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Samarium 149

Samarium 149 is an indirect product of U-235 fission and has a very large neutron capture cross-section (about 42,000 barns). It does not decay since it is a stable isotope. In a typical nuclear reactor fueled with uranium-235, the presence of 149Sm as an indirect fission product is very important in the power operation of a nuclear reactor.

What is Samarium

Samarium is a naturally-occurring chemical element with atomic number 62, which means there are 62 protons and 62 electrons in the atomic structure. The chemical symbol for samarium is Sm. Samarium is a typical member of the lanthanide series, and it is a moderately hard silvery metal that readily oxidizes in air.

Samarium was first discovered in 1879 by the French chemist Paul Émile Lecoq de Boisbaudran. The name samarium is after the mineral samarskite from which it was isolated. Although classified as a rare earth element, samarium is the 40th most abundant element in the Earth’s crust and is more common than metals like tin.

Naturally occurring samarium consists of five stable isotopes, 144Sm (3.08%), 149Sm (13.82%), 150Sm (7.37%), 152Sm (26.74), 154Sm 22.74%), and two isotopes with very long half-life 147Sm (15.00%), 148Sm (11.25%). Therefore naturally-occurring samarium is slightly radioactive – about 128 Bq/g.

In the nuclear industry, especially natural and artificial samarium 149 has an important impact on the operation of a nuclear reactor. Samarium 149 has a very large neutron capture cross-section (about 42,000 barns). Since natural samarium contains about 14% of 149Sm, it can be used as an absorbing material in control rods.

Samarium 149 is also an indirect product of U-235 fission. It is important for physicists and reactor operators to understand the mechanisms that produce and remove samarium from the reactor to predict how the reactor will respond following changes in power level.

Table of Neutron Poisons
Table of Neutron Poisons

Samarium 149

samarium 149 - cross-section
Samarium – 149. Neutron capture and total cross-sections.
Source: JANIS (Java-based Nuclear Data Information Software); The JEFF-3.1.1 Nuclear Data Library

As was written, samarium 149 has a significant impact on the operation of a nuclear reactor. Samarium 149 is an indirect product of U-235 fission and has a very large neutron capture cross-section (about 42,000 barns). It does not decay since it is a stable isotope. Almost no samarium 149 results directly from fission (γSm =  10-12), but most comes from the decay chain, Nd-149 (β decay, 1.73 hr; γNd = 1.09%) to Pm-149 (β decay, 53.1 hr) to Sm-149 (stable). The instantaneous production rate of samarium-149 is dependent on the promethium-149 concentration and, therefore, on the local neutron flux history. On the other hand, the destruction rate of samarium-149 is also dependent on the instantaneous local neutron flux. Its significance is primarily caused by two factors:

  • its high capture cross-section, which is about 42,000 barns
  • its high total yield, which is about 1.08%

Neither the cross-section nor the yield is as big for this nuclide as for xenon 135, so the samarium reactivity effects are much smaller.

Table - yields - xenon, iodine, promethium
Table of total yields for various nuclei – thermal fission.

In a typical nuclear reactor fueled with uranium-235, the presence of 149Sm as an indirect fission product is very important in the power operation of a nuclear reactor. In contrast to xenon poisoning, at zero-power operation, the presence of 149Sm may not be neglected since its concentration is significant. Engineers and operators must perfectly know the behavior of a reactor with samarium. The presence of 149Sm is associated with the following operational issues:

  • Equilibrium Samarium
  • Response to Reactor Shutdown and Startup

To understand these issues, we must perfectly understand the production and removal of samarium 149.

Samarium Production and Removal

Samarium production and removalSamarium Production

Fission does not produce Sm 149 directly, and the fission yield of samarium 149 is nearly zero. Sm-149 is in the decay chain of the fission product neodymium 149, which decays to promethium 149. Because of the short half-life of Nd-149 (compared to the half-life of Pm-149), promethium may be considered as if it were formed directly from fission. The decay sequence is depicted in the figure.

Samarium Removal

An important difference between Xe-135 and Sm-149 is that samarium 149 is a stable isotope and remains in the core after shutdown. There are only two ways of samarium removal, and one of these processes is the samarium burn up when the reactor is at power operation. The rate of samarium burnup is dependent upon the neutron flux and the samarium 149 concentration (i.e., the reaction rate).

The second process is associated with refueling. During refueling, one-third or one-quarter of the core is usually removed from the spent fuel pool and replaced by fresh fuel assemblies. At the same time, the remainder is rearranged to a location in the core better suited to its remaining level of enrichment. Therefore refueling naturally leads to a decrease in the overall samarium content in the core.

Samarium 149 – Differential Equations

Assuming that fission does not produce Sm 149 directly and neglects the small amount of promethium burnup, the situation is described as follows. The production and removal of samarium can be characterized by the following differential equations.

samarium - differential equations

Samarium Equilibrium – Promethium Equilibrium

When the rate of production of promethium equals the rate of removal of promethium, equilibrium exists. This equilibrium is also known as “samarium 149 reservoir” since all of this promethium must undergo decay to samarium. The promethium concentration remains constant and is designated NPm(eq) in equilibrium. The following equation for the promethium equilibrium concentration can be determined from the preceding equation by setting the dNPm/dt =0.

promethium equilibrium - equation

Since the equilibrium promethium concentration is proportional to the fission reaction rate, it is also proportional to the reactor power level.

When the production rate of samarium equals the rate of removal, equilibrium also exists for samarium. The samarium concentration remains constant and is designated NSm(eq). The following equation for the samarium equilibrium concentration can be determined from the preceding equation by setting the dNSm/dt =0. For samarium to be in equilibrium, promethium must also be in equilibrium. Substituting the expression for equilibrium promethium concentration into the equation for equilibrium samarium results in the following equation:

samarium equilibrium - equation

This expression for equilibrium samarium 149 concentration during reactor operation illustrates that equilibrium samarium 149 concentration is independent of neutron flux and power level. It follows the time of saturation is dependent upon the neutron flux level. The equilibrium concentration usually produces negative reactivity (samarium worth) of about -600 pcm.

Response to Reactor Shutdown and Startup

After reactor shutdown, the neutron flux drops to zero, and there remains no channel of removal of samarium. On the other hand, a significant amount of accumulated promethium decays to samarium; therefore, the concentration of samarium increases to a new level. This buildup depends on the neutron flux level before the shutdown(i.e., upon the promethium equilibrium).

The new equilibrium is reached in approximately 20 days, and since samarium 149 is stable, the concentration remains constant during reactor outage. As shown in the figure, samarium 149 does not peak as xenon-135 does but increases slowly to a maximum value. As was written, samarium can be removed from the core by refueling. During refueling, one-third or one-quarter of the core is usually removed from the spent fuel pool and replaced by fresh fuel assemblies (without samarium). At the same time, the remainder is rearranged to a location in the core better suited to its remaining level of enrichment. Therefore refueling naturally leads to a decrease in the overall samarium content in the core.

After reactor startup, samarium concentration usually decreases due to samarium burnup and very slow decay of promethium. Similarly, transient changes in samarium on power level changes are very small compared to xenon and change very slowly over a week. In each case, the samarium level returns to the same equilibrium value.

Although samarium-149 has a constant poisoning effect during long-term sustained operation, its behavior during initial startup and post-shutdown and restart periods require special reactor design considerations.

samarium equilibrium

It was written that the samarium equilibrium is independent of the neutron flux level; therefore, stationary samarium worth is also independent. Note that the promethium equilibrium, which determines especially the samarium peak concentration after shutdown, is flux dependent! The reactor shutdown must be considered in estimated critical conditions calculations, and it can influence MTC at the beginning of the next cycle.

Moreover, especially high flux research reactors must not be shut down suddenly. Sudden shutdown of a reactor with a thermal flux of about 1019 neutrons/cm-2.s-1 can cause more than thirty times higher samarium poisoning than PWRs. This can cause permanent poisoning and preclude any reactor startup. These reactors must lower the reactor power gradually to burn off as much samarium 149 as possible before shutdown.

Special reference: Paul Reuss, Neutron Physics. EDP Sciences, 2008. ISBN: 978-2759800414.

 
References:
Nuclear and Reactor Physics:
  1. J. R. Lamarsh, Introduction to Nuclear Reactor Theory, 2nd ed., Addison-Wesley, Reading, MA (1983).
  2. J. R. Lamarsh, A. J. Baratta, Introduction to Nuclear Engineering, 3d ed., Prentice-Hall, 2001, ISBN: 0-201-82498-1.
  3. W. M. Stacey, Nuclear Reactor Physics, John Wiley & Sons, 2001, ISBN: 0- 471-39127-1.
  4. Glasstone, Sesonske. Nuclear Reactor Engineering: Reactor Systems Engineering, Springer; 4th edition, 1994, ISBN: 978-0412985317
  5. W.S.C. Williams. Nuclear and Particle Physics. Clarendon Press; 1 edition, 1991, ISBN: 978-0198520467
  6. G.R.Keepin. Physics of Nuclear Kinetics. Addison-Wesley Pub. Co; 1st edition, 1965
  7. Robert Reed Burn, Introduction to Nuclear Reactor Operation, 1988.
  8. U.S. Department of Energy, Nuclear Physics and Reactor Theory. DOE Fundamentals Handbook, Volume 1 and 2. January 1993.
  9. Paul Reuss, Neutron Physics. EDP Sciences, 2008. ISBN: 978-2759800414.

Advanced Reactor Physics:

  1. K. O. Ott, W. A. Bezella, Introductory Nuclear Reactor Statics, American Nuclear Society, Revised edition (1989), 1989, ISBN: 0-894-48033-2.
  2. K. O. Ott, R. J. Neuhold, Introductory Nuclear Reactor Dynamics, American Nuclear Society, 1985, ISBN: 0-894-48029-4.
  3. D. L. Hetrick, Dynamics of Nuclear Reactors, American Nuclear Society, 1993, ISBN: 0-894-48453-2. 
  4. E. E. Lewis, W. F. Miller, Computational Methods of Neutron Transport, American Nuclear Society, 1993, ISBN: 0-894-48452-4.

See above:

Reactor Operation