106 Nuclear - ChemConnections

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NUCLEAR CHEMISTRY
1
Dr. Ron Rusay
Chem 106
Spring 2004
© Copyright 1994-2004 R.J. Rusay
NUCLEAR CHEMISTRY
Nuclear Particles:
1
Mass
Charge
Symbol
1
1
1
PROTON
NEUTRON
1 amu
1 amu
© Copyright 1994-2004 R.J. Rusay
+1
0
H+,
1
1
1 H, 1 p
1
0n
Nuclear Decay / Radioactivity
Unstable nuclei “decay” i.e. they lose particles
which lead to other elements and isotopes.
 The elements and isotopes produced may
also be unstable and go through further
decay.

Nuclear
decay: reactions
conserve mass.

© Copyright 1994-2004 R.J. Rusay
QuickTime™ and a
Sorenson Video decompressor
are needed to see this picture.
Nuclear Particles
emitted from unstable nucleii
 Emitted
Particles:
Mass Charge Symbol
 alpha
particle 4 amu
 beta particle very small
 gamma
very very small
 positron
very small
© Copyright 1994-2004 R.J. Rusay
+2
-1
4He2  ;( 4He);4 
2
2
2
0e
0
1
1
0

+1
0
1
Nuclear Penetrating Power
alpha particle: low
 beta particle: moderate
 gamma: high


X-rays?
Water
© Copyright 1994-2004 R.J. Rusay
•Dosimeters measure radiation absorbed
•Radiation effects are cumulative (Madame Curie)
•rad = radiation absorbed dose ( 0.01 J/kg)
•rem= radiation equivalent for man (= rad x Q; Q=1 for X-rays,3
for neutrons, 10 for p+, 20 for -particles)
•Background radiation = 0.13 rem
•Annual limit is set at 0.17 rem above background
Alpha Decay–Heavy Elements

 238U
234Th
+  + e
t1/2 = 4.48 x 10 9 years
 210Po

+  +e
206Pb
t1/2 = 138 days
 256Rf

252No
60
27
Co
+ +e
t1/2 = 7 ms
For Cobalt 60 predict the alpha decay product:
60
27
Co
 4He  ? 56 Mn
2
25
Nuclear Decay Series
 If
the nuclei produced from radioactive
decay are unstable, they continue to
decay until a stable isotope results.
 An example is Radium which produces
Lead
226Ra     206Pb
88
82
© Copyright 1994-2004 R.J. Rusay
The 238U Decay
Series
Radiodating Methods
Three isotopes are currently used:
Carbon-14
half life 5,730 yrs
Potassium-40 half life 1.3 x 10 9 yrs
Uranium-238 half life 4.47 x 10 9 yrs
 The age of samples can be determined by
measuring their disintegrations over time.

© Copyright 1994-2003 R.J. Rusay
Decrease in Number of 14C
Nuclei Over Time
Radiocarbon Dating for Determining
the Age of Artifacts
An ancient wood sample has 6.25% of the
14C of a reference sample. What is the age
of the sample?
Nuclear Reactions
The mass of the visible universe is 73% H2
and 25% He. The remaining 2%, “heavy”
elements, have atomic masses >4.
 The “heavy” elements are formed at very high
temperatures (T>10 6 oC) by FUSION, i.e.
nuclei combining to form new elements.
 There is an upper limit to the production of
heavy nuclei at A=92, Uranium.
 Heavy nuclei split to lighter ones by FISSION

© Copyright 1994-2003 R.J. Rusay
NUCLEAR STABILITY
Patterns of Radioactive Decay
Alpha decay ()–heavy isotopes
 Beta decay () –neutron rich isotopes
 Positron emission ()–proton rich isotopes
 Electron capture–proton rich isotopes
x-rays
 Gamma-ray emission ()
 Spontaneous fission–very heavy isotopes

© Copyright 1994-2003 R.J. Rusay
NUCLEAR ENERGY

EINSTEIN’S
EQUATION FOR THE
CONVERSION OF
MASS INTO ENERGY
2
E
= mc

m = mass (kg)
c = Speed of light
8
c = 2.998 x 10 m/s

Mass  Energy
Electron volt (ev)
The energy an electron acquires when it moves through
a potential difference of one volt:
1 ev = 1.602 x 10-19J
Binding energies are commonly expressed in units
of megaelectron volts (Mev)
1 Mev = 106 ev = 1.602 x 10 -13J
A particularly useful factor converts a given mass defect
in atomic mass units to its energy equivalent in electron
volts:
1 amu = 931.5 x 106 ev = 931.5 Mev
Nuclear Reactions



Fission and Fusion reactions are highly exothermic
(1 Mev / nucleon).
This is 10 6 times larger than “chemical” reactions
which are about 1 ev / atom.
Nuclear fission was first used in a chain reaction:
235U 1n236U 141Ba 92Kr3 1n
36
0
92 0
92
56
© Copyright 1994-2003 R.J. Rusay
Nuclear Reactions:
Fission:


Fusion:
Fission and Fusion reactions are highly exothermic
(1 Mev / nucleon).
This is 10 6 times larger than “chemical” reactions
which are about 1 ev / atom.
Nuclear Reactions

Nuclear fission was first used in a chain reaction:
235U 1n236U141Ba 92Kr3 1n
36
0
92 0
92
56
Nuclear Reactions / Fission
The Fission Chain Reaction proceeds
geometrically: 1 neutron -> 3 -> 9 -> 27 -> 81
etc.
 1 Mole of U-235 (about 1/2 lb) produces
2 x 1010 kJ which is equivalent to the
combustion of 800 tons of Coal!
 Commercial nuclear reactors use fission to
produce electricity....Fission bombs were
used in the destruction of Hiroshima and
Nagasaki, Japan, in August 1945.

© Copyright 1994-2003 R.J. Rusay
The Nuclear Dawn
August 6, 1945
QuickTime™ and a
Cinepak decompressor
are needed to see this picture.
Nuclear Power Plant
Worldwide Nuclear Power Plants
Chernobyl, Ukraine
April,1986 and April,2001
Nuclear Reactions / Fusion
http://crystals.llnl.gov


Fusion has been described as the chemistry of the
sun and stars.
It too has been used in weapons. It has not yet found
a peaceful commercial application
The application has great promise in producing
relatively “clean” abundant energy through the
combination of Hydrogen isotopes particularly from
2H, deuterium and 3H, tritium: (NIF/National Ignition
Facility, LLNL)
2H3H4He 1n18.38MeV
0
© Copyright 1994-2004 R.J. Rusay

National Ignition Facility
Lawrence Livermore National Laboratory
National Ignition Facility
Lawrence Livermore National Laboratory
© Copyright 1994-2004 R.J. Rusay
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