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AI and Nuclear Fusion Vol.2: Ignition, Burn Physics & Power Balance

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Last updated at Posted at 2026-02-13

title: "AI and Nuclear Fusion Vol.2: Ignition, Burn Physics & Power Balance"
emoji: "🔥"
type: "idea"
topics: ["nuclear", "fusion", "plasma", "energy", "AI"]
published: false

AI and Nuclear Fusion Vol.2: Ignition, Burn Physics & Power Balance

Series: