BLD-NUCL84-02 · Lesson 2 · 24 clock hours · theory
Neutron Interactions and Cross Sections
Objective. Students will explain how neutrons interact with matter (scatter, absorption, fission), define macroscopic and microscopic cross sections, and use the concept to compare moderator and fuel neutron behavior.
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Neutron Interactions and Cross Sections
Why Neutron Behavior Matters
Every nuclear power plant generates heat through fission — the splitting of heavy nuclei, almost always uranium-235 (U-235). Fission is triggered by neutrons, and controlling neutrons means controlling reactor power. To operate a reactor safely, you must understand how neutrons interact with the atoms they encounter and how scientists quantify the probability of each interaction. That quantification is the cross section.
Types of Neutron Interactions
When a neutron enters a nucleus, one of several outcomes is possible:
Scattering occurs when the neutron bounces away from the nucleus. In elastic scattering, kinetic energy is conserved — the nucleus recoils and the neutron slows down. This is the dominant mechanism by which neutrons lose energy in a moderator. In inelastic scattering, the nucleus absorbs the neutron briefly, then re-emits it at lower kinetic energy while the nucleus releases a gamma ray. Inelastic scattering is important in heavy materials such as U-238.
Absorption occurs when the neutron is captured by the nucleus and is not re-emitted. Several outcomes are possible after absorption: the nucleus may emit gamma radiation (radiative capture), it may undergo fission, or it may emit another particle. Boron-10 is a prime example of a strong absorber; it captures a thermal neutron and emits an alpha particle, making it extremely useful for reactivity control via control rods and boric acid.
Fission is a special case of absorption in which the nucleus — most commonly U-235 or Pu-239 — splits into two lighter fission products, releases energy (~200 MeV per event), and emits on average 2–3 prompt neutrons. These new neutrons continue the chain reaction.
Microscopic Cross Section (σ)
Because neutron-nucleus interactions are probabilistic, physicists define the microscopic cross section (σ) as an effective target area that a single nucleus presents to an approaching neutron. It is not a physical dimension of the nucleus; it is a measure of interaction probability. The unit is the barn, where 1 barn = 10⁻²⁴ cm².
Different reactions have different cross sections: σ_s (scattering), σ_a (absorption), σ_f (fission). The total cross section σ_t = σ_s + σ_a. Cross sections depend strongly on neutron energy. For many absorbers, σ_a is proportional to 1/v — that is, it increases as the neutron slows down (the "1/v region"). This is why slow (thermal) neutrons are far more likely to cause fission in U-235 than fast neutrons are.
Macroscopic Cross Section (Σ)
In a real material, there are enormous numbers of nuclei. The macroscopic cross section (Σ) accounts for nuclear density:
Σ = N × σ
where N is the number density of nuclei (nuclei per cm³) and σ is the microscopic cross section (cm²). Σ therefore has units of cm⁻¹ and represents the probability per unit path length that a neutron undergoes a given interaction.
Mean Free Path (λ)
The mean free path (λ) is the average distance a neutron travels between interactions:
λ = 1 / Σ
A small mean free path means neutrons interact very frequently — the material is a strong moderator or absorber. A large mean free path means neutrons travel farther before interacting.
Moderators and the Role of Water
Light water (H₂O) is an effective moderator because hydrogen has a very large elastic scattering cross section and a low mass. Because a hydrogen nucleus (proton) has nearly the same mass as a neutron, a head-on collision can transfer almost all the neutron's kinetic energy in a single collision — analogous to a billiard ball striking another ball of equal mass. After roughly 18–25 collisions with hydrogen, a fast fission neutron (born at ~2 MeV) is slowed to thermal energies (~0.025 eV at room temperature).
Oxygen, the other component of water, has a much smaller scattering cross section and contributes less to moderation but does not significantly absorb neutrons, so it does not poison the chain reaction.
Boron for Reactivity Control
Boron-10 has an exceptionally large thermal absorption cross section — several thousand barns. This makes it ideal for reactor control. Dissolved boric acid in the primary coolant (chemical shim) or solid boron in control rods allows operators to add strong absorption without physically moving structures when fine adjustments are needed. Increasing boron concentration reduces neutron population and lowers reactor power; decreasing it allows power to rise.
Safety Implications
Understanding cross sections is directly tied to safe operations:
- Reactivity control: Operators rely on the high absorption cross sections of boron and hafnium in control rods to shut down the reactor quickly (SCRAM). Failure to account for changes in moderator temperature — which shift the neutron energy spectrum — can cause unexpected reactivity changes.
- Radiation shielding: Materials with high scattering cross sections (water, polyethylene) are placed around neutron sources to slow and absorb neutrons, reducing dose rates to workers. Always follow plant radiation work permit (RWP) requirements and wear designated PPE — including dosimetry — when working in areas with elevated neutron flux.
- Criticality safety: Inadvertently assembling a critical mass of fissile material outside a reactor is an extreme hazard. Knowing that a material has a large σ_f helps workers recognize which materials and configurations deserve extra controls under the facility's nuclear criticality safety program.
Key terms10
Microscopic cross section (σ)A measure of the probability that a single nucleus will interact with a neutron in a specific way; expressed in barns (1 barn = 10⁻²⁴ cm²). It is not a physical size but a probabilistic effective target area.
Macroscopic cross section (Σ)The probability per unit path length that a neutron undergoes a given interaction in a bulk material; calculated as Σ = N × σ, where N is nuclear number density. Units are cm⁻¹.
Mean free path (λ)The average distance a neutron travels in a material between successive interactions of a given type; λ = 1 / Σ. A short mean free path indicates frequent interactions.
