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Introduction to Modern Physics A (mainly) historical perspective on - atomic physics - nuclear physics - particle physics

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Planck’s “Quantum Theory” The “oscillators” in the walls can only have certain energies – NOT continuous!

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Page 1: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Introduction to Modern Physics

A (mainly) historical perspective on

- atomic physics - nuclear physics- particle physics

Page 2: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Theories of Blackbody Radiation

Classical disaster !

Quantum solution

Page 3: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Planck’s “Quantum Theory”

The “oscillators” in the walls can only have certain energies – NOT continuous!

1,

5

kThc

eTI

Page 4: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

The Photoelectric Effect

Light = tiny particles!

Wave theory: takes too long to get enough energy to eject electronsParticle theory: energy is concentrated in packets -> efficiently ejects electrons!

Page 5: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics
Page 6: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

The Photoelectric Effect

Energy of molecular oscillator, E = nhfEmission: energy nhf -> (n-1)hf Light emitted in packet of energy E = hf

Einstein’s prediction: hf = KE + W (work function)

Page 7: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

c = f

Speed of light3 x 108

meter/secondor

30cm (1 foot) per

nanosecond

Wavelength (meter)

Frequency#vibrations/

second

Page 8: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

hf = KE + W (work function)

Page 9: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

The Photoelectric Effect

Wave Theory Photon Theory

Increase light intensity ->more electrons with more KE

Increase light intensity -> more photons -> more electronsbut max-KE unchanged !

Frequency of light does not affect electron KE Max-KE = hf - W

If f < f(minimum) , where hf(minimum) = W,Then NO electrons are emitted!

X

X

Page 10: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

How many photons from a lightbulb?

100W lightbulb, wavelength = 500nm

Energy/sec = 100 Joules

E = nhf -> n = E/hf = E/hc

n = 100J x 500 x 10-9 = 2.5 x 1020 !! 6.63 x 10-34 J.s x 3 x 108 m/s

Page 11: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

So matter contains electrons and light can be emitted in “chunks”… so what does this tell us about atoms??

Possible models of the atom

Which one is correct?

Page 12: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Electric potentialV(r) ~ 1/r

The Rutherford Experiment

Page 13: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Distance of closest approach ~ size of nucleus

At closest point KE -> PE, and PE = charge x potential

KE = PE = 1/40 x 2Ze2/R

R = 2Ze2/ (40 x KE) = 2 x 9 x 109 x 1.6 x 10-19 x Z 1.2 x 10-12 J= 3.8 x 10-16 Z meters = 3.0 x 10-14 m for Z=79 (Gold)

Page 14: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

The “correct” model of the atom

…but beware of simple images!

Page 15: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Atomic “signatures”

Rarefied gas

Only discrete lines!

An empirical formula!

2

1211

2 nR

2

1211

2 nR

n = 3,4,…

Page 16: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

The Origin of Line Spectra

Page 17: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Newton’s 2nd Law and Uniform Circular Motion

F = ma

Acceleration = v2/rTowards center of circle!

Page 18: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

How do we get “discrete energies”?

Linear momentum = mv

Radius r

Angular momentumL = mvr

Bohr’s “quantum” condition – motivated by the Balmer formula

2hnmvrL n ,...3,2,1n

Page 19: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Electron “waves” and the Bohr condition

De Broglie(1923): = h/mv

Only waves with a whole number of wavelengths persist

Quantized orbits!

n = 2r

2hnmvrL n

Same!!

Page 20: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Electrostatic force: Electron/Nucleus

COULOMBS LAW

Page 21: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Combine Coulomb’s Law with the Bohr condition:

maF Newton’s 2nd LawCircular motion r

va2

nn rmv

reZe 2

20

)(4

1

2hnmvrL n

nmrnhv2

Page 22: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

1

2

20

22

rZn

mZehnrn

mx

xxxx

mehr

10

1931

1234

20

2

1

10529.0

)10602.1)(1011.9)(14.3()1085.8)(10626.6(

(for Z = 1, hydrogen)

Page 23: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Calculate the total energy for the electron:Total Energy = Kinetic + Potential EnergyElectrostatic potential r

ZerQV

00 41

41

Electrostatic potential energy r

ZeeVU2

041

Page 24: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

nn r

ZemvE2

0

2

41

21

Total energy

Substitute

12

2

2220

42 18

EnZ

nhmeZEn

eVJoulesxh

meE 6.13181017.28 2

0

4

1

Page 25: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

2

6.13neVEn

So the energy is quantized !… now we can combine this with

hchf

EEhf lu

Page 26: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

223

0

42 1'1

8'11

nnchmeZEE

hc n

…and this correctly predicts the line spectrum for hydrogen,…and it gets the Rydberg constant R right!…however, it does not work for more complex atoms…

Page 27: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics
Page 28: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Experimental results

Page 29: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Quantum Mechanics – or how the atomic world really works (apparently!)

De Broglie(1923): = h/mv

Take the wave description of matter for real: Describe e.g. an electron by a “wavefunction” (x), then this obeys:

)()()(2 2

22

xExxUdxd

mh

Schroedinger’s famous equation

Page 30: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Now imagine we confine an electron in a “box” with infinitely hard/high walls:

Page 31: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Waves must end at the walls so:

Page 32: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

and the energy levels for these states are:

Discrete energies!

Page 33: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

The probabilities for the electron to be at various places inside the box are:

vs. Classical Mechanics

Uniform probability!

Page 34: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Applying the same quantum mechanical approach to the hydrogen atom:

Probability “cloud”

Bohr radius

Page 35: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

The “n = 2” state of hydrogen:

Page 36: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Atomic orbitals

Page 37: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Weird stuff!!

Page 38: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Weird stuff!!

Ghosts!!??

Page 39: Introduction to Modern Physics A (mainly) historical perspective on - atomic physics  - nuclear physics - particle physics

Conclusions- Classical mechanics/electromagnetism does not describe atomic behavior- The Bohr model with a “quantum condition” does better…but only for hydrogen- Quantum mechanics gives a full description and agrees with experiment- …but QM is weird!!