Lecture XVI

Physics 367

Safety and Nuclear Energy



Three Mile Island


Three Mile Island in 1999.

Three Mile Island 900 MWe Pressurized Water Reactor.

High-pressure and high-temperature Water isolated in a closed reactor loop heats water in the secondary system to produce steam to turn a turbine.

The apparatus used to transfer this energy is called a heat exchanger. These devices use a lot of water to circulate to carry thermal energy from one place within the reactor to another.

In case of emergency shutdowns [SCRAMs], the reactors built in the United States have an emergency core cooling system [ECCS], which involves pumping large amounts of water into a reactor core that is heating too fast.

designs of that era had (1)lots of pumps, valves, and water pipes in the nuclear reactor operated from a control room and (2)vast arrays of control dials and other indicators showing conditions in the plant in the control room.


The sequence of the Three Mile Island accident on 28 March 1979 occurred this way [refer to the discussion in Ch. 18 of Energy].

During routine maintenance of the steam generator side of the heat exchanger two weeks before the accident, 2 valves in auxiliary feedwater pumps were manually closed and then inadvertently left closed.

The incident began when a feedwater pump to the heat exchanger failed. The loss of feedwater caused the primary system to overheat causing the primary system pressure to increase. The backup systems did not begin immediately [by design], and a SCRAM occurred. The pressure relief valve opened to release excess pressure buildup. All this happened as designed by safety engineers.

The three backup feedwater pumps, however, were disabled by the closed valves, and so did not kick in after the built-in 15 second delay.

The pressure relief valve stayed open long enough to lower the pressure; at that point the relief valve should have closed. The valve stuck, and failed to close. This was not noticed by the operators for 2 1/2 hours.


The emergency core cooling system turned on by design as the pressure dropped too low, but the operators thought that the ECCS had turned on by mistake and manually turned the ECCS off. This leads to an uncovered core as water boils away and escapes through the stuck relief valve.

The operators saw the core cooling still as the steam escapes, so they mistakenly turned off the water pumps to the core, thinking that would push the temperature back up. This made the accident much worse. The core was uncovered for 13.5 hours.

The liquid released by the stuck valve ruptured a holding tank seal, ultimately spilling 400,000 gallons of radioactive water onto containment vessel floor!.

A bubble of hydrogen from water that endothermically broke up was in the core during the accident. The hydrogen could have exploded--chemically--but did not.

The final toll:
15-30% of the core was uncovered
45% of the core melted
70% of the core was damaged
20 tonnes of debris fell to the bottom of the reactor
large amount of radioactivity released [1.1 x 1012 Bq]

Summary: human error was the main cause; mechanical failure was important.

Some important lessons about the design of control rooms were learned by power plant managers.


Chernobyl


Chernobyl in 1997.

The Chernobyl disaster was much greater than at Three Mile Island. Here, too, human error was the cause.

Part of the problem was in the design of the Russian RBMK reactors, especially the effective lack of a containment vessel and the choice that graphite was used as the moderator.

What started as a reasonable test of the use of turbine generators as source of emergency power for the computers essential to control turned into a nightmare as repeated operator mistakes amplified the design flaws. No one will build this design again. Rehearsing the scenario is unfruitful.


The sequence of events during the accident on 25 April 1986 occurred this way [also refer to the discussion in Ch. 18 of Energy].

The operators wanted to test the reactor by turning the power down slowly. They reduced power to 1/2.

The power grid was short of energy relative to demand, so the shutdown was delayed for many hours. When the shutdown was recommenced, the power level plunged. This wouldn't do for the experiment, so the engineers switched off the turbine to stop power drain but this also turned off the ECCS! This was in direct violation of regulations.

The shutdown was also stopped, a violation of operating protocol.

The power still fell, so all control rods were pulled. Recall that control rods are inserted into the reactor to absorb neutrons.

The drop slowed, and the control rods were pulled out farther.

