Nuclear Chemistry “Nuclear Reaction” – Anytime the nucleus of an atom changes. Nuclear Chemistry.
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Transcript of Nuclear Chemistry
Chapter 19Nuclear Chemistry
General Chemistry: An Integrated Approach
Hill, Petrucci, 4th Edition
Mark P. HeitzState University of New York at Brockport
© 2005, Prentice Hall, Inc.
Chapter 19: Nuclear Chemistry 2
Introduction
Nuclear properties can be used to distinguish among the various isotopes of an element
Examples: carbon-13, carbon-14 C,C 146
136
EOS
Radioactivity, or radioactive decay, is the spontaneous change of the nuclei accompanied by the emission of subatomic particles and/or high-frequency electromagnetic radiation
Chapter 19: Nuclear Chemistry 3
Radioactivity andNuclear Equations
A nucleus with a specified number of protons and neutrons is a nuclide
The two sides of a nuclear equation must have the same totals of atomic numbers and mass numbers EOS
Together, protons and neutrons are called nucleons
C136
Mass number
Atomic number
Chapter 19: Nuclear Chemistry 4
Radioactive Decay Products
Effect of an electric field on particle emission:
EOS
Chapter 19: Nuclear Chemistry 5
Modes of Radioactive Decay
HeThU 42
23490
23892
Sum of mass numbers: 238 = 234 + 4
EOS
Sum of atomic numbers: 92 = 90 + 2
Chapter 19: Nuclear Chemistry 6
Types of Radioactive Decay
ePaTh 01
23491
23490 Beta Decay
00
23490
m23490 ThTh Gamma Decay
eMgAl 01
2612
2313 Positron Decay
EOS
TeeI 12552
01
12553 Electron Capture
Chapter 19: Nuclear Chemistry 7
Radioactive Elements
Most of the naturally occurring nuclides of the lighter elements have stable nuclei; they are not radioactive
Even though they are radioactive, many nuclides of high atomic number are found in natural sources
EOS
The half-life (t1/2) of a radioactive nuclide is the time required for one-half the nuclei in a sample of the nuclide to decay
Chapter 19: Nuclear Chemistry 8
Radioactive Decay Series
A series of radioactive decays beginning with a long-lived radioactive nuclide and ending with a nonradioactive one is called a radioactive decay series
EOS
Chapter 19: Nuclear Chemistry 9
Radioactive Decay Rates
The radioactive decay law states that the rate of disintegration of a radioactive nuclide, called the decay rate or activity, A, is directly proportional to the number of atoms present
Rate of Radioactive Decay = A = N
EOS
Radioactive decay is a first-order process. The decay constant, , is analogous to k in the rate of reaction
Chapter 19: Nuclear Chemistry 12
Radiocarbon Dating
Carbon-14 is formed at a nearly constant rate in the upper atmosphere by the bombardment of nitrogen-14 with neutrons from cosmic radiation
EOS
Carbon-14 in living matter decays by – emissions at a rate of about 15 disintegrations per minute per gram of carbon
The half-life for carbon-14 is 5730 years. This dating method works well if an object is between 5000 and 50,000 years old
Chapter 19: Nuclear Chemistry 13
Synthetic Nuclides
Rutherford, in 1919, was able to convert nitrogen-14 into oxygen-17 plus some extra protons by bombarding the nitrogen atoms with particles. This a naturally occurring form of oxygen and is not radioactive
EOS
Phosphorus-30 was the first synthetic radioactive nuclide
Chapter 19: Nuclear Chemistry 14
Transuranium Elements
In 1940, the first of the transuranium elements—elements with a Z > 92—was synthesized by bombarding uranium-238 nuclei with neutrons
EOS
PueNp
NpeU
UnU
23994
01
23993
23993
01
23992
23893
01
23892
Chapter 19: Nuclear Chemistry 15
Transuranium ElementsConsiderable energy must be imparted to a positive ion in order for it to overcome repulsion by a positively charged nucleus. A machine, called a charged-particle accelerator, or cyclotron, is capable of this process
EOS
Chapter 19: Nuclear Chemistry 16
Nuclear Stability
EOS
Stable, nonradioactive nuclei are found within the “belt of stability”
Chapter 19: Nuclear Chemistry 17
Energetics of Nuclear ReactionsWhile working out the details of the theory of special relativity, Einstein derived the equation for the equivalence of mass and energy: E = mc2
Nuclear energies are normally expressed in the unit MeV (megaelectronvolt): 1 u = 931.5 MeV
EOS
m = –0.0061 u or –5.7 MeV
Chapter 19: Nuclear Chemistry 18
Nuclear Binding EnergyThe energy released in forming a nucleus from its protons and neutrons is called the nuclear binding energy and is expressed as a positive quantity
EOS
This explains why there is a mass loss of 0.0304 u in the formation of a helium nucleus from the two protons and two neutrons which comprise it. This quantity is called the mass defect of the nucleus
Chapter 19: Nuclear Chemistry 21
Nuclear FissionThe breakup of a heavy nucleus into two lighter fragments is called nuclear fission
EOS
Chapter 19: Nuclear Chemistry 22
Nuclear Fission Reactions
A nuclear reactor is designed to tame the nuclear fission process so that energy is released in a controlled manner
EOS
When a nucleus undergoes fission, some mass is converted into energy; about 3.2 × 10–11 J or approximately 8 × 107 kJ/g
Chapter 19: Nuclear Chemistry 24
Nuclear Fusion
The process of combining light nuclei into a heavier one is called nuclear fusion
EOS
Fusion is much more difficult to accomplish than fission because, with fusion, the nuclei must be forced extremely close together
– accomplished in the uncontrolled fusion reactions of hydrogen bombs
Chapter 19: Nuclear Chemistry 25
A Fusion ReactorThis close approach requires that the nuclei have enormously high thermal energies (over 40,000,000 K)
EOS
Chapter 19: Nuclear Chemistry 26
Effect of Radiation on Matterparticles only dislodge electrons from atoms and are termed ionizing radiation
Electrons freed by ionizing radiation are called primary electrons
Some primary electrons are energetic enough to ionize other atoms and molecules, producing secondary electrons
EOS
Chapter 19: Nuclear Chemistry 27
Effects of Ionizing Radiation
EOS
Ionizing radiation can excite electrons to higher energy levels with the emission of electromagnetic radiation such as X rays and ultraviolet light
Chapter 19: Nuclear Chemistry 28
Radiation DetectorsOne of the simplest and oldest ways to detect ionizing radiation is to observe the clouding it produces on photographic film
EOS
The most familiar radiation detection device is the Geiger–Müller counter
Chapter 19: Nuclear Chemistry 30
Radiation Dosage1000 rem: Almost certain to cause death
450 rem: A short-term dose would kill 50% of a population within 30 days1 rem: A short-term dose would likely cause about 100 cases of cancer within 20 to 30 years for every 1 million people exposed130 mrem/y: The normal average background radiation dosage20 mrem: The typical dose in a chest X ray examination
EOS5 mrem/y: Result of nuclear power production
Chapter 19: Nuclear Chemistry 31
Approximate Stopping Distances
Materials vary in ability to block radiation
EOS
Chapter 19: Nuclear Chemistry 32
Medical Diagnosis and Therapy
Radioisotopes are widely used to diagnose various disorders: most have very short half-lives
Although ionizing radiation can induce cancer, it can also be used to treat cancer cells, which are destroyed more easily by radiation than are healthy, normal cells
EOS
In some instances, radioactive chemicals (called radiopharmaceuticals) can be ingested and allowed to find their own way to the targeted tissue
Chapter 19: Nuclear Chemistry 33
Radioactive TracersRadioactive nuclides can be used as radioactive tracers, and their atoms can be attached to other substances, which are then said to be “tagged”
EOS
These tracers can be used to:
– Detect leaks in underground piping systems
– Determine frictional wear in piston rings
– Determine the uptake of phosphorus and its distribution in plants
Chapter 19: Nuclear Chemistry 34
Summary of Concepts
• The five types of radioactive nuclides involve emission of alpha () particles, beta () particles, gamma () rays, positrons, and electron capture
• All known nuclides with Z > 83 are radioactive, and many of them occur naturally as members of four radioactive decay series
EOS
• In the formation of an atomic nucleus from its protons and neutrons, a quantity of mass is converted into energy