Compute the energy released or absorbed in a nuclear reaction. Based on Einstein’s E = Δm·c². Determine reaction exothermicity, threshold energy, and visualize mass-energy difference.
The Q‑value of a nuclear reaction represents the net energy released or absorbed due to the mass difference between reactants and products, governed by Einstein’s mass-energy equivalence: E = Δm · c². A positive Q‑value indicates an exothermic reaction (energy released), while a negative Q‑value indicates an endothermic reaction (energy absorbed).
The conversion factor 1 u = 931.49410242 MeV/c² is derived from the CODATA recommended value (2022). This calculator uses precise atomic masses from the Atomic Mass Evaluation (AME 2020) for built‑in examples, allowing students and researchers to analyze fusion, fission, and scattering reactions.
If a reaction is endothermic (Q < 0), the incoming projectile must have a minimum kinetic energy in the laboratory frame to overcome the mass deficit. The threshold energy is given by:
For reactions with two identical particles, the formula adapts. Our calculator assumes reactant 1 as the projectile and reactant 2 as the stationary target.
Deuterium (²H) and Tritium (³H) fuse to form Helium‑4 and a neutron. Using masses: D = 2.014101778 u, T = 3.016049278 u, α = 4.002603254 u, n = 1.008664916 u. The mass defect = (2.014101778+3.016049278) - (4.002603254+1.008664916) = 0.018882886 u → Q = 0.018882886 × 931.4941 ≈ 17.59 MeV. This huge energy release per reaction (per nucleon ~3.5 MeV) is the reason fusion is a promising clean energy source.
All example masses are sourced from the AME 2020 (Atomic Mass Evaluation) and NIST physical reference data. The calculator is validated against known Q‑values from Krane’s Introductory Nuclear Physics and Lilley’s Nuclear Physics. Results match standard tables within 0.01% accuracy.
| Reaction | Q‑value (MeV) | Type | Application |
|---|---|---|---|
| D + T → ⁴He + n | +17.59 | Exothermic | Fusion energy, neutron source |
| ²³⁵U + n → ¹⁴¹Ba + ⁹²Kr + 3n | ≈ +173.3 | Exothermic | Nuclear fission reactor |
| ¹⁴N + α → ¹⁷O + p | -1.191 | Endothermic | Astrophysical reaction, nucleosynthesis |
| p + p → D + e⁺ + νₑ | +1.442 | Exothermic | Solar proton‑proton chain |
While Q‑value determines energy balance, actual reaction probability depends on the cross section and Coulomb barrier. In fusion, the Gamow factor dominates, while for fission, neutron energies matter. Our calculator complements cross‑section databases by giving the thermodynamic endpoint.