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(S-8) Nuclear Power


    Note: This is a side-excursion into the basics of nuclear energy, beyond the main scope of "from Stargazers to Starships." It is included because nuclear energy is important to modern society, and because section S-7 "The Energy of the Sun" has already provided many of the basic ideas. Bear in mind that even without math, this can be a fairly difficult subject and that the discussion is rather lengthy.


    Index

S-2.Solar Layers

S-3.The Magnetic Sun

S-3A. Interplanetary
        Magnetic Fields

S-4. Colors of Sunlight

S-4A.Color Expts.

S-5.Waves & Photons

Optional: Quantum Physics

Q1.Quantum Physics

Q2. Atoms   (and 6 more) --------------------------

S-6.The X-ray Sun

S-7.The Sun's Energy

S-7A. The Black Hole at
        our Galactic Center

LS-7A. Discovery
      of Atoms and Nuclei

S-8.Nuclear Power

S-9.Nuclear Weapons

    The ideas from section S-7 are reviewed in what follows next. The rest of the section is a qualitative discussion of all key processes involved in the practical use nuclear energy.

A Review of Nuclear Structure

    The way the Sun generates its energy helps understand the way a nuclear power station does so. The two processes are however quite different.

Here some facts about the way protons and neutrons combine to form nuclei, as covered in section S-7 about the Sun:

  1.   Apart from their electrical charge, protons and neutrons ("nucleons") are quite similar. They can attract other nucleons and combine with them to form heavier nuclei, a process which releases energy. For instance, on the Sun pairs of protons combine with pairs of neutrons to form helium nuclei. In the process atomic particles gain great speed, and that is how the Sun's heat is generated.


  •   Unlike gravity or electrical forces, the nuclear force is effective only at very short distances. At greater distances, the protons repel each other because they are positively charged, and charges of the same kind repel.

      For that reason, the protons forming the nuclei of ordinary hydrogen--for instance, in a balloon filled with hydrogen--do not combine to form helium (a process which also would require some to combine with electrons and become neutrons). They cannot get close enough for the nuclear force, which attracts them to each other, to become important! Only in the core of the Sun, under extreme pressure and temperature, can such a process take place.

  •   Other small nuclei can similarly combine into bigger ones and release energy, but in combining such nuclei, the amount of energy released is much smaller. The reason is that while the process gains energy from letting the nuclear attraction do its work, it has to invest energy to force together positively charged protons, which also repel each other with their electric charge.

  •   Once iron is reached--a nucleus with 26 protons--this process no longer gains energy (nickel also has peak binding energy). In even heavier nuclei, we find energy is lost, not gained by adding protons. Overcoming the electric repulsion (which affects all protons in the nucleus) requires more energy than what is released by the nuclear attraction (effective mainly between close neighbors). Energy could actually by gained, however, by breaking apart nuclei heavier than iron.

  •   In the biggest nuclei (elements heavier than lead), the electric repulsion is so strong that some of them spontaneously eject positive fragments--usually nuclei of helium, which form very stable combinations ("alpha particles"). This spontaneous break-up is one of the forms of radioactivity found in nuclei.

  •   Nuclei heavier than uranium break up too quickly to be found in nature, although they can be produced artificially. The heavier they are, the faster is their spontaneous decay.

        In summary, then: iron or nickel nuclei are the most stable ones, and the best sources of energy are therefore nuclei as far removed from iron as possible. One can combine the lightest ones--nuclei of hydrogen (protons)--to form nuclei of helium, and that is how the Sun gets its energy. Or else one can break up the heaviest ones--nuclei of uranium--into smaller fragments, and that is what nuclear power companies do.

    How many Protons, how many Neutrons?

        As already noted, protons and neutrons (jointly called "nucleons") are intrinsically similar, and can convert into each other, absorbing or emitting an electron to maintain proper electric charge. What determines how many of each are found in a nucleus?

        The nuclear forces apparently prefer equal numbers of each kind, and light nuclei--helium, carbon, nitrogen, oxygen--usually maintain a 50:50 ratio, although nuclear variants ("isotopes") with small deviations from equality may exist and may be stable.

        In heavier nuclei, because of the electric repulsion between protons, this equality no longer holds. Imagine a nucleus with 56 nucleons, and suppose we could choose how many of this total would be neutrons and how many protons. What would be the most stable combination?

        Choosing 28 of each kind might provide the most stable nuclear binding, but that is offset by the energy required to hold in close quarters 28 positive protons. So nature compromises: the preferred combination--the nucleus of the most common form of iron--has 30 neutrons but only 26 protons.

        As nuclei get heavier, the fraction of protons drops still further--about 45% in mid-range nuclei, and less than 40% in the heaviest ones, those of uranium. Ordinary uranium ("U-238") has 92 protons but 146 neutrons, for a total of 238 nucleons. As will be seen, this gradual change in the proton/neutron ratio is essential to the nuclear chain reaction.
       

