1Chemistry 2C Lecture 24: May 26 th, 2010 1)Belts of Stability 2)Magic Numbers 3)Einstein and his...
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Transcript of 1Chemistry 2C Lecture 24: May 26 th, 2010 1)Belts of Stability 2)Magic Numbers 3)Einstein and his...
1Chemistry 2C Lecture 24: May 26th, 2010
1) Belts of Stability2) Magic Numbers
3) Einstein and his Equation4) Artificial Radioactivity
5) Nuclear kinetics6) Binding Energies
7) Fusion and Fission
Lecture 24: Nuclear
2Chemistry 2C Lecture 24: May 26th, 2010
What kind of particle is emitted in this radioactive decay?
Question
Yes: The mass number is unchanged and the nuclear number is increased by one. A neutron has decomposed to a proton and an electron, thus emitting
an electron from the nucleus.
231 23190 91 ?Th Pa
Option 3: Perhaps the nucleus has emitted a beta particle?
Option 1: Perhaps the nucleus has emitted an alpha particle?No: The mass number hasn’t changed, which should by four if an alpha
particle is emitted!
Option 2: Perhaps the nucleus has emitted a gamma particle?
Yes/No?: The emission of a gamma particle (by itself) doesn’t change both the nuclear number and the mass number. This doesn’t fly with the info
above!
3Chemistry 2C Lecture 24: May 26th, 2010
RadioactivityThe amount of radioactive contamination
released by human activity is rather small, in global terms, but the radiation
background is also rather low. Some sources claim that the Earth's background
radiation level has tripled since the beginning of the twentieth century. In fact, the total amount of radioactivity
released by man is inconsequential to the large quantities of radioactivity in the
natural environment
Fiestaware was a very popular brand of ceramic tableware. Before the early 1940's the orange color of it was made with uranium in the glaze
(uranium was used to get the color, not just accidentally)
4Chemistry 2C Lecture 24: May 26th, 2010
The belt of Stability
Answer: Many factors contribute to this question, but we can make some
observations. Some patterns exist!
Question: Why do nuclei decay. Why are they unstable?
It turns out that certain numbers of protons or of neutrons are specially
stable in nuclides. Protons and neutrons are treated separately. The sum is not
the important number. Even numbers are more stable than odd numbers. When
those two rules don't predict, then nearness to the belt of stability predicts.
5Chemistry 2C Lecture 24: May 26th, 2010
As Z increases, the number of neutrons has to go up faster
than Z goes up because the
“nuclear glue” that makes the nucleus stable is provided by the neutrons. Remember the
positively charged protons are
electrically repelled from each other! Above Z=83, all
elements are radioactive!
Most Z>83 nuclides decay via emission
Positron (+) emission or electron capture
preferred here!
emission preferred here!
The Belt of Stability
6Chemistry 2C Lecture 24: May 26th, 2010
# of Protons
Magic Numbers
# of Neutrons
Upshot: Nature prefers even number of protons or neutrons
# of stable nuclides
odd odd 4
even odd 55
odd even 50
even even 163
examples
21 H
63 Li
136 C
4722Ti
2311 Na
2713 Al
126 C
168 O
Magic numbers
# of protons: 2, 8, 20, 28, 50, 82, 114# of neutrons: 2, 8, 20, 28, 50, 82, 126,
184
These numbers correspond to the filling of nuclear shells in a similar way that filled electron orbitals are stable (e.g. noble gases)
7Chemistry 2C Lecture 24: May 26th, 2010
Radioactive Anomalies
All elements above 83 are radioactive, but below that
only technetium (Z=43) and promethium (Z=61) have no
stable isotopes).
Note: Both have odd number of protons!
Tc isotopes:
Half-life: 2.6x 106 y
Half-life: 4.2x 106 y
Half-life: 2.1x 106 y
9743Tc9843Tc9943Tc
Pm isotopes:
Half-life: 17.7 y
Half-life: 5.5 y
Half-life: 2.62 y
14561 Pm
14761 Pm
14661 Pm
8Chemistry 2C Lecture 24: May 26th, 2010
Einstein’s Famous FormulaThe theoretical physics equation E = mc2 states a relationship between energy (E), in whatever
form, and mass (m). In this formula, c², the square of the speed of light in vacuum, is the conversion factor required to formally convert from units of mass to units of energy, i.e. the
energy per unit mass.
