Neutron Flux and Reaction Rate Calculator

Compute neutron reaction rate from flux and cross-section, or find thermal flux from reactor power density. Uses R = Nσφ = Σφ.

⚡ Neutron Flux and Reaction Rate Calculator
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Reaction Rate R
Macroscopic Cross-Section Σ
Mean Free Path λ = 1/Σ
Neutron Flux φ
Neutron Flux φ
Fission Rate Rf
Power Density (check)
Energy per Fission (J)

⚡ What is the Neutron Reaction Rate?

The neutron reaction rate R describes how many nuclear reactions (absorptions, fissions, or scatterings) occur per unit volume per unit time in a material exposed to a neutron field. The fundamental formula is R = N × σ × φ = Σ × φ, where N is the number of target atoms per cm³, σ (sigma) is the microscopic cross-section in cm² (commonly expressed in barns, where 1 barn = 10⁻²⁴ cm²), and φ (phi) is the neutron flux in neutrons per cm² per second. The product Nσ = Σ is the macroscopic cross-section in cm⁻¹, representing the reaction probability per unit path length of a neutron.

The reaction rate formula appears throughout nuclear engineering in three major contexts. In reactor physics, the fission reaction rate R_f = Σ_f × φ directly gives the power produced per cm³ of fuel: power density P = R_f × Q, where Q is the energy per fission (approximately 200 MeV). This links the neutron flux (measured by detectors) to the thermal power output. In radiation shielding, the absorption reaction rate determines how quickly a neutron beam is attenuated as it passes through a shield material. In activation analysis, the capture reaction rate in a sample, integrated over an irradiation time, determines the induced radioactivity used to identify and quantify trace elements.

The neutron flux itself is defined as φ = n × v, where n is the neutron number density (neutrons/cm³) and v is the neutron speed (cm/s). This is not the same as the number of neutrons crossing a surface per second per cm² in one direction (the neutron current J); flux is isotropic and includes neutrons traveling in all directions. In a thermal reactor, the flux spectrum extends from thermal energies (0.025 eV) through the epithermal resonance region up to fast energies above 1 MeV. The one-group reaction rate formula R = Σφ uses energy-averaged cross-sections and is a widely used engineering approximation.

This calculator computes the neutron reaction rate from user-supplied flux, microscopic cross-section, and atom number density. It also provides the reverse calculation: finding the neutron flux from reactor power density and fission cross-section, which is useful when designing experiments in reactor facilities or estimating irradiation conditions from known power levels. Scientific notation input makes it easy to work with the wide range of magnitudes encountered in nuclear problems, from 10² barns for common nuclides to 10⁶ barns for the highest resonance peaks.

📐 Formula

Reaction Rate: R = N × σ × φ = Σ × φ
R = reaction rate (reactions/cm³/s)
N = atom number density (atoms/cm³) = (ρ × NA) / A
σ = microscopic cross-section (cm²) - convert barns: 1 barn = 10−24 cm²
φ = neutron flux (n/cm²/s)
Σ = macroscopic cross-section (cm−1) = N × σ
Mean Free Path: λ = 1 / Σ (cm)
Flux from Power Density:
φ = P / (Σf × Q)
P = power density (W/cm³)
Σf = fission macroscopic cross-section (cm−1)
Q = energy released per fission (J) = Q(MeV) × 1.602 × 10−13 J/MeV
Atom Number Density: N = (ρ × NA) / A
ρ = material density (g/cm³)
NA = Avogadro's number = 6.022 × 1023 mol−1
A = atomic mass (g/mol)

📖 How to Use This Calculator

Steps

1
Select calculation mode - choose "Reaction Rate (R = Nσφ)" to find the reaction rate from flux and cross-section, or "Flux from Power" to find the neutron flux from reactor power density and fission cross-section.
2
Enter neutron flux and cross-section - in Reaction Rate mode, enter the flux mantissa and exponent (e.g., 3.0 and 13 for 3.0 × 10¹³ n/cm²/s), the microscopic cross-section σ in barns from the ENDF/B nuclear data library, and the atom number density N using mantissa and exponent fields.
3
Click Calculate - the calculator returns the macroscopic cross-section Σ in cm², mean free path λ in cm, and reaction rate R in reactions/cm³/s displayed in scientific notation.
4
Use Flux from Power mode for reactor design - switch to "Flux from Power", enter the power density in W/cm³, fission macroscopic cross-section Σ_f in cm², and energy per fission Q in MeV (default 200 MeV), then calculate to obtain the thermal neutron flux and fission rate per cm³.

💡 Example Calculations

Example 1 - U-235 Fission Rate in LWR Fuel

Thermal flux 3.0 × 10¹³ n/cm²/s, σ_f = 582 barns, N = 6.96 × 10²&sup0; atoms/cm³

1
σ in cm²: 582 × 10−24 = 5.82 × 10−22 cm²
2
Σ_f = N × σ = 6.96 × 10²&sup0; × 5.82 × 10−22 = 0.4050 cm−1
3
R = Σ × φ = 0.4050 × 3.0 × 10¹³ = 1.215 × 10¹³ fissions/cm³/s
4
λ = 1 / Σ = 1 / 0.4050 = 2.469 cm (mean free path to fission)
R = 1.215 × 10¹³ fissions/cm³/s | Σ = 0.4050 cm−1 | λ = 2.469 cm
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Example 2 - Cadmium-113 Thermal Neutron Capture (High Cross-Section)

Flux 1.0 × 10¹² n/cm²/s, σ = 20600 barns (Cd-113), N = 3.2 × 10¹&sup9; atoms/cm³

1
σ in cm²: 20600 × 10−24 = 2.06 × 10−20 cm²
2
Σ = 3.2 × 10¹&sup9; × 2.06 × 10−20 = 0.6592 cm−1
3
R = 0.6592 × 1.0 × 10¹² = 6.592 × 10¹¹ captures/cm³/s
4
λ = 1 / 0.6592 = 1.517 cm (cadmium strongly absorbs thermal neutrons)
R = 6.592 × 10¹¹ captures/cm³/s | Σ = 0.6592 cm−1 | λ = 1.517 cm
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Example 3 - Flux from LWR Power Density

Power density 200 W/cm³, Σ_f = 0.350 cm−1, Q = 200 MeV/fission

1
Q in joules: 200 MeV × 1.602 × 10−13 J/MeV = 3.204 × 10−11 J
2
φ = P / (Σ_f × Q) = 200 / (0.350 × 3.204 × 10−11) = 200 / 1.121 × 10−11
3
φ = 1.784 × 10¹³ n/cm²/s
4
R_f = Σ_f × φ = 0.350 × 1.784 × 10¹³ = 6.244 × 10¹² fissions/cm³/s
φ = 1.784 × 10¹³ n/cm²/s | R_f = 6.244 × 10¹² fissions/cm³/s
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❓ Frequently Asked Questions

What is the neutron reaction rate formula R = Nσφ?+
The reaction rate R (reactions per cm³ per second) equals the product of atom number density N (atoms/cm³), microscopic cross-section σ (cm²), and neutron flux φ (n/cm²/s). The product Nσ = Σ is the macroscopic cross-section (cm⁻¹). The formula is R = Σφ = Nσφ. It is the fundamental equation linking the neutron population (flux), the target material (cross-section), and the rate of nuclear reactions in the material.
What is neutron flux and how is it defined in reactor physics?+
Neutron flux φ = n × v, where n is the neutron number density (neutrons/cm³) and v is the neutron speed (cm/s). It represents the total path length traveled by all neutrons in 1 cm³ per second, and its unit is n/cm²/s. Flux is isotropic (counts neutrons traveling in all directions) and differs from neutron current J, which is the net flow in one direction. In a reactor, typical thermal flux values range from 10¹² to 5×10¹³ n/cm²/s.
What is the microscopic cross-section σ and why is it measured in barns?+
The microscopic cross-section σ is the effective target area per atom for a specific nuclear reaction. It is a quantum mechanical probability expressed as an area. The barn unit (10⁻²⁴ cm²) was introduced because early nuclear physicists found cross-sections surprisingly large compared to the geometric size of nuclei. Common values: U-235 fission at thermal energies is 582 barns, Cd-113 thermal absorption is 20,600 barns, and H-1 thermal scattering is about 20 barns.
What is the macroscopic cross-section Σ and how does it relate to mean free path?+
The macroscopic cross-section Σ = Nσ (units cm⁻¹) is the reaction probability per unit path length of a neutron in the material. The mean free path λ = 1/Σ (cm) is the average distance a neutron travels before undergoing the reaction. A material with Σ = 0.5 cm⁻¹ has λ = 2 cm. Total macroscopic cross-section Σ_total = Σ_absorption + Σ_scatter is the sum over all reaction types.
How is the neutron flux related to reactor power density?+
Power density P = R_f × Q = Σ_f × φ × Q, where R_f is the fission rate per cm³, Q is the energy per fission (≈3.2×10⁻¹¹ J), and Σ_f is the fission macroscopic cross-section. Rearranging: φ = P / (Σ_f × Q). For a typical LWR with P = 200 W/cm³, Σ_f = 0.35 cm⁻¹, and Q = 200 MeV, the thermal flux is approximately 1.8×10¹³ n/cm²/s.
What are typical atom number density values for reactor materials?+
Atom number density N = (ρ × Nₐ) / A. For UO2 fuel at density 10.4 g/cm³ and molecular weight 270 g/mol: N_U = 2.32×10²² atoms/cm³. For 3% enriched fuel, N_235 = 6.96×10²⁰ atoms/cm³. For water at 1.0 g/cm³: N_O = 3.34×10²² atoms/cm³, N_H = 6.68×10²² atoms/cm³. For boron at 500 ppm in water: N_B ≈ 3.0×10¹⁹ atoms/cm³.
What is the difference between thermal and fast neutron reaction rates?+
Thermal neutrons (energy ~0.025 eV) have much larger cross-sections than fast neutrons for most reactions. U-235 fission cross-section is 582 barns at thermal energies but only about 1 barn for fast neutrons above 1 MeV. Thermal reaction rates dominate fission and absorption in thermal reactors. Fast reaction rates dominate elastic scattering from light nuclei (like hydrogen) and inelastic scattering from heavier nuclei. For accurate calculations, the reaction rate must be integrated over the full energy spectrum: R = integral of Σ(E) × φ(E) dE.
How are neutron cross-sections measured experimentally?+
Cross-sections are measured by time-of-flight (TOF) spectrometry at national laboratories. A pulsed neutron beam from a linac or reactor is directed at a thin sample, and the transmitted intensity is measured as a function of neutron arrival time (which gives neutron energy). The cross-section is σ = (1/N × t) × ln(I₀/I), where N is the sample atom density, t is the thickness, I₀ is the incident beam, and I is the transmitted beam. Databases like ENDF/B (USA), JEFF (Europe), and JENDL (Japan) compile these measurements.
What is activation analysis and how is it related to reaction rate?+
Neutron activation analysis (NAA) exploits R = Nσφ to identify elements. A sample placed in flux φ for time t accumulates radioactivity at rate R = Nσφ. After irradiation, gamma spectroscopy measures the induced activity A = R × (1 - e^(-λt)), where λ is the product isotope's decay constant. Known φ and σ from tables yield N, identifying and quantifying the element. NAA detects trace elements at parts-per-billion concentrations, used in forensics, archaeology, and food safety.
What is neutron fluence and how does it differ from flux?+
Neutron fluence Φ (capital phi) is the time-integrated flux: Φ = integral of φ(t) dt over the irradiation period, with units n/cm². It represents the total neutron exposure of a material. Radiation damage in structural materials is measured in fluence (or in dpa, displacements per atom, derived from the fast fluence above 1 MeV). Total reactions in a sample after irradiation time t equal R_total = Σ × φ × t = Σ × Φ.
How does neutron self-shielding affect reaction rate in thick samples?+
The formula R = Nσφ assumes a uniform flux throughout the material. In thick samples where Σ × thickness is not much less than 1, neutrons are significantly attenuated as they penetrate, so the flux decreases with depth. The effective flux seen by inner atoms is lower, and the average reaction rate is less than Nσφ_surface. This self-shielding effect must be corrected using the factor (1 - e^(-Σt))/(Σt) for a slab of thickness t. For thin samples (Σt much less than 0.1), self-shielding is negligible.
What are common applications of neutron reaction rate calculations in industry?+
Neutron reaction rate calculations are used in: (1) Reactor power monitoring - converting measured neutron flux to power output for control system feedback. (2) Fuel burnup tracking - integrating the fission rate over time to calculate fissile inventory depletion. (3) Radioisotope production - designing irradiation positions in research reactors to produce medical isotopes (Mo-99, I-131, Lu-177) at target yields. (4) Radiation shielding design - calculating neutron absorption rates in shield materials. (5) Waste management - computing activation of structural components that become radioactive waste after decommissioning.