The Fusion Record — Fusion Energy News ← Home · Knowledge base
Concepts & Physics

Fusion Energy Gain Factor

The ratio Q of fusion power produced to external heating power supplied—the single number that defines whether a fusion device crosses the threshold from energy consumer to energy producer.

Reviewed Last reviewed: 9 Aug 2026 · Category: Concepts & Physics

Definition

The fusion energy gain factor, universally denoted Q, is the ratio of the total fusion power produced by a plasma to the external heating power supplied to sustain it:[1]

Definition: Q = Pfusion / Pheating

Key thresholds:
Q = 1: Scientific breakeven
Q ≈ 5: Approximate minimum for net electricity
Q = 10: ITER design target
Q → ∞: Ignition

Physical Meaning

As Q increases, a progressively larger fraction of the plasma heating comes from internal alpha particles. At Q = 5, alpha heating and external heating contribute roughly equally. At Q = 10, alpha heating provides about two-thirds. At ignition (Q → ∞), alpha heating alone sustains the burn.[1]

Scientific Q vs. Engineering Q

The standard Q considers only heating power delivered to the plasma, not total wall-plug electricity. For a fusion power plant to produce net electricity, Qeng > 1 is required, which generally demands Q well above 10.[3]

Experimental Milestones

Verified results:[2]

ITER and Future Devices

ITER is designed for Q ≥ 10, producing ~500 MW from 50 MW of external heating. DEMO-class power plants generally target Q ≥ 25–50.[3]

Sources

  1. Lawson, J.D. "Some Criteria for a Power Producing Thermonuclear Reactor." Proceedings of the Physical Society B, vol. 70, no. 1, 1957, pp. 6–10.
  2. Keilhacker, M. et al. "High fusion performance from deuterium-tritium plasmas in JET." Nuclear Fusion, vol. 39, no. 2, 1999, pp. 209–234.
  3. ITER Physics Expert Groups et al. "Chapter 1: Overview and summary." Nuclear Fusion, vol. 39, no. 12, 1999, pp. 2137–2174.
  4. Wurzel, S.E. and Hsu, S.C. "Progress toward fusion energy breakeven and gain as measured against the Lawson criterion." Physics of Plasmas, vol. 29, 2022, 062103.

Related