Elastic scatteringA neutron-nucleus collision in which total kinetic energy is conserved; the neutron loses energy and slows down, especially effective when the target nucleus has a mass close to the neutron's mass.
Radiative captureA type of neutron absorption in which the compound nucleus emits a gamma ray rather than undergoing fission; a neutron loss mechanism that competes with fission in the fuel and contributes to reactivity loss.
BarnThe unit of microscopic cross section; 1 barn = 10⁻²⁴ cm². The name reflects the ironic comment that uranium nuclei looked 'as big as a barn' to early researchers measuring neutron cross sections.
Thermal neutronA neutron that has been slowed to an energy in equilibrium with its surrounding medium, approximately 0.025 eV at room temperature. Thermal neutrons have a much higher probability of causing fission in U-235 than fast neutrons.
1/v regionThe portion of the neutron energy spectrum — from thermal energies up through the epithermal region — where the absorption cross section of many nuclides is inversely proportional to neutron velocity, meaning slower neutrons are absorbed far more readily.
ModeratorA material used to slow fast fission neutrons to thermal energies through repeated elastic scattering collisions; effective moderators have high scattering cross sections, low absorption cross sections, and low atomic mass (e.g., light water, heavy water, graphite).
FissionThe splitting of a heavy fissile nucleus (such as U-235) upon neutron absorption into two lighter fission product nuclei, releasing approximately 200 MeV of energy and 2–3 prompt neutrons that can sustain the chain reaction.
Worked examples4
1. The macroscopic thermal-neutron absorption cross section of borated water is given as Σ_a = 0.022 cm⁻¹. Calculate the mean free path for absorption.
- Recall the mean free path formula: λ = 1 / Σ.
- Substitute the given macroscopic cross section: λ = 1 / 0.022 cm⁻¹.
- Perform the division: λ = 45.45 cm.
Answer: λ ≈ 45.5 cm. A thermal neutron in this borated water travels an average of about 45.5 cm before being absorbed.
2. Hydrogen in liquid water has a number density N ≈ 6.68 × 10²² atoms/cm³ and a thermal scattering microscopic cross section σ_s ≈ 38 × 10⁻²⁴ cm² (38 barns). Calculate the macroscopic scattering cross section Σ_s for hydrogen in water.
- Write the relationship: Σ_s = N × σ_s.
- Substitute values: Σ_s = (6.68 × 10²² atoms/cm³) × (38 × 10⁻²⁴ cm²/atom).
- Multiply the coefficients: 6.68 × 38 = 253.84.
- Combine the powers of ten: 10²² × 10⁻²⁴ = 10⁻².
- Result: Σ_s = 253.84 × 10⁻² cm⁻¹ = 2.538 cm⁻¹, which rounds to approximately 2.54 cm⁻¹.
Answer: Σ_s ≈ 2.54 cm⁻¹ for thermal-neutron scattering in hydrogen (water). This large value confirms that water is a very effective scattering medium.
3. Using the macroscopic scattering cross section from the previous example (Σ_s = 2.54 cm⁻¹ for hydrogen in water), calculate the mean free path for a thermal neutron scattering in water (hydrogen contribution only).
- Apply λ = 1 / Σ_s.
- Substitute: λ = 1 / 2.54 cm⁻¹.
- Divide: λ = 0.394 cm.
Answer: λ ≈ 0.39 cm. Thermal neutrons collide with hydrogen nuclei on average every 0.39 cm — illustrating how efficiently water slows neutrons through frequent collisions.
4. A material has a microscopic absorption cross section of 759 barns and a number density of 1.32 × 10²¹ atoms/cm³. Find (a) the macroscopic absorption cross section Σ_a and (b) the mean free path for absorption λ.
- Convert σ_a to cm²: 759 barns × 10⁻²⁴ cm²/barn = 759 × 10⁻²⁴ cm².
- Calculate Σ_a = N × σ_a = (1.32 × 10²¹) × (759 × 10⁻²⁴ cm²).
- Multiply coefficients: 1.32 × 759 = 1001.88.
- Combine powers: 10²¹ × 10⁻²⁴ = 10⁻³.
- Σ_a = 1001.88 × 10⁻³ cm⁻¹ ≈ 1.002 cm⁻¹.
- Calculate λ = 1 / Σ_a = 1 / 1.002 cm⁻¹ ≈ 0.998 cm.
Answer: Σ_a ≈ 1.00 cm⁻¹ and λ ≈ 1.00 cm. This relatively short mean free path shows the material is a moderately strong absorber at thermal energies.
The math in this lesson1
Learners compute neutron mean free path as the reciprocal of the macroscopic cross section.
A-SSE.1
In class: Instructor-led lecture with energy-spectrum diagrams: students trace a fast neutron from fission through slowing-down to thermal energies, annotating interactions at each stage on a printed 1/v cross-section graph. · Cross-section comparison worksheet: using tabulated values for hydrogen, oxygen, U-235, U-238, and boron-10, students calculate mean free path for thermal neutrons in water and explain why light water is an effective moderator and why boron is used for reactivity control. · Small-group analogy exercise: groups build a simple probabilistic model (dice-roll simulation) to illustrate the statistical nature of neutron absorption versus scattering, then present findings and connect to why reactor power is predictable despite individual randomness.
Materials: Printed thermal cross-section tables (ENDF/B data, instructor-summarized), graph paper, scientific calculators, Lamarsh & Baratta textbook, whiteboard
Check: Two-part check: (1) students correctly define and distinguish microscopic vs. macroscopic cross section in writing; (2) correctly calculate mean free path for at least 3 of 4 given scenarios. Pass mark 80%.
Practice check8
Answer each question, then check it. Nothing is recorded; this is your own practice.
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