong>of</strong> energy. We call<br />

those quanta photons.<br />

• The energy <strong>of</strong> a photon is given by<br />

Albert Einstein<br />

Germany and Switzerland<br />

Kaiser-Wilhelm-Institut (now Max-<br />

Planck-Institut) für Physik<br />

Berlin, Germany<br />

b. 1879<br />

(in Ulm, Germany)<br />

d. 1955<br />

• ν is the photon frequency<br />

• h is Planck’s constant<br />

X-Rays<br />

• Generation <strong>of</strong> electromagnetic radiation by electrons impinging on a metal surface<br />

(inverse photo effect), i.e. conversion <strong>of</strong> kinetic energy <strong>of</strong> electrons to photons.<br />

Discovered by Wilhelm Rontgen (1895).<br />

schematic <strong>of</strong> an x-ray tube:<br />

• properties <strong>of</strong> X-rays:<br />

• propagates along straight lines (independent <strong>of</strong> magnetic or electric fields)<br />

• intensity increases with electron flux<br />

• faster electrons generate higher energy (more penetrating) X-rays<br />

• can expose photo sensitive materials<br />

• can generate phosphorescence or fluorescence light when interacting with hitting<br />

other materials


X-Ray Spectra<br />

Tungsten (W):<br />

Molybdenum (Mo):<br />

observations:<br />

• continuous spectrum generated by decelerated charges (Bremsstrahlung)<br />

• lower cut-<strong>of</strong>f wavelength λ (upper cut-<strong>of</strong>f frequency ν) is set by maximum electron<br />

energy<br />

• cut-<strong>of</strong>f is independent <strong>of</strong> material and only dependent on electron energy<br />

Minimum Wave Length <strong>of</strong> X-Rays<br />

• lower cut-<strong>of</strong>f wavelength λ min<br />

(upper cut-<strong>of</strong>f frequency ν max<br />

)<br />

• typical x-ray range <strong>of</strong> wave lengths: λ = 10 -11 m to 10 -8 m = 0.01 nm to 10 nm<br />

• exercise: Typical x-ray sources use electron energies <strong>of</strong> 50 keV. What is the<br />

corresponding minimum wave length or maximum frequency <strong>of</strong> emitted x-rays?


(The first ever) Nobel Prize in Physics (1901)<br />

"in recognition <strong>of</strong> the extraordinary services he has rendered by the discovery <strong>of</strong><br />

the remarkable rays subsequently named after him"<br />

Wilhelm Conrad Röntgen<br />

Germany<br />

Munich University<br />

Munich, Germany<br />

b. 1845<br />

d. 1923<br />

• The first x-ray image ever:<br />

The hand <strong>of</strong> Roentgen’s wife.<br />

X-Ray Diffraction<br />

• How to measure the wave length <strong>of</strong> x-rays?<br />

• Observe diffraction from a grating. For large diffraction angles to be observed<br />

period <strong>of</strong> diffraction grating needs to be comparable to wavelength <strong>of</strong> radiation<br />

(0.01 nm to 10 nm).<br />

• diffract x-rays in a solid state crystal in which atoms are spaced regularly on sub<br />

nanometer distances.<br />

e.g. a cubic crystal (NaCl)<br />

Bragg lattice planes:<br />

a i<br />

: lattice plane<br />

distances


Point Scattering <strong>of</strong> X-Rays<br />

• scattering <strong>of</strong> an X-ray from a point-like scattering object (a single<br />

atom for example)<br />

• scattered waves from point-like sources interfere<br />

• the interference is constructive only in special directions<br />

• Which are these special directions?<br />

Bragg Diffraction<br />

first Bragg condition:<br />

• consider two paths I and II with same incidence and reflection angle θ:<br />

second Bragg condition<br />

• criterion on difference <strong>of</strong> lengths for paths I and II for constructive interference:<br />

Only if both conditions are fulfilled scattered x-ray light is observed in that direction.


