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18 Apr 2002 Physics 102 Lecture 9 1 Quantum Mechanics Physics 102 18 April 2002 Lecture 9 Planck Bohr Schroedinger Heisenberg From: http://www.th.physik.uni-frankfurt.de/~jr/portraits.html

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18 Apr 2002 Physics 102 Lecture 9 1

Quantum Mechanics

Physics 102

18 April 2002

Lecture 9

Planck Bohr Schroedinger HeisenbergFrom: http://www.th.physik.uni-frankfurt.de/~jr/portraits.html

18 Apr 2002 Physics 102 Lecture 9 2

Blackbody radiationRecall: a perfect blackbody absorbs and re-emits all

radiation that falls upon it.

All blackbodies at a given temperature emit the samepower in the same frequency band, i.e. they all have thesame characteristic spectrum.

The total power emitted increases like T4. As you mayrecall from last semester:

At the end of the 1800s, no one could predict the radiatedpower, Q, as a function of frequency.

Q T AtB= σ 4

Pow

er

The frequency at which mostpower is emitted isproportional to the temperature

18 Apr 2002 Physics 102 Lecture 9 3

Blackbody radiation cont.In 1900, Planck found that by assuming the blackbody was

made up of tiny atomic oscillators that could absorb oremit discrete amounts of energy with E=hf he couldmatch the observed spectrum.

Energy is as photons in units of E hf=

h x= −6 6 10 34. Js

Ihfc

ef hf

k TB

=−

2 1

1

3

2

wherewith:

IfSpectrum of the oldest lightin the universe!

FYI:

18 Apr 2002 Physics 102 Lecture 9 4

The hot filament of an incandescent bulb is a goodsource of blackbody radiation. When observed through adiffraction grating, a broad spectrum is seen. When thetemperature of the filament is decreased:

A. The intensity of the spectrum decreases but the relativeintensities at all frequencies (colors) stay the same.

B. The intensity of the spectrum remains the same at highfrequencies (blue) but there is less red light.

C. The intensity decreases at all frequencies though bluelight is diminished more than red light.

D. The intensity decreases at all frequencies though redlight diminishes more than blue.

18 Apr 2002 Physics 102 Lecture 9 5

The reality of photons: photoelectric effect

Broad spectrum lamp

Ejected electron

Zinc plate

Electroscope

Light (electromagnetic radiation) impinging on a metalejects electrons from its surface.

Ejection of electrons depends onlight’s frequency, with a minimumfrequency required to eject any. If the frequency is toolow, no electron is ejected regardless of intensity.

18 Apr 2002 Physics 102 Lecture 9 6

Light is passed through a quartz prism. Theenergy of the dispersed light is measured in fivelocations 1-5. Which of the following is true:

1

2

3

4

5

A. There is only energy where wesee light in locations 2, 3, & 4.

B. The energy of the photons ishigher in the low number locations(UV) than in the high numberlocations (infrared)

C. We use quartz to enhance the dispersion and transmission ofvisible light and consequently give more energy to all the photons.

D. The energy of the photons increases in going from the infrared(location 1) to the UV (location 5).

18 Apr 2002 Physics 102 Lecture 9 7

ammeter tomeasure current

battery to accelerate electrons

A

UV

e

+

Observe that thereis current onlywhen UV shineson the cathode:photons need aminimum energyto photoejectelectrons.

18 Apr 2002 Physics 102 Lecture 9 8

Photoelectric effect cont.

The number of electrons ejected depends on intensity, butthe energy of the ejected electrons is independent ofenergy.

The wave model cannot explain the photoelectric effect.Einstein explained it using photons with E=hf.� A photon ejects an electron if it has the energy.� Intensity number of photons number of electrons.

For ejected electrons, KE=hf-W0 where W0 is the workfunction and depends on the metal.

∝ ∝

18 Apr 2002 Physics 102 Lecture 9 9

The momentum of a photon

� From relativity, we expect that p=E/c for photons

� Imagine a photon colliding with an electron at rest� conservation of energy and

� conservation of momentum

� imply (using relativistic formulaefor electron):

( )θ−=λ−λ′ cos1mch

(recall that λf=c)

Arthur Compton (Ph.D. Princeton 1916) demonstrated thatphotons have momentum as well as energy.

longer wavelength:

lower energy

18 Apr 2002 Physics 102 Lecture 9 10

A very weak light source emits a single photon in thedirection of a Young double-slit apparatus. The filmbehind the double slit will register:

A. A single dot behind one or the other slit

B. An interference pattern produced by the double slit.

C. Neither of the above.

Single photon/double slitThere seems no question that light acts as though it ismade of particles--photons--that carry momentumand energy.

Film?????

