phy 102: quantum physics topic 3 de broglie waves

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PHY 102: Quantum Physics Topic 3 De Broglie Waves

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PHY 102: Quantum Physics Topic 3 De Broglie Waves. Wave-particle duality De Broglie Waves Particles in boxes: Energy quantisation Quantisation of orbital angular momentum in Bohr model. Einstein’s postulate. - PowerPoint PPT Presentation

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Page 1: PHY 102: Quantum Physics Topic 3 De Broglie Waves

PHY 102: Quantum Physics

Topic 3De Broglie Waves

Page 2: PHY 102: Quantum Physics Topic 3 De Broglie Waves

•Wave-particle duality

•De Broglie Waves

•Particles in boxes: Energy quantisation

•Quantisation of orbital angular momentum in Bohr model

Page 3: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Einstein’s postulate

A beam of light can be treated as a stream of particles (PHOTONS) with zero rest mass

Each photon has energy:

hchfEp

where h is a constant (Planck’s constant, h ≈ 6.63 x 10-34 Js)

f, λ, c, are frequency, wavelength and velocity of light (in vacuum) respectively.

Light intensity is proportional to PHOTON FLUX (no of photons passing through unit area per second)

Page 4: PHY 102: Quantum Physics Topic 3 De Broglie Waves

2222 pcmcE

consequently, particle with zero rest mass (eg photon) has momentum pgiven by:

h

chf

cEp

From Special Theory of Relativity……………

Page 5: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Wave-particle Duality

So, an electromagnetic wave of wavelength λ and frequency f can be thought of as a stream of particles with energy E and momentum p given by:

hfE

hp

Page 6: PHY 102: Quantum Physics Topic 3 De Broglie Waves

The de Broglie HypothesisIn 1924, de Broglie suggested that if waves of wavelength λ were associated with particles of momentum p=h/λ, then it should also work the other way round…….

A particle of mass m, moving with velocity v has momentum p given by:

hmvp

Page 7: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Kinetic Energy of particle

mk

mh

mpKE

222

22

2

22

If the de Broglie hypothesis is correct, then a stream of classical particles should show evidence of wave-like characteristics……………………………………………

Page 8: PHY 102: Quantum Physics Topic 3 De Broglie Waves

De Broglie wavelength of everyday objects…

Eg. Tennis ball….

Mass ~60gVelocity ~ 100mph ≈ 45 m/s

Momentum =

De Broglie wavelength =

Page 9: PHY 102: Quantum Physics Topic 3 De Broglie Waves

De Broglie wavelength of a 1keV electron..

KE =

Momentum =

De Broglie wavelength =

Page 10: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Observation of wave-like behaviour

Just like a classical wave, effects such as diffraction and interference observed when the wave interacts with objects with dimensions of the same order as the wavelength, ie

d~So, wave-like properties not observed for everyday macroscopic objects, which have de Broglie wavelengths ~10-34 m.

What about our electrons, with λ~ 10-10 – 10-11m……??

Page 11: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Electron Diffraction

Page 12: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Electron Diffraction

sin2dn

Page 13: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Standing de Broglie wavesEg electron in a “box” (infinite potential well)

V=0

V= V=

Electron “rattles” to and fro

V=0

V= V=

Standing wave formed

Page 14: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Wavelengths of confined states

V=0

V= V=

L

LkL ; 2

LkL 2 ;

LkL 3 ;

32

Page 15: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Energies of confined states

V=0

V= V=

L

In general:

Lnk

n = 1, 2, 3, 4, 5, ……….

2

22222

22 mLn

mkE

ie QUANTISED ENERGY LEVELS

Page 16: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Example calculation 1Calculate the separation between the two lowest energy states for an electron confined in an infinite potential well of width 1nm………

Page 17: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Example calculation 2Calculate the separation between the two lowest energy states for an oxygen molecule confined in a 1cm cubic box

m=2.7 x 10-26 kg

Page 18: PHY 102: Quantum Physics Topic 3 De Broglie Waves

When do quantisation effects become important?

Rule of thumb: at temperatures below which kT becomes comparable with ΔE.

For our confined electron (example 1), T~10000K

For our oxygen molecule, T~10-15K !!!!!!!!

So, quantisation effects easy to observe for electron, whereas the translational motion of the gas atom in the “normal sized” box obeys classical mechanics (continuous energy distribution)

(NB kT at room temperature (300K) is about 0.025eV)

Page 19: PHY 102: Quantum Physics Topic 3 De Broglie Waves

The Bohr Model (1912-13)Bohr suggested that the electrons in an atom orbit the positively-charged nucleus, in a similar way to planets orbiting the Sun

(but centripetal force provided by electrostatic attraction rather that gravitation)

Hydrogen atom: single electron orbiting positive nucleus of charge +Ze, where Z =1:

r

v

F+Ze

-e

Page 20: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Failure of the Classical model

The orbiting electron is an accelerating charge.

Accelerating charges emit electromagnetic waves and therefore lose energy

Classical physics predicts electron should “spiral in” to the nucleus emitting continuous spectrum of radiation as the atom “collapses”

CLASSICAL PHYSICS CAN’T GIVE US STABLE ATOMS………………..

Page 21: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Quantisation of angular momentum

Bohr now makes the bold assumption that the orbital angular momentum of the electron is quantised………

Since v is perpendicular to r, the orbital angular momentum is just given by L = mvr.

Bohr suggested that this is quantised, so that:

nnhmvr 2

IMPLICATIONS???..........................................................................

Page 22: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Electron standing waves and the Bohr ModelBohr’s suggestion that orbital angular momentum of electrons is quantised is equivalent to the requirement that an integer number of de Broglie wavelengths must fit into the electron orbit:

Page 23: PHY 102: Quantum Physics Topic 3 De Broglie Waves

Electron standing waves and the Bohr Model

nrn 2 nne

rvmhn 2

nnen rvmL ne

n

ne vmL

vmhn

2

nnhLn 2