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NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic Calculations Photon Interactions with Matter Nuclear Energetics
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NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

Mar 28, 2015

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Page 1: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

NE 105 - Introduction to Nuclear EngineeringSpring 2011

Classroom Session 4 - Fundamental Concepts End

Nuclear Energetics Intro

•Classic and Relativistic Calculations•Photon Interactions with Matter•Nuclear Energetics

Page 2: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

2

Electron Volt

Work done by one electron accelerated through a potential difference of one volt

1 eV = 1.60217646x10-19 J

Example:What is the speed (m/s) of a 12 eV 134Xe

ion?(from the chart of the nuclides: 134Xe Weights = 133.905394

AMU)Use classic concept of KE for nowamu in table 1.5Joule = Energy, Work = Force (N) x d =kg m2/s2

Page 3: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

3

Correction of the book… REMEMBER!

Please ignore the c2. It is confusing

Book: Page 6

Page 4: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

4

4156.4 m/s ~9,300 m.p.hi.e. even very low energy ions are moving pretty fast

Please remember this is ONLY for classical calculations.At energies close to “c”, need to use relativistic calculations

Page 5: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

5

What is the speed of a 100.00 MeV proton:

102

,540

m/s

5,4

67 g

/s

1.3

8e8

m/s

138

40 m

/s

3e8

m/s

20% 20% 20%20%20%1. 102,540 m/s2. 5,467 g/s3. 1.38e8 m/s4. 13840 m/s5. 3e8 m/s

Page 6: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

6

100MeV proton = 0.46 c :close to the speed of light.

i.e. classic equations do NOT hold

i.e. 0.46 is likely wrong

What is the speed of a 100.00 MeV proton:

Page 7: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

7

Newton Laws

For over 200 years, Newton’s laws worked Accurately described many physical

behaviors Unifying the earth and the skies

Previously: Sub-lunar sphere: impure and imperfect Skies: perfect and immutable (circle,

ether)

Page 8: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

8

Special Theory of Relativity - Effects

“Mass Increase” with increasing velocity

Increase quantified by Lorentz factor ():

m(v) m0

1 v 2 c 2

2 2 1

v<<<c 1 classic limit1 always

v~c 0 effect is max

v c

Page 9: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

9

Length and time are also modified relative to an object’s speed

For example: To find speed…

L(v) L0 1 v 2 c 2

22

0

1)(

cv

tvt

Special Theory of Relativity - Effects

Page 10: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

10

What is the kinetic energy of a 100.00 MeV proton?

Hint: Relativistic speeds, i.e. use this equation:

Special Theory of Relativity - Effects

2 20E mc m c KE

m(v) m0

1 v 2 c 2

Page 11: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

11

The error grows as v c

Reminder: simple error is

Accepted Value - Obtained Value100 % Error

Accepted Value

Page 12: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

12

Remember

Relativistic calculation required when:

kinetic energy ~ rest energy

What is the rest mass of an electron? What is the rest mass of a p+ or n0? What is the rest mass of heavy ions?

(Table 1.5 book)

Use:eVkeVMeV

Page 13: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

13

What is the kinetic energy of a 1 MeV electron? Rest mass of the electron, me=0.511MeV

0.5

11 M

eV

0.4

89 M

eV

0.9

99 M

eV

1 M

eV

0 M

eV

20% 20% 20%20%20%

1. 0.511 MeV2. 0.489 MeV3. 0.999 MeV4. 1 MeV5. 0 MeV

Page 14: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

14

What is the speed of a 1 MeV electron? Rest mass of the electron, me=0.511MeV

0.58c 0.81c

0.86c 0.94c

0.993c

20% 20% 20%20%20%

1. 0.58c2. 0.81c3. 0.86c4. 0.94c5. 0.993c

Page 15: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

15

Solution:2 2

0

22 0

2

0.511 1 1.511

m cand solving for v, from relativistic equation mc = :

0.5111 0.94

1.511

mc m c KE MeV MeV MeV

v c c

Page 16: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

16

Special Theory of Relativity - Effects

In Nuclear Engineering we rarely work with neutrons of more than 10MeV.

We stick to classic calculations for KE of p, n, , ions, and fission fragments

Homework 2.3. What is the error in computing speed of a 10 MeV neutron classically instead of relativistically?

Page 17: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

Radiation Interaction with Matter

Ionizing Radiation

Page 18: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

19

Photon Interactions

EnergyHighIntermediateLow

Pair Production

Compton Scattering

Photoelectric Effect

Page 19: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

20

Pair Production

Page 20: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

21

Compton Scattering

Page 21: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

22

The Photoelectric Effect

Page 22: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

23

Compton Scattering – The Experiment

E

E’

In 1922, Compton obtained this dataScattered X-Rays had an increase in wavelengthCan you explain why?

Page 23: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

24

Compton Scattering – Light has p!

If light is a wave, then radiation scattered by an electron should have no change in wavelengthIn 1922, Compton demonstrated that that x-rays scattered from electrons had a decrease in wavelength.

This is only possible if light is treated as a particle with linear momentum equal to p=h/

)cos1(' secm

h

Why the equation written for the photon angle?

1 1 1(1 cos )

' seE E m c

EE’

Page 24: NE 105 - Introduction to Nuclear Engineering Spring 2011 Classroom Session 4 - Fundamental Concepts End Nuclear Energetics Intro Classic and Relativistic.

25

Follow equations

But pay attention to unitsFor wavelength please use nm

6.63 -34

e

h e J

m c

. s

9.11e-31 kg 3e8 m / s

1 kg

2m

1 J 2. s

1 9

1

e nm

m [ ] nm