22.02
INT R ODUCTION T O
A P P L I E D N U C L E A R PH Y SICS
Spring 2012 Prof. Paola Cappellaro
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G O ALS OF 22.02
I ntro duction to A pplied N ucl ear P hysics
Learn the basic principles of nuclear and radiation science
After taking this class, you will able to study (and understand) any application of nuclear and radiation science
Keyword: WHY ?
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YO U R G O A L S ?
What are your goals and INTERESTS?
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NUCLEAR PH Y SICS
Describes nuclear properties and radiation: structure and characteristics of nuclei radiation sources and interaction with matter
T o understand nuclear structure and radiation we study: nuclei, nucleons and electrons
microscopic processes
T o understand we need modern physics Quantum mechanics
(Special Relativity)
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W H A T A R E T H E M AG I C N U M B E R S ?
Image by MIT OpenCourseWare.
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W H A T A R E T H E M AG I C N U M B E R S ?
A computer
pr ogram variable ? Rock band?
Iphone App?
Games to win to clinch the season?
Number of jobs?
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W H A T A R E T H E M AG I C N U M B E R S ?
© Wikimedia Foundation. License CC BY-SA. This content is excluded from our Creative Commons license. For more inf o 7 rmation, see http://ocw.mit.edu/fairuse .
W H A T A R E T H E M AG I C N U M B E R S ?
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App screenshot © Design7; "The Magic Numbers" cover art © EMI; news article excerpt © The New York Times Company . All rights reserved. This content is exclude d from our Creative Commons license. For more information, see http://ocw.mit.edu/fairuse .
W H A T A R E T H E M AG I C N U M B E R S ?
In nuclear physics?
2 8 20 28 50 82 126
And why are they magic?
You’ll find out at the end of this lecture
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BINDING ENERGY
Mass-energy equivalence
E = mc 2
Nuclei are composed of protons and neutrons,
held together by some energy
Z m proton + N m neutron / = M Nucleus
Dif ference in mass ➜ dif ference in energy
This explains why we get energy from nuclear fission, from fusion, from radioactive decay products...
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NUCLEAR NOMENCL A TURE
Atoms/nuclei are specified by # of neutrons: N
protons: Z
[Z electron in neutral atoms]
Atoms of same element have same atomic number Z
Isotopes of the same element have same atomic number Z but dif ferent number of neutrons N
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A X
Z
NUCLEAR NOMENCL A TURE
Isotopes are denoted by
X is the chemical symbol
A = Z + N is the mass number
E.g. : 235 U, 238 U [Z is redundant here]
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NUCLEAR NOMENCL A TURE
N uclide
atom/nucleus with a specific N and Z
I sobar
nuclides with same mass # A ( ≠ Z,N)
I sotone
nuclides with same N, ≠ Z
I somer
same nuclide (but dif ferent energy state)
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BINDING ENERGY
Mass-energy equivalence
E = mc 2
Nuclei are held together by the binding energy
Z m proton + N m neutron / = M Nucleus
Dif ference in mass ➜ dif ference in energy
Why is there a mass dif ference?
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BINDING ENERGY
Binding Energy = [Mass of its constituents-Nucleus Mass] x c 2
m N
B = ⇥ Z m p + N m n — ( A X ) ⇤ c 2
In terms of measurable quantities:
B = Z m p + N m n — [ m A ( A X ) — Z m e ] c 2
B is always n p e o g s a i t t i i v v e e for stable nuclei
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SEMI-EMPIRIC AL MASS FORMULA
M ( Z, A ) = Z m ( 1 H ) + N m n — B ( Z, A ) /c 2
From a simple model of the nucleus, described as a liquid drop
➜ formula for B(Z,A)
5 terms, plot B(Z,A) vs. A
Photo courtesy of cdw9 on Flickr. License CC BY-NC.
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SEMI-EMPIRIC AL MASS FORMULA
M ( Z, A ) = Z m ( 1 H ) + N m n — B ( Z, A ) /c 2
With binding energy given by:
Surface Coulomb
B ( A, Z ) = a v A — a s A 2 / 3 — a c Z ( Z — 1) A — 1 / 3
— a sy m
Volume ( A — 2 Z ) 2
A
+ δ a p A
— 3 / 4
{
symmetry pairing
Photo courtesy of cdw9 on Flickr. License CC BY-NC.
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SEMF: Binding Energ y per Nucleon
B/A
(binding energy per nucleon)
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A (Mass number)
0 50 100 150 200 250
B(Z,A)/A ~ cst.(8 MeV) - corrections
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B/A: JUMPS
B/A
(binding energy per nucleon)
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A (Mass number)
0 50 100 150 200 250
“Jumps” in Binding energy from experimental data
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AT O M S P E R I O D I C P R O P E R T I E S
‡ Ê Ionization Energy (similar to B per nucleon)
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2000
kJ per Mole
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Z
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AT O M I C P E R I O D I C TA B L E
Periodic properties → atomic structure Ionization Energy (similar to B per nucleon)
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CHA R T OF NUCL ID ES
http://ww w .nndc.bnl.gov/chart/
“Periodic” , more complex properties → nuclear structure
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W H A T A R E T H E M AG I C N U M B E R S ?
2 8 20 28 50 82 126
And why are they magic?
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W H A T A R E T H E M AG I C N U M B E R S ?
2 8 20 28 50 82 126
And why are they called magic?
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W H A T A R E T H E M AG I C N U M B E R S ?
2 8 20 28 50 82 126
And why are they called magic?
Maria Goeppert Mayer “discovered” them in ~1945 Observation of periodicity in binding energy
➜ shell model for nuclei
Eugene Wigner believed in liquid-drop model, did not trust new theory
➜ called these numbers “magic”
Quantum mechanics only can explain them As well as many other “misteries”,
e.g. randomness of radioactive decay
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22.02 SPRING 2012
Class Logistics
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RECI T A TIONS
There will be weekly recitations
Recitations will review some topics from lecture and mathematical background
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TEXTBOOKS
Lecture notes
Usually posted before the lecture
Kenneth S. Krane,
Introductory Nuclear Physics, Wiley
David J. Griffiths
Introduction to Quantum Mechanics, 2nd edition Pearson Prentice Hall, 2005
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P-S ETS
The problem sets are an essential part of the course T ry solving the Pset on your own
Discuss with other students Attend recitations
Ask T A and Professor
P- sets will be posted
9 P-sets, tentative schedule in Syllabus hand-out P-set solutions will be posted
No p-sets will be accepted after the deadline
W orst P-set grade will be dropped
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GRADING
Homework 25%
W orst P-set grade will be dropped
Mid- T erm 30%
W eek before Spring Break: Conflicts?
Final exam 40%
“Mostly” on second part of class Class Participation 5%
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QU E S T I O N S ?
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MIT OpenCourseWare http://ocw.mit.edu
22.02 Introduction to Applied Nuclear Physics
Spring 2012
For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms .