Chapter 30 Nuclear Physics and Radioactivity
Describe a proton neutron nucleon
Z atomic number A atomic mass number N = A - Z
isotope natural abundance
How is the radius of a nucleus estimated? r = 1.2 x 10-15 A 1/3
atomic mass unit u What is the standard for u?
binding energy
Know how to calculate the total and average binding energy.
A table of atomic masses will be given.
Be aware of the graph in figure 30-1.
What evidence do we have that the strong nuclear force exists?
How strong is the strong nuclear force compared to the electrical force?
What is the range of the strong nuclear force?
Is there an equation which is used to calculate the strength of the strong nuclear force?
Know the trend of the graph of N vs. Z
weak nuclear force
radioactivity Becquerel
Half-Life
model for alpha decay model for beta decay
positron electron capture
neutrino model for gamma decay
disintegration energy Q = (MParent - Mdaughter - Mother)c2
conservation of nucleon number
Chapter 30 continued
half-life decay constant l D N = - l N D t
N = No e-l t Activity = l N 1 Curie = 3.7 x 1010 decays per second
T ½ = 0.693 / l
decay series
Which isotopes in the decay chain will have the greatest abundance?
Radioative dating
What is the goal?
What are the assumptions?
How are calculations performed?
Section 30-12 PHY162 only
What is the basic mechanism by which we detect radiation?
How does a Geiger counter operate?
How does a cloud chamber operate?
How does a bubble chamber operate?
PHY162
radii of atoms, ionization energies across the periodic table
Hydrogen atom calculations of probability using y 2 1,0,0
tunneling
Chapter 31 Nuclear Energy
nuclear reaction transmutation
reaction energy Q-value Q = ( Mreactants - Mproducts) c2
What are the most effective projectiles for causing nuclear reactions?
fission compound nucleus
fission fragments
chain reaction self-sustaining chain reaction
first nuclear reactor when? where? why?
moderator heavy water
enriched fuel critical mass fuel rod
control rods delayed neutrons
core primary coolant loop
secondary coolant loop heat exchanger
breeder reactor atom bomb design
radioactive fallout
fusion
plasma magnetic confinement
tokamak break-even
Three Mile Island Chernobyl
PHY162
derivation of radioactive decay law
classification of elementary particles gauge bosons, leptons, hadrons, baryons
particle resonances
quarks (if not covered on MWF)
Chapter 31 continued
How does radiation damage a cell?
dose curie radionuclides
absorbed dose rad gray
RBE quality factor rem
Why do alpha rays have the highest quality factor?
background radiation sources
How can you lower the dose you receive from a radioactive source? 3 ways
radiation sickness
tracer
NMR
Chapter 32 Elementary Particles
What are two reasons that high energy particles are produced?
How does a Van de Graaff accelerator accelerate charged particles?
How does a cyclotron accelerate charged particles?
How does a synchrotron accelerate charged particles?
How does a linear accelerator accelerate charged particles?
Which of the above is used to create the highest particle energy?
Name the 6 "elementary particles" from the list of the 1930’s.
What two characteristics does antimatter have compared to the regular matter particle?
Does the photon have an antiparticle?
When does annihilation occur?
Why were quarks proposed?
What are the characteristics of quarks?
How many quarks are required to construct a proton or neutron?
What is the goal of Grand Unified Theories?
Name one experimental test for Grand Unified Theories.
Chapter 33 Astrophysics and Cosmology
How has the accepted view of the earth’s position in the universe changed over time?
How can the data of the sun’s orbit be used to estimate the number of stars in the Milky Way Galaxy?
How are distances to stars and galaxies determined?
parallax
apparent vs. absolute brightness
At what point does a cloud of gas become a star?
What is the main sequence?
As a star ages, why does its core contract?
nucleosynthesis
What causes a supernova?
neutron star pulsar
General Theory of Relativity
principle of equivalence
geodesic
black hole
expansion of the universe v = Hd
Big Bang
Copyright© 2001 - 2006 by Greg Clements Permission is granted to reproduce this document as long as 1) this copyright notice is included, 2) no charge above photocopy costs is made, and, 3) the use is for an educational purpose. Editing of the document to suit your own class style and purposes is allowed.