Skip to main content

Neutron Physics Background

  • Chapter
  • First Online:

Abstract

This chapter introduces fundamental properties of the neutron. It covers reactions induced by neutrons, nuclear fission, slowing down of neutrons in infinite media, diffusion theory, the few-group approximation, point kinetics, and fission product poisoning. It emphasizes the nuclear physics bases of reactor design and its relationship to reactor engineering problems.

This is a preview of subscription content, log in via an institution.

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   129.00
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Notes

  1. 1.

    You can get the data from http://ie.lbl.gov/toimass.html

  2. 2.

    The speed of neutrons in a reactor is sufficiently low that one can neglect relativistic effects therefore m = m 0, the neutron rest mass (1.6748 × 10−27 kg).

  3. 3.

    FEMP computer code has been developed by Professor Patrick McDaniel of University of New Mexico, Nuclear Engineering Department.

  4. 4.

    This effort was taken in place under contract by McDaniel and Zohuri in time period of 2001–2003 but never was a finished effort, although a lot of work was put into it and somewhat a new modified version NJOY with recoil capability was developed.

  5. 5.

    One can calculate the total binding energy of a nucleus from the mass defect, Δm which is the difference between the mass of the bound nucleus and the sum of the masses of the nucleons, using Einstein’s equation \( {E}_{{\mathrm{b}}_{\mathrm{Total}}}=\Delta m{c}^2 \).

References

  1. P.E. Hodgson, E. Gadioli, E. Gadioli Erb, Introductory Nuclear Physics (Oxford Science Publications, Oxford, 1997)

    Google Scholar 

  2. D.G. Madland, J. Rayford Nix, New calculation of prompt fission neutron spectra and average prompt neutron multiplicities. Nucl. Sci. Eng. 81, 213–271 (1982)

    Article  Google Scholar 

  3. J. Lewins, Nuclear Reactor Kinetics and Control (Pergamon Press, Oxford, 1978)

    Google Scholar 

  4. K. Ott, R.J. Neuhold, Nuclear Reactor Dynamics (American Nuclear Society, LaGrange Park, 1985)

    Google Scholar 

  5. R.J. LaBauve, T.R. England, D.C. George, C.W. Maynard, Fission product analytic impulse source functions. Nucl. Technol. 56, 332–339 (1982)

    Google Scholar 

  6. A.F. Henry, Nuclear Reactor Analysis (The MIT Press, Cambridge, 1975)

    Google Scholar 

  7. J.R. Lamarsh, Introduction to Nuclear Reactor Theory (Addison Wesley, Boston, 1966)

    Google Scholar 

  8. B. Zohuri, Combined Cycle Driven Efficiency for Next Generation Nuclear Power Plants: An Innovative Design Approach (Springer, New York, 2015)

    Book  Google Scholar 

  9. B. Zohuri, P. McDaniel, A comparison of a recuperated open cycle (air) brayton power conversion system with the traditional steam rankine cycle for the next generation nuclear power plant. Nucl. Sci., October 2015

    Google Scholar 

  10. B. Zohuri, Innovative Open Air Brayton Combined Cycle Systems for the Next Generation Nuclear Power Plants (University of New Mexico Publications, Albuquerque, 2014)

    Google Scholar 

  11. P.J. McDaniel, B. Zohuri, C.R.E. de Oliveira, in A Combined Cycle Power Conversion System for Small Modular LMFBRs, ANS Transactions, September 2014

    Google Scholar 

  12. Cycle Power Conversion System for the Next Generation Nuclear Power Plan, ANS Transactions, November 2012

    Google Scholar 

  13. C. Forsberg, P. McDaniel, B. Zohuri, Variable electricity and steam from salt, helium, and sodium cooled base-load reactors with gas turbines and heat storage, in Proceedings of ICAPP 2015

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Problems

Problems

  1. Problem 1.1

    If atomic mass unit is designated by u, where 1 u is exactly one-twelfth of the mass of the 12C atom, equal to 1.661 × 10−27 kg, then calculate the energy equivalent to a conventional mass equal to 1 u.

  2. Problem 1.2

    Calculate the energy as Problem 1.1 using MeV as units.

  3. Problem 1.3

    1. (a)

      Calculate the mass defect and the binding energy for a nucleus of an isotope of tin 120Sn (atomic mass M = 119.9022 u) and for an isotope of uranium 235U (atomic mass M = 235.0439). Assume the measured mass of the atom is M; the mass defect ΔM is given by

      $$ \Delta M=Z\cdot \left({m}_{\mathrm{p}}+{m}_{\mathrm{e}}\right)+\left(A-Z\right)\cdot {m}_{\mathrm{n}}-M $$
      • \( Z\cdot {m}_{\mathrm{p}} \) = total mass of proton

      • \( Z\cdot {m}_{\mathrm{e}} \) = total mass of electron

      • \( \left(A-Z\right)\cdot {m}_{\mathrm{n}} \) = total mass of neutrons

    2. (b)

      Assume the total binding energy for uranium is approximately the same as tin; what would be the total energy that will be released after fission of a single U235 nucleus?