18 Apr 2002 Physics 102 Lecture 9 11

Wave-Particle Duality

So is light a wave or a particle?� In some circumstances it behaves like a particle

(photoelectric effect, Compton effect, …)

� In others it behaves like a wave (Young double slit,diffraction, …)

“I think I can safely say that nobody understands quantummechanics” - Richard Feynman (Princeton Ph.D. 1942)

18 Apr 2002 Physics 102 Lecture 9 12

100 e 3000 e 70000 eTonomura et al AJP 57, 1989

The Wave Nature of Matter

� By analogy, de Broglie (1924) suggested that matter mayhave wave-like properties, with λ=h/p.

� Davisson (Ph.D. Princeton) and Germer demonstrateddiffraction of electrons by crystals in 1925

� Electrons passing through a double slit act like light.

18 Apr 2002 Physics 102 Lecture 9 13

A beam of electrons is shot toward a crystal with aninteratomic spacing of 0.1 nm. Diffraction spots are seenwith a regular spacing of 0.1 radians. The electrons havea wavelength of about:

A. 100 nanometer

B. 1 nanometer

C. 0.01 nanometer

D. 0.0001 nanometers

From which we can derive their momentumthrough

ph x Js== ==

−−

λ λ6 6 10 34.

18 Apr 2002 Physics 102 Lecture 9 14

Particles act like waves and obey the laws ofdiffraction.

Light acts like a particle with zero rest mass andcollides with massive particles much as anothermassive particle would.

To understand the basis of our reality we have to ascribe tothe fundamental constituents of Nature properties of whichwe have no direct experience.

At the quantum level, Nature is fundamentally different thanat the “macro” level.

18 Apr 2002 Physics 102 Lecture 9 15

The Heisenberg Uncertainty Principle

� The narrower the slit we try to shine light through, thewider the diffraction pattern that results:

� The same is true for particles (since they are waves!):constraining the position increases the scatter in themomentum.

� The uncertainty principle puts a limit on how well two“complementary” quantities can be measuredsimultaneously.

∆ ∆∆ ∆

x p h

E t h

≥≥

4

4

ππ

θ λ∝∝ / w

Heisenberguncertaintyrelations

18 Apr 2002 Physics 102 Lecture 9 16

Atomic Structure: The Nucleus

The “plum-pudding” model (ca. 1900) imagined electronsembedded in a jelly-like positive medium

Rutherford, Geiger, and Marsden found that alpha particlesfired at a thin gold foil occasionally scattered backwards

This implied a dense, heavy nucleus

18 Apr 2002 Physics 102 Lecture 9 17

The Bohr Atom

� Bohr assumed electrons orbited nucleus in circular pathsand that the only stable orbits had angularmomentum in integer units of

� Using Coulomb’s law, you should show (and know!)that

� An atom emits or absorbs a photon of energy En1-En2when it jumps from one stable orbit to another(discontinuously).

L m v r nh

n e n n== ==2π

E nn ∝ 1 2

This was the geniusof his model.

18 Apr 2002 Physics 102 Lecture 9 18

Line Spectra and Electron Orbits

� An atom emits or absorbs quanta of energy when anelectron jumps from one allowed energy level to another.

� The quanta show up at discrete frequencies,characteristic of the type of atom.

f E h= ∆ /

visible

UV

Hydrogen

n=3 to n=2transitionYou can see this!

18 Apr 2002 Physics 102 Lecture 9 19

De Broglie Waves and the atom

� Using de Broglie’s wavelength for an electronand the quantization of angular momentumwe find:

� This has a natural graphical interpretation:allowed orbits are have

circumference equal to an integer number of wavelengths

� Think standing waves!

rn π=λ 2

π= 2nhLλ == h p

L prh

rnh== == ==

λ π2Thus:

18 Apr 2002 Physics 102 Lecture 9 20

Quantum Mechanics

� Particles are described by “wave functions” ψ that havea complex value at each point of space.

� The magnitude of the wave function squared describesthe probability of detecting the particle at a given spot.

� The wave function evolves deterministically accordingto Schrödinger’s equation:

� Solving this equation leads to a determination of thepossible orbits of the electrons and in turn to the“quantum numbers” in sec 30.5. These quantum numbersallow us to classify atoms and their bonds.

ψ⋅+ψ∇−=∂ψ∂

PEmt

i 22

2

hh

18 Apr 2002 Physics 102 Lecture 9 21

After quantum

� P.A.M. Dirac unified relativity with quantum mechanicsand gave birth to “field theory”

� Field theory was used to describe a wide variety sub-atomic phenomena. In fact, the 1999 Nobel prize was forwork in field theory.

� In theory today, the hot topic is “string theory” in whichthe elemental building blocks of Nature are tinyvibrating strings that live in a multidimensional (e.g. 10)dimensional space. The extra dimensions are “curled up”so we can’t experience them.