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Lawson criterion

Criterion for igniting a nuclear fusion chain reaction

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Through Normal distribution, Maxwell–Boltzmann distribution and Temperature

The concept was first developed by John D. Lawson in a classified 1955 paper that was declassified and published in 1957. As originally formulated, the Lawson criterion gives a minimum required value for the product of the plasma (electron) density ne and the "energy confinement time" τE that leads to net energy output.

Later analysis suggested that a more useful figure of merit is the triple product of density, confinement time, and plasma temperature T. The triple product also has a minimum required value, and the name "Lawson criterion" may refer to this value.

On August 8, 2021, researchers at Lawrence Livermore National Laboratory's National Ignition Facility in California confirmed to have produced the first-ever successful ignition of a controlled nuclear fusion reaction surpassing the Lawson's criteria in the experiment.

Energy balance

The central concept of the Lawson criterion is an examination of the energy balance for any fusion power plant using a hot plasma. This is shown below:

Net power = Efficiency × (Fusion − Radiation loss − Conduction loss)

  1. Net power is the excess power beyond that needed internally for the process to proceed in any fusion power plant.
  2. Efficiency is how much energy is needed to drive the device and how well it collects energy from the reactions.
  3. Fusion is rate of energy generated by the fusion reactions.
  4. Radiation loss is the energy lost as light (including X-rays) leaving the plasma.
  5. Conduction loss is the energy lost as particles leave the plasma, carrying away energy.

Lawson calculated the fusion rate by assuming that the fusion reactor contains a hot plasma cloud which has a Gaussian curve of individual particle energies, a Maxwell–Boltzmann distribution characterized by the plasma's temperature. Based on that assumption, he estimated the first term, the fusion energy being produced, using the volumetric fusion equation.

Fusion = Number density of fuel A × Number density of fuel B × Cross section(Temperature) × Energy per reaction

  1. Fusion is the rate of fusion energy produced by the plasma
  2. Number density is the density in particles per unit volume of the respective fuels (or just one fuel, in some cases)
  3. Cross section is a measure of the probability of a fusion event, which is based on the plasma temperature
  4. Energy per reaction is the energy released in each fusion reaction

This equation is typically averaged over a population of ions which has a normal distribution. The result is the amount of energy being created by the plasma at any instant in time.

Lawson then estimated the radiation losses using the following equation:

PB=1.4×10−34⋅n2⋅T1/2Wcm3

where n is the number density of the cloud and T is the temperature. For his analysis, Lawson ignores conduction losses. In reality this is nearly impossible; practically all systems lose energy through particle transport, where mass leaves the plasma and carries away its energy.

By equating radiation losses and the volumetric fusion rates, Lawson estimated the minimum temperature for the fusion for the deuterium–tritium (D-T) reaction

12D+13T→24He(3.5MeV)+01n(14.1MeV)

to be 30 million degrees (2.6 keV), and for the deuterium–deuterium (D-D) reaction

12D+12D→13T(1.0MeV)+11p(3.0MeV)

to be 150 million degrees (12.9 keV).

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