  4. Problem 1.4

    Calculate the mass defect for lithium-7. The mass of lithium-7 is 7.016003 amu. Assuming that:

    • m p = mass of a proton (1.007277 amu)

    • m n = mass of neutron (1.008665 amu)

    • m e = mass of an electron (0.000548597 amu)

  5. Problem 1.5

    Consider that 1 amu is equivalent to 931.5 MeV of energy; the binding energy can be calculated using the following relationship:

    $$ \mathrm{Binding}\ \mathrm{e}\mathrm{nergy} = \Delta m\left(\frac{931.5\;\mathrm{M}\mathrm{e}\mathrm{V}}{1\;\mathrm{amu}}\right) $$

    Then calculate the mass defect and binding energy for uranium235. One uranium235 atom has a mass of 235.043924 amu.

  6. Problem 1.6

    Calculate the decay constant, mean life, and half-life of a radioactive isotope which radioactivity after 100 days is reduced 1.07 times.

  7. Problem 1.7

    A block of aluminum has a density of 2.699 g/cm3. If the gram atomic weight of aluminum is 26.9815 g, then calculate the atom density of aluminum.

  8. Problem 1.8

    Since the activity and the number of atom are always proportional, they may be used interchangeably to describe any given radionuclide population. Therefore, the following is true.

    $$ A={A}_0{\mathrm{e}}^{-\lambda t} $$

    where

    • A = activity present at time t

    • A 0 = activity initially present

    • λ = decay constant (time−1)

    • t = time

    Assuming a sample of material contains 20 μg of californium-252 and this element has a half-life of 2.638 years; then calculate:

    1. (a)

      The number of californium-252 atoms initially present

    2. (b)

      The activity of californium-252 in curies, assuming the relationship between the activity, number of atoms, and decay constant is shown in \( A=\lambda N \), where A is the activity of nuclide (disintegrations/s), λ-decay constant of the nuclide (1/s), and finally N the number of atoms of the nuclide in the sample

    3. (c)

      The number of californium-252 atoms that will remain in 12 years

    4. (d)

      The time it will take for the activity to reach 0.001 curies

  9. Problem 1.9

    Plot the radioactive decay curve for nitrogen-16 over a period of 100 s. The initial activity is 142 curies and the half-life of nitrogen-16 is 7.13 s. Plot the curve on both linear rectangular coordinates and a semilog scale.

  10. Problem 1.10

    Find the macroscopic thermal neutron absorption cross section for iron, which has a density of 7.86 g/cm. The microscopic cross section for absorption of iron is 2.56 barns, and the gram atomic weight is 55.847 g.

  11. Problem 1.11

    An alloy is composed of 95 % aluminum and 5 % silicon (by weight). The density of the alloy is 2.66 g/cm. Properties of aluminum and silicon are shown below.

    Element

    Gram atomic weight

    σ a(barns)

    σ s(barns)

    Aluminum

    26.9815

    0.23

    1.49

    Silicon

    28.0855

    0.16

    2.20

    1. 1.

      Calculate the atom densities for the aluminum and silicon.

    2. 2.

      Determine the absorption and scattering macroscopic cross sections for thermal neutrons.

    3. 3.

      Calculate the mean free paths for absorption and scattering.

  12. Problem 1.12

    What is the value of σ f for uranium-235 for thermal neutrons at 500 °F? Uranium-235 has σ f of 583 barns at 68 °F.

  13. Problem 1.13

    If a one cubic centimeter section of a reactor has a macroscopic fission cross section of 0.1 cm−1, and if the thermal neutron flux is 1013 neutrons/cm2 s, what is the fission rate in that cubic centimeter?

  14. Problem 1.14

    A reactor operating at a flux level of 3 × 1013 neutrons/cm2 s contains 1020 atoms of uranium-235 per cm3. The reaction rate is 1.29 × 1012 fission/cm3. Calculate Σ f and σ f.

  15. Problem 1.15

    The microscopic cross section for the capture of thermal neutrons by hydrogen is 0.33 barn and for oxygen 2 × 10−4 barn. Calculate the macroscopic capture cross section of the water molecule for thermal neutrons.

  16. Problem 1.16

    Calculate the minimum energy that a neutron with energy 1 MeV can be reduced to after collision with:

    1. (a)

      Nucleus of hydrogen

    2. (b)

      Nucleus of carbon

Rights and permissions

Reprints and permissions

Copyright information

© 2017 Springer International Publishing Switzerland

About this chapter

Cite this chapter

Zohuri, B. (2017). Neutron Physics Background. In: Neutronic Analysis For Nuclear Reactor Systems. Springer, Cham. https://doi.org/10.1007/978-3-319-42964-9_1

Download citation

  • DOI: https://doi.org/10.1007/978-3-319-42964-9_1

  • Published:

  • Publisher Name: Springer, Cham

  • Print ISBN: 978-3-319-42962-5

  • Online ISBN: 978-3-319-42964-9

  • eBook Packages: EnergyEnergy (R0)

Publish with us

Policies and ethics