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Q-value of a Nuclear Reaction

Calculates the energy released or absorbed in a nuclear reaction from the difference in rest mass between reactants and products.

Nuclear Reactor Physics Nuclear Reactions

Q-value CalculatorNuclear Reaction Energy

Q = ( Σmreactants − Σmproducts ) · c²
Q = energy released (+) or absorbed (−)  ·  Σmreactants = total reactant mass  ·  Σmproducts = total product mass
⟹ Solve⟷Q, mR, mP
J
kg
kg
Please fix the errors above.
Solve for:
Presets:
Q-value—
—
Q: —mR: —mP: —
1 u = 1.66054×10⁻²⁷ kg  ·  1 MeV = 1.60218×10⁻¹³ J
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Q-value (MeV)—
Small (< 1 MeV) Medium (1–10 MeV) Large (10–100 MeV) Very Large (> 100 MeV)
Q = (mR − mP) · c²  ·  c = 2.99792458×10⁸ m/s  ·  Positive Q = exothermic (energy released)

Variables

Symbol Quantity Unit
Q Reaction Q-value MeV
Σm_reactants Total mass of reactants u
Σm_products Total mass of products u
c² Speed of light squared conversion factor 931.5 MeV/u

What it means

The Q‑value of a nuclear reaction is the net energy released or absorbed during the reaction. It is calculated from the mass difference between the initial (reactants) and final (products) nuclei: Q = (Σm_reactants − Σm_products) c². If Q > 0, the reaction is exothermic (releases energy); if Q < 0, it is endothermic (requires energy input). This parameter is crucial for evaluating whether a reaction can sustain a chain reaction (e.g., fission) or be used for fusion. It also determines the kinetic energy of the products. Q‑values are tabulated for various reactions and are used in nuclear physics, reactor design, and astrophysics (e.g., stellar nucleosynthesis). Understanding Q is essential for selecting reactions for energy production, transmutation, or medical isotope production.

Worked example

Q‑value of Nuclear Reaction – Two Examples

Real‑World
Scenario: Uranium‑235 fission has a mass defect of 0.161 u between reactants and products. The nuclear physicist calculates the Q‑value (energy released) per fission event using 1 u = 931.5 MeV to understand the energy yield of the fission process.
ParameterValue
Mass defect0.161 u
1Q = 0.161 × 931.5 = 150 MeV
Result 150 MeV ✓ Fission energy
Scenario: The fusion reaction of deuterium and tritium to form helium‑4 releases a neutron with a mass defect of 0.0189 u. The fusion engineer calculates the Q‑value to evaluate the energy yield for a potential fusion power plant design.
ParameterValue
Mass defect0.0189 u
1Q = 0.0189 × 931.5 = 17.6 MeV
Result 17.6 MeV ✓ Fusion energy
Nuclear insight: The Q‑value is the energy released or absorbed in a nuclear reaction. A positive Q‑value means the reaction releases energy (exothermic), while a negative Q‑value means it absorbs energy (endothermic).

Common mistakes

  • Q‑value: The energy released (or absorbed) in a nuclear reaction – in MeV or joules.
  • Mass sums: Σm_reactants – sum of masses of reactants (nuclei, particles) before the reaction.
  • Σm_products: Sum of masses of products after the reaction.
  • Sign: If Q > 0, energy is released (exothermic); if Q < 0, energy is absorbed (endothermic).
  • c²: Use the conversion 1 u = 931.5 MeV/c² or the SI factor – be consistent.

Applications

The Q‑value of a nuclear reaction is the net energy released (or absorbed) during the reaction, calculated from the mass difference between reactants and products, Q = (Σm_reactants − Σm_products)·c². This is fundamental for determining whether a nuclear reaction is exothermic or endothermic. Nuclear physicists and engineers use Q‑values to evaluate the feasibility of nuclear reactions for energy production (fission, fusion), to design accelerators, and to understand the energy balance in nuclear astrophysics. By knowing the Q‑value, they can predict the kinetic energies of reaction products and design appropriate experiments and devices. It is a key parameter in nuclear data libraries and reactor physics codes.

  • Evaluation of nuclear reaction energetics for fission and fusion
  • Design of particle accelerators and nuclear experiments
  • Nuclear astrophysics modelling of stellar nucleosynthesis
  • Calculation of neutron and gamma energies from reactions
  • Development of nuclear fuel and target materials