    Nuclear Fission

        Uranium nuclei in nature are unstable. Each of their 92 protons repels the rest, and sooner or later (half of them within 4.5 billion years) they eject a positive fragment, an "alpha particle" which is another term for a rapidly moving nucleus of helium. Almost all the helium atoms we extract from natural gas and from rocks--for filling balloons and for other uses--were originally created as alpha particles.

        But there exists a way of speeding up this break-up, by exposing the material to free neutrons.

          Free neutrons are not found in nature (they would decay into protons and electrons), but they can be released from atoms of beryllium by bombarding them with alpha particles from radioactive materials, or by other methods. Since they are only attracted by nuclei (while protons are repelled before they get close enough for the nuclear attraction to do its job), they can easily enter a nucleus and stick to it--a bit like small magnets clicking onto a chunk of steel.

          Such an attraction releases energy. If the nucleus is heavy and unstable, like that of uranium, adding energy destabilizes it even more, to where it may break up immediately. The interesting thing about such a break-up is the spectacular way in which it sometimes happens, as was discovered by Hahn and Meitner in 1939. Instead of breaking off a little chip, a helium nucleus containing less than 2% of the mass, the entire nucleus splits into 2 comparable fragments, typically containing 1/3 and 2/3 of the mass.

          This process is called nuclear fission and besides the speed with which it can take place, it has at least two other remarkable features:

    1.   It releases much more energy then the chipping-off of a helium nucleus ("alpha radioactivity").
    2.   The fragments themselves are unstable. If you break up a nucleus which has (say) 40 protons for every 60 neutrons, into fragments whose optimal ratio is only (say) 45 to 55, there is bound to be some adjustment.

        Ordinarily, such an adjustment calls for the conversion of some neutrons into protons (plus emitted electrons, "beta rays"), a process known as "beta radioactivity." Such an adjustment does in fact occur, making such fragments fiercely radioactive, and turning their disposal into a major issue for the nuclear power industry.

        But at first, when the nucleus breaks up, the fragments are too unstable for such a gradual process. A quicker adjustment is needed, and the fragments achieve it by each emitting one or sometimes more free neutrons.

    The Chain Reaction

        On the average, about two neutrons are released this way per fission event. But it takes only one neutron to initiate another fission! Thus if fissionable nuclei are so densely packed that each neutron is bound to produce a new fission, the number of fission events quickly multiplies: 2, 4, 8, 16, 32, 64, 128... Since the energy release is proportional to the rate of fission, it also grows--very quickly!

        This chain reaction is what makes a nuclear bomb (or "atomic bomb") function. The material with nuclei prone for fission--usually plutonium, an artificial heavy elements with 94 protons--must be compressed tightly and at the appropriate moment, exposed to a blast of neutrons. A variety of tricks, all of them top secret, is used to make sure that at least an appreciable fraction of its atoms undergoes fission before the whole thing blows apart.

        Commercial nuclear power is produced somewhat differently, in a more controlled fashion. The fuel is uranium 235 (U-235)--a variant ("isotope") with 92 protons but only 143 neutrons, not 146, an odd number which makes it less stable. Natural uranium consists mostly of U-238, and it can absorb a neutron without undergoing fission (it ultimately turns into plutonium). U-238 therefore will not support a chain reaction. However, 0.7% of uranium is U-235, which can fission as soon as it absorbs a neutron.

          By using a clever design, one can actually build a reactor fueled by natural uranium. The trick is to form the fuel into rods, and put between them some material ("moderator") which slows down neutrons but does not absorb them, e.g. pure carbon or "heavy water" containing the heavy isotope of hydrogen. Neutrons produced in a rod generally escape into the moderator, and by the time they hit another rod, they are moving very slowly: such slow neutrons are gobbled up much more avidly by U-235 than by U-238, so that even in a rod containing only 0.7% U-235, the U-235 atoms make most of the "catches. "

      The Critical Mass

        It should be added that many neutrons are also lost--escaping from the edges of the reactor into the surrounding material, or being absorbed inside it by the " wrong " nuclei, the ones which do not undergo fission. In fact, a reactor needs to be carefully designed to sustain a chain reaction in the first place: but it can be done.

        From the beginning, complex and very expensive methods were devised to separate U-235 or to enrich its percentage past 0.7%. Today many (though not all) commercial power reactors use enriched fuel, which makes the design of reactors easier and more controllable. With enriched fuel, ordinary water can serve as moderator, and it is even feasible to combine moderator and fuel, dissolving some uranium compound in water which acts both as moderator and as a distributor of heat. Canada's "CANDU" power reactors use ordinary uranium, but because ordinary water may absorb some neutrons, it is surrounded by "heavy" water (whose hydrogen is replaced by its heavy isotope, deuterium).