In chemical reaction, mass changes aren’t noticeable.
In nuclear reaction, mass changes are noticeable and large energies are involved.
Example:238 234 492 90 2U Th He
238.0003 u
233.9942 u
4.0015 u
237.9957 u
For nuclides (ignoring electrons)
9Chemistry 2C Lecture 24: May 26th, 2010
Einstein’s Famous Formula
Example: 238 234 492 90 2U Th He
238.0003 u
233.9942 u
4.0015 u
237.9957 u
For nuclides (ignoring electrons)
m = 0.0046 u / nucleus
m = 0.0046 g / mol
E=mc2
=(0.0046 g / mol) ( 2.9979 x108 m/s)2
=4.13 x 1011 J/mol
That is a lot of energy!!!!
10Chemistry 2C Lecture 24: May 26th, 2010
Artificial Radioactivity Not all nuclear reactions are spontaneous. These reactions occur when
stable isotopes are bombarded with particles such as neutrons. This method of inducing a nuclear reaction to proceed is termed artificial
radioactivity. This meant new nuclear reactions, which wouldn't have been viewed spontaneously, could now be observed. Since about 1940, a set of
new elements with atomic numbers over 92 (the atomic number of the heaviest naturally occurring element, Uranium) have been artificially
made. They are called the transuranium elements.
The first artificial radionuclide that was discovered was by Irene Jolet-Curie and Frederic Joliot.
27 4 30 113 2 15 0Al He P n
30 30 015 14 1P Si neutron
11Chemistry 2C Lecture 24: May 26th, 2010
Artificial Radioactivity
Example 26-2
Write a nuclear equation for the production of 124I by bombardment of 121Sb with particles
121 4 12451 2 53 ?Sb He I
Whilst the nuclear number is balanced in the equation, the mass number is not! If a neutron were also ejected after the absorption of an -particle,
then both will be balanced.
121 4 124 151 2 53 0Sb He I n
12Chemistry 2C Lecture 24: May 26th, 2010
Artificial Radioactivity Example 26-2
Write the nuclear equation for the subsequent decay of 124I by positron emission.
124 ? 053 ? 1 X I
Balance the nuclear number and mass number separately!
• Mass number is unaffected by the change of a proton to a neutron and emission of a positron!
• The nuclear number decreases by one after this process
124 124 053 52 1 Te I
13Chemistry 2C Lecture 24: May 26th, 2010
Artificial Radioactivity The making of new elements is very important!
1) Make new elements2) Make isotopes for cancer therapy and bone scans, etc.
Here on campus, we have the Crocker Nuclear Law, a medium –sized circular accelerator call a cyclotron. It can produce charged particles
with a lot of kinetic energy which in turn can cause neutrons to be formed. At UC Berkeley, there is the Lawrence Radiation Lab (Lawrence
Berkeley National Lab), where many new elements have been made: Americium (Z=95), Berkelium (Z=97), Californium (Z=98).
To make new elements, nuclei of the lighter elements are used to bombard heavier
ones:249 15 260 198 7 105 0 4 Cf N Db n
14Chemistry 2C Lecture 24: May 26th, 2010
Transuranium Metals
Americium is the only synthetic (man-made) element that can be purchased at Walmart. It does
not exist in nature and all of it that exists in the world, and at Walmart, was creating in nuclear
reactors and extracted from spent fuel rods during reprocessing
It's illegal to disassemble a smoke detector and remove the tiny radioactive dot that is contained in every ionization detector.
Berkelium and Californium can be created in nuclear reactors and have few industrial applications. They are extremely radioactive, extremely
toxic, and extremely hard to get.
15Chemistry 2C Lecture 24: May 26th, 2010
TimescalesSome of the artificially produced elements have long enough lifetimes to get some measurable amount of product formed, but sometimes only a
few atoms have been detected.
All radioactive nuclei will decay, eventually, but when? For a single nucleus, it’s impossible to predict when, but for a collection of atoms there
is a statistical probability for decay.
This process is a first order process, with the rate of decay is called activity
A=N
Rate of decay: Decay constant # of atoms
Units: Activity of a Radioactive Material: New: The becqueral (1dis/sec)
Old: The Curie (3.7 x 1011 dis/sec)dis=disintegration event
16Chemistry 2C Lecture 24: May 26th, 2010
Timescales
This can be integrated directly to give ln N = -t + C, where C is a constant of integration.
Although radioactive decay involves discrete events of nuclear disintegration, the number of events is so large that it can be treated like a continuum and the methods of calculus employed to predict the behavior. The result from the decay probability can be put in the differential form:
Taking the exponent of both sides gives
so the standard form of the decay equation is
17Chemistry 2C Lecture 24: May 26th, 2010
Timescaleshe rate of radioactive decay is typically expressed in terms of either the
radioactive half-life, or the radioactive decay constant. They are related as follows:
The half-life and the decay constant give the same information, so either may be used to characterize decay. Another useful concept in radioactive decay is
the average lifetime.
Only because of the underlying 1st order kinetics
18Chemistry 2C Lecture 24: May 26th, 2010
Timescales
Half-lived vary immensely among radionuclides
t1/2 = 5730 years146 C
4019 K
21484 Po
12353 I
11149 In
t1/2 = 1.25 x 109 years
t1/2 = 1.64 x 10-4 years
t1/2 = 13.3 hours
t1/2 = 10 hours
Used in carbon dating
Used in thyroid imaging
Used in spinal and cranial fluid imaging
natural
artificial
19Chemistry 2C Lecture 24: May 26th, 2010
Unlike Chemical reactions
Unlike chemical reaction, these half-lived are Temperature independent and also do not depend at all on the state of the
mater or type of chemical combination
k=Ae-Ea/RT
20Chemistry 2C Lecture 24: May 26th, 2010
Binding Energy
It is found that the nuclei weigh less than the masses of the individual particles in them. This is called the “mass deficit.”
When the nuclear particles (nucleons) come together to form a nuclear, energy is released (this is an exothermic reaction)
The binding energy is the energy needed to break the nucleus into individual protons and neutrons
21Chemistry 2C Lecture 24: May 26th, 2010
Binding EnergyThe enormity of the nuclear binding energy can perhaps be better
appreciated by comparing it to the binding energy of an electron in an atom. The comparison of the alpha particle binding energy with the binding energy
of the electron in a hydrogen atom is shown below. The nuclear binding energies are on the order of a million times greater than the electron binding
energies of atoms
A lot of energy!
For -particle, the mass deficit is 0.0305uPlugging into E=mc2, gives you an energy of 1.492 x 10-10 J
22Chemistry 2C Lecture 24: May 26th, 2010
Binding EnergyNuclear energy can be extracted by generating nuclides with greater binding
energy from those of lesser (thus releasing energy that can be used for constructive uses.
Fe is the most stable nuclide with greatest binding energy
Fusion works on this side of Fe (taking small nuclides to
make bigger ones)
Fission works on this side of Fe
(taking big nuclides to
smaller ones)
23Chemistry 2C Lecture 24: May 26th, 2010
Fission and FusionDuring the search for new elements in the 1930’s, it was discovered that bombarding a nucleus with neutrons could cause a nuclear to absorb a
neutron and then split into two large fragments.
This gives overall increase in energy as the sum of the binding energies for Ba and Kr are higher than for U!
235 1 23692 0 92U n U
236 92 141 192 36 56 0 3U Kr Ba n
E=8.2x107 kJ/g of 235U = 3 tons of coal combustion
More neutrons are produced as products faster than being absorbed! This is a chain reaction that exponentially increases the rate =
explosion!!!!
24Chemistry 2C Lecture 24: May 26th, 2010
Fission and Fusion
The chain reaction is the basis for both a nuclear bomb and for a nuclear fission reactor. Hopefully, in a reactor, the chain reaction is controlled, and
generated heats which is used to make steam and run a turbine to generate electricity.