The operator blocked the emergency valves to prevent the water from carrying away the heat. This was truly crazy.

A few seconds later...BOOM!

A graphite fire broke out, and continued. It carried radioactivity upward by convection.

The final toll:
31 people died in the accident.
Total destruction of the reactor.
Radioactivity released over northern hemisphere [2 x 1017 Bq].


Recommendations for change

The worst problems in nuclear power facilities are in the machinery, structure, and piping. These can generally be dealt with before they will cause problems by intelligent design, retrofitting when problems with a design are discovered, and maintenance. Human errors and unforeseen catastrophes cannot be planned for directly. The role of human error is clear in both accidents. We were our own worst enemy

What was done?

The control rooms of new plants were redesigned to impart information and reduce the information overload for the operators. This is one good consequence of the accidents.

Computers will be used much more in the control rooms, decreasing the number of dials the operators must watch, and allowing them access to relevant information about a problem.

The role of redundancy was clear before the accidents, but the continued training of operators was neglected. Also, there were no mechanisms to allow operators to learn from accidents or near accidents in other reactors. Such an information exchange is now in place.


Should we panic?

The important thing to do is to see what the consequences actually are in comparison to other risks in life. No option is without risk. People use cars despite the fact that there are over

-50,000 deaths per year in the U.S. alone from auto accidents.
-Falls account for 18,000 deaths.
-Fires for 9,000.
-Drowning for 6,000.
-Other accidents for another 30,000.
-Cancer alone claims 300,000 per year.

Estimates of mortality from coal from all causes range around 6,000 to 10,000--about 30--50 deaths overall for each of the 200 coal plants in the U.S. In nuclear, perhaps there are 200 to 800 or so deaths per year, mostly in construction and mining. The net mortality from TMI was 0; from Chernobyl 31.


Nuclear Fusion

The binding energy curve shows that nucleons can fall deeper into the nuclear ``well'' in two circumstances--when a large nucleus breaks up or fissions into two smaller nuclei, and when two nuclei smaller in mass than combine into a larger nucleus with mass that is still smaller than that of .



If we look at the binding energy per nucleon of helium-4 [] we find it is much larger than that for helium-3 [], tritium [], or lithium-5 []. Helium-4 is much more stable for some reason. In fact, it might even be possible that would exist inside a nucleus, because the average binding energy is so large. If so, one might expect that the helium-4 nucleus could ``leak out'' from the parent nucleus. This does happen: the helium-4 nucleus is called an alpha-particle []. These -particles are the source of the alpha-rays observed in radioactive decays.


Fusion can only occur when the nucleons get close enough together so that the attractive strong nuclear force is stronger than the repulsive electric force between the protons in the nuclei that combine. This means that the nucleons must get within about 1 fm of each other, because the strong nuclear force does not extend beyond this distance.

To get a nuclear fusion reaction to start it is necessary to give the nuclei enough energy to come close together. The energy provided to start the fusion reaction going is called the nuclear activation energy.

There are several ways that have been considered to achieve this necessary closeness. Thermonuclear fusion works by giving the atoms of material to be fused a very high kinetic energy by increasing the temperature. The sun and other stars are examples of thermonuclear fusion. The temperature in the sun's interior is about 10 MK. When temperatures are this high, there is enough energy to rip off all the electrons from the atoms and produce a plasma. Plasma is ionized matter containing equal amounts of positive and negative charges. Most material in the universe is plasma.



A schematic of a Tokamak.

On Earth, plasma must be contained within a small region to allow fusion to occur. It is necessary to keep the plasma from touching any walls of a container. Even if the container were made of cardboard rather than metal, it would not be vaporized by contact. The plasma would lose all its energy instead. Magnetic fields are used for this purpose in Tokamaks.