        Such a reactor--or a chunk of plutonium--will not support a chain reaction if it is too small. If the amount of fissionable material is less than a critical mass, the average fission occurs too close to the surface. Even though (say) 2 neutrons are produced in each fission, on the average 1.2 of them escape to the outside before hitting another nucleus, leaving only 0.8 neutrons to continue the process, whereas one or more are needed.

        When processing nuclear fuel, or reprocessing fuel rods, it is therefore essential to work only with small quantities to prevent any accidental chain reaction. On 30 September 1999, at the nuclear processing plant in Tokaimura, Japan, workers thought they would save time by combining several batches of a solution of uranium. With a flash of blue light, a chain reaction began, giving three workers very bad doses of radiation and lasting 18 hours. After 3 months one worker died (in spite of extreme measures), one was discharged from the hospital and one is still (as of 12/99) in intensive care.

        A detailed report on the accident ("What Happened in Tokaimura?") appeared in "Physics Today", December 1999, p. 52-4. A similar accident occured in the US in the 1950s, when a worker extracting plutonium from a solution in one liquid into another took a shortcut and combined several batches. He died of radiation exposure within two days.

          [A note about history: The first nuclear reactor was designed by Enrico Fermi and was built under the stands of an old stadium at the University of Chicago. Rather than rods, it used cylindrical pellets of uranium, and these were embedded in a big "pile" of bricks of pure carbon, the moderator. It achieved a self-sustaining chain reaction on 2 December, 1942, and the name "atomic pile" for a nuclear reactor remained in use for about a decade afterwards. ]

    The Controlled Nuclear Reactor

        Because a nuclear reactor requires neutrons that have slowed down, it has a built-in delay and cannot explode like a nuclear bomb (even if scary films claim otherwise). Still, the chain reaction can grow very rapidly, and unless it is controlled, the reactor could in principle heat up to where it melts down. The usual method of control is to insert among the fuel "control rods" which strongly aborb neutrons--e.g. of the metal cadmium, also used in electroplating. By absorbing free neutrons, these rods slow down or stop the chain reaction.

        Fortunately, nature has been helpful here. About 1% of the neutrons released in fission are not emitted promptly but are delayed, by a fraction of a second. Reactors are always operated to produce just barely enough neutrons to sustain a chain reaction. If for some reason the heat output starts to rise, the delayed neutrons slow down the rate of increase to where an automatic mechanism lowering or raising the control rods is fast enough to stop it.

        Power reactors in the US use ordinary water as a moderator, inside a "pressure vessel" made of thick steel, with rod-like fuel elements and control rods fitted through openings in its lid. To start the chain reaction

    • the control rods are withdrawn part of the way,
    • the fast fission fragments heat the fuel elements,
    • the fuel elements heat the water, steam is produced (usually, "clean" steam in pipes separated from the radioactive reactor water), the steam turns turbines,
          and
    • generators attached to the turbines produce electricity.
    That is the basic process --the details are many and much more complicated.

        Is this the energy of the future? As of this writing (1999) France gets 75% of its electric energy from nuclear power, and many industrial countries, short on coal and oil, also obtain an appreciable fraction of their energy this way--e.g. 1/3 of the energy used in Japan and Spain. In the US, after an enthusiastic start, the use of nuclear power has leveled off to about 20% of the power generated, mainly due to public resistance to nuclear energy.

        The US however is fortunate in having large reserves of coal: its growing energy consumption is largely met by these fuels. Environmentally, the choice is between two alternatives:

    •   Burning coal and natural gas, which produces carbon dioxide (CO2) and other pollutants, and which may therefore amplifies the "greenhouse effect" and accelerate global warming; or else
    •   Using nuclear power stations, with the associated production of nuclear waste.

        It is not easy to choose, and if we reject both options, we can expect much higher power costs and much less available power.

    Nuclear Waste

        The trouble with fission power is that the "fission fragments" from the break-up of uranium or plutonium are very "hot, " extremely radioactive. This creates two serious problems:

    1.   The problem of waste storage, arising from the long "lifetime" of these substances, the time over which their activity persists.

          Nuclear waste contains a wide range of substances. Some have short lifetimes: their radioactivity is intense, but it "burns out" after hours, days, weeks or months (their hazard is different--see further below). However, some waste substances stay "hot" (radioactive) for decades and centuries, and their radioactivity is still so intense that they need to be kept away from human contact for a thousand years, maybe several thousand. At least initially, nuclear wastes also need to be cooled, because their radioactivity still generates heat.

          It has been proposed to cast nuclear waste into a glassy slag and isolate it in underground caverns, but fears remain--no human activity in past history has required such an unfailing long-term commitment (toxic chemicals also may do so, if they are buried instead of destroyed). Luckily, the amount of nuclear wastes is relatively small. As waste products of nuclear fuel, they have about the same weight as the fuel itself, of which a few tons can supply a city with electricity for years.
          Still, they must be handled by remote control, and must have no chance to contaminate ground water.

    2.   The possibility of reactor meltdown. In the regular operation of a nuclear power station, fuel rods accumulate an appreciable amount of fission fragments. On a rotating schedule, each rod is replaced with a new one and its radioactive waste is removed and stored; but at any time, the rods contain enough of such waste to generate a lot of heat--enough, in fact, to melt the rod itself, if for some reason the flow of steam (or hot water) which removes its heat were to fail.

    Nuclear Accidents

        Suppose something went wrong with the cooling mechanism. Automatically, of course, control rods are lowered and any chain reaction stops immediately. But the radioactive waste in the reactor core continues to generate heat, so that cooling must still be provided for some hours, if not days. On 28 March 1979, at the nuclear power station at Three Mile Island, outside Harrisburg, Pennsylvania, a minor malfunction led to a series of errors, shutting down for a while both the main and emergency cooling systems.

        The residual heat of the nuclear wastes melted part of the core and created (by chemical reaction) free hydrogen, which further complicated the situation. The billion-dollar reactor was a total loss, but the worst damage was probably to the public's trust in the safety of nuclear power. Still, the reactor vessel was not breached, and the second line of defense, the heavy concrete "containment building" inside which it was housed, also remained intact.

        The power reactor at Chernobyl, near Kiev, capital of the Ukraine, had a different design--like Fermi's original reactor, it used a pile of carbon (graphite) to slow down neutrons, with pipes inside it carrying the fuel rods, control rods and cooling water. It was a big reactor, and was not enclosed in a containment building.

        On 25 April 1986, an unwise engineering experiment at low power got out of control. The power level surged, the reactor vessel burst, and the hot steam and graphite (as well as combustible zirconium metal used in the fuel rods) reacted with hot steam and with oxygen of the atmosphere to produce an intense fire, whose plume rose to high altitudes and spread radioactive debris over a wide area. Of the fire-fighters called to extinguish the fire, many later died from radiation. Towns and villages near Chernobyl had to be evacuated (they remain empty as of 1999) and agricultural produce over much of Europe was contaminated. The remains of the reactor were later encased in a thick cover of concrete, entombing the radioactive waste left inside it.

        Since these accidents, nuclear power generation in the US has proceeded without any major mishap. However, nuclear waste is still kept in temporary storage, as the national policy for its treatment and disposal continues to be debated. The other reactor at at Three Mile Island (and even the ones at Chernobyl) have been restarted to supply power again.     An overview of "Nuclear Power Damage in Japan in the Earthquake of 3/2011" from The Washington Post, 3-12-2011 is linked here.

        As the example of France suggests, nuclear power can be the main energy source of an industrial nation, though it calls for a high level of professional competence and carefully designed safety features. At the same time, the accidents at Three Mile Island and Chernobyl are a reminder that this power source carries unique risks of its own.

    Further Exploring

        If you have the time and the motivation, an enormous number of sources can give you more detailed information about matters discussed here, both in print and on the web. There is, for instance, "The Virtual Nuclear Tourist", a very detailed overview of the nuclear power industry.

        Twenty five years after the accident at Three Mile Island, J. Samuel Walker, a historian with the Nuclear Regulatory Commission, published "Three Mile Island: A Nuclear Crisis in Historical Perspective (315 pp, $24.94, U. Calif Press, Berkeley, 2004). Its review is found in "Science,"vol. 305, p. 181, 9 July 2004.

        Another rich source of information (also covering nuclear weapons) is the book "Megawatts and Megatons: A Turning Point in the Nuclear Age?" by Richard L. Garwin and Georges Charpak, 431 pp, $30, Knopf, New York, 2001.

        A shorter, 4 page summary of nuclear power (comparable to this web page) is "Nuclear Fission: Atoms Unleashed", the center feature section ("Inside Science #157") betw. p. 28-9 in New Scientist, 18 January 2003.


    Questions from Users:                 *** Gases that fill balloons
                                        *** Nuclear reactors and bombs
                                  *** Ionizing Radiation and the origin of Life
                            *** Radiation risks from uranium counterweights

      •     Nuclear power unfortunately also provides some most destructive weapons.
        To learn more about those, see the attached section Nuclear Weapons

    "From Stargazers to Starships" continues with sections dealing with spaceflight and spacecraft, starting with The Principle of the Rocket

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    Author and Curator:   Dr. David P. Stern
         Mail to Dr.Stern:   stargaze("at" symbol)phy6.org .

    Last updated: 11-15-2004
    Re-formatted 27 March 2006