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LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos
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LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

Dec 20, 2015

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Page 1: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

LECTURE 19

BARRIER PENETRATION

TUNNELING PHENOMENA

PHYSICS 420SPRING 2006Dennis Papadopoulos

Page 2: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

Fig. 7-1, p.232

Page 3: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

We’ve learned about this situation: the finite potential well…

…but what if we “turn it upside down”?

This is a finite potential barrier.

When we solved this problem, our solutions looked like this…

I II IIIU

-L/2 L/2

E

What would you expect based on your knowledge of the finite box?

Page 4: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.
Page 5: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

Fig. 7-5, p.238

Page 6: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.
Page 7: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

(in actuality the light field in the optically dense space is evanescent, i.e. exponentially decaying)

Page 8: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

Below, the thick curves show the reflectance as the thickness of the low-index layer (air) changes from 10 to 900 nm. Note that as the layer thickness

increases, the reflectance becomes closer to total at 41 degrees. That is, FTR gives way to TIR.

Page 9: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

Qualitatively:

Page 10: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

(pure momentum states)

)()( tkxitkxiI BeAe

)()( tkxitkxiIII GeFe

to the left of the barrier

to the right of the barrier

Instructive to consider the probability of transmission and reflection…

R+T=1 of course…

2

2

*

*

incident*

reflected*

)(

)(

A

B

AA

BBR

2

2

*

*

incident*

dtransmitte*

)(

)(

A

F

AA

FFT

Page 11: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

+ +

+ +

+ +

+ +

+ +

+

0

E

-U

U(x)=-exx

0

eEx /2

dxExUmET )(22

exp)(

2

3

02

3

2

0 2

3

2

3

2

)(

2

2

e

Eexxe

dxxxedxExU

x

x

1

3

24exp)(

2

3

e

EmET

Page 12: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.
Page 13: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.

U(r)

r

E

R

rkZerU /2)( 2

EkZeR /2 21

kinetic energy of escaping

alpha particle

0

0 84exp)(r

ZR

E

EZET

Separation of centers of alpha and nucleus at edge of barrier 9.1 fm

Height of barrier 26.4 MeV

Radius at which barrier drops to alpha energy 26.9 fm

Width of barrier seen by alpha 17.9 fm

Alpha's frequency of hitting the barrier 1.1 x 10^21/s

Page 14: LECTURE 19 BARRIER PENETRATION TUNNELING PHENOMENA PHYSICS 420 SPRING 2006 Dennis Papadopoulos.