Two other published methods involve focusing of energy on small pellets called ``microballoons'' containing the material to be fused. In laser fusion, the beam of a powerful laser is broken into 32 parts, and all are focused simultaneously on a pellet from all sides. This causes an implosion of the microballoon that pushes the nuclei close enough together to cause fusion. In inertial fusion, accelerators make beams of particles. As in laser fusion, the beams hit the microballoon from all sides and initiate fusion through the collapse of the microballoon, which pushes the reactants close together.

To get net energy out from one of these methods, the reaction must produce more energy than is needed to supply the activation energy. This is needed to create the plasma and bring the plasma to high temperature in the case of thermonuclear fusion. It is the energy needed to run the laser in laser fusion. It is the energy needed to produce the beams of particles in inertial fusion.


Example - deuterium fusion.

In deuterium fusion, two deuterium nuclei combine to produce helium-3. The reaction is

+ + n

The average binding energy per nucleon is:

deuterium = 1.1 MeV
helium-3 = 2.8 MeV
neutron = 0 MeV

The total binding energy is:

deuterium = 2(1.1 MeV) = 2.2 MeV
deuterium = 2(1.1 MeV) = 2.2 MeV
helium-3 = 3(2.8 MeV) = 8.4 MeV

The total energy released from the fusion of two deuterium nuclei into helium-3 is thus the difference between the amount of energy given up by the nucleons to form helium-3 minus the amount they had already given up to be part of the deuterium nuclei:

8.4 MeV - 2.2 MeV - 2.2 MeV = 4.0 MeV.

This is less than the energy from fission, but it involves combination of much smaller masses. However, the amount of energy per mass is much greater. The amount of energy released per unit of mass of the fusion reactants is

(4.0 MeV)(1.6 x 10-19 J/eV)/(4 amu)(1.66 x 10-27 kg/amu)
= 9.6 x 1012 J/kg.


The energy from fusion in general appears as kinetic energy of the nucleus and the protons, neutrons, and/or electrons produced, as well as as -radiation and neutrinos. Because the forces holding the nuclei together are so strong, this is a lot of energy. There is about 2.8 x 105 times as much energy available from the fission of a deuterium nucleus as from the burning of a carbon atom [33.8 MJ/kg] and thus there is plenty of deuterium available in the oceans to provide virtually unlimited energy for generations to come.

A coal-fired plant [1000MW] uses 100 kg of coal/s or 8,640,000 kg/day.

A fission power reactor [1000MW] uses ~3 kg of uranium-235 per day.

A fusion power plant [1000MW] would use 1 kg of deuterium per day. To produce this amount of energy almost 1019 fusions/sec must take place.


Sustained Fusion

In general to sustain fusion the Lawson criterion must be satisfied:

(density)x(confinement time) > 6x1019 m-3s

This criteria has been met in research reactors. However in order to construct a working fusion power plant the energy out must exceed the total energy put in. At present it is not understood how to accomplish this. As a result engineers cannot yet design a working fusion power plant. The figure below indicates the history of fusion research and where the research stands relative to the expected parameters of a working fusion power plant.


Nucleosynthesis

Since the nuclei formed up to iron-56 are more stable than lower-A nuclei, we expect that these will be formed in stars. As we saw, fusion occurs in stars' interiors. In our sun, only helium fusion is possible. In more massive stars, elements up to iron-56 can be made.

How do we get more massive elements?

The answer is that they come from endothermic nuclear reactions rather than from exothermic nuclear reactions. When a star has burned all of its fuel into the various elements, the fire blanks suddenly. The outer part of the star is no longer suspended by the fire inside. The whole outer part of the star falls in because of gravity, and the energy of that in falling mass causes a tremendous implosion, immediately followed by a tremendous explosion. Such an event is a supernova.

This ejects most of the star's matter. During the implosion phase, energy can be transformed from gravitational energy to other forms of energy. In particular, heavy elements are fused from lighter constituents. This material was part of the cloud that eventually formed our sun and the solar system. It is for this reason that one can either say that we all contain a little stardust, or that we are all made of interstellar garbage.