X-Ray Diffraction Measurement Apparatus<br />

• measure lattice plane distances with known wave lengths <strong>of</strong> x-rays<br />

• or measure x-ray wavelength with crystal with known lattice plane<br />

distances<br />

• exercise: Determine the lattice constant a <strong>of</strong> the NaCl cubic lattice from<br />

its density and molar mass.<br />

Nobel Prize in Physics (1915)<br />

"for their services in the analysis <strong>of</strong> crystal structure by means <strong>of</strong> X-rays"<br />

Sir William Henry Bragg<br />

1/2 <strong>of</strong> the prize<br />

United Kingdom<br />

London University<br />

London, United Kingdom<br />

b. 1862<br />

d. 1942<br />

William Lawrence Bragg<br />

1/2 <strong>of</strong> the prize<br />

United Kingdom<br />

Victoria University<br />

Manchester, United Kingdom<br />

b. 1890<br />

(in Adelaide, Australia)<br />

d. 1971


Compton Effect<br />

• quantum theory <strong>of</strong> light states that a photon behaves as a relativistic<br />

particle with zero rest mass<br />

• consider an x-ray photon colliding with a single electron at rest<br />

• energy and momentum conservation can be used to analyze the problem<br />

Momentum <strong>of</strong> a Photon<br />

Photons in vacuum (like any electromagnetic wave) propagate with the velocity <strong>of</strong><br />

light c ~ 3. 10 8 m/s.<br />

Thus they do behave like relativistic particles.<br />

energy <strong>of</strong> a relativistic particle:<br />

rest mass <strong>of</strong> photon:<br />

energy <strong>of</strong> a photon:<br />

resulting momentum <strong>of</strong> a photon:


Compton Effect Calculation<br />

find the difference in wavelength λ’– λ between the incident and the scattered photon<br />

before after after collision<br />

photon<br />

electron<br />

- along direction <strong>of</strong> incidence<br />

- perpendicular<br />

solve for electron momentum:<br />

the total electron energy after the<br />

collision is:<br />

kinetic energy<br />

rest energy<br />

Compton Effect Calculation<br />

(4) with (0) results in:<br />

equating (3) and (5) we find:<br />

with<br />

the result is:<br />

Compton wave length


Compton Effect Measurement Apparatus<br />

• The Compton effect can only be measured easily with x-rays because the Compton<br />

wavelength is small. Therefore the fractional change <strong>of</strong> the photon wavelength is<br />

smaller for larger wavelength.<br />

• Also the photons are scattered <strong>of</strong>f weakly bound electrons in a metal rather than<br />

free electrons.<br />

Compton Effect Spectra<br />

λ<br />

• forward scattered spectrum shows<br />

only peak at input wave length λ<br />

• at scattering angles φ > 0 a<br />

Compton peak appears at the scattered<br />

wavelength λ’<br />

λ’<br />

• at φ > 0 a peak remains at the<br />

incident wave length due to<br />

scattering from more strongly bound<br />

electrons (looks like higher effective<br />

mass <strong>of</strong> electron m 0<br />

*<br />

due to stronger<br />

binding to nucleus)<br />

• experiment to be demonstrated in<br />

class


Nobel Prize in Physics (1927)<br />

"for his discovery<br />

<strong>of</strong> the effect<br />

named after him"<br />

"for his method <strong>of</strong> making the paths <strong>of</strong><br />

electrically charged particles visible by<br />

condensation <strong>of</strong> vapour"<br />

• The observation <strong>of</strong> the Compton<br />

effect clearly demonstrates that<br />

photons carry a momentum and<br />

thus also confirms that light<br />

has particle properties.<br />

Arthur Holly Compton<br />

1/2 <strong>of</strong> the prize<br />

USA<br />

University <strong>of</strong> Chicago<br />

Chicago, IL, USA<br />

b. 1892<br />

d. 1962<br />

Charles Thomson Rees Wilson<br />

1/2 <strong>of</strong> the prize<br />

United Kingdom<br />

University <strong>of</strong> Cambridge<br />

Cambridge, United Kingdom<br />

b. 1869<br />

(in Glencorse, Scotland)<br />

d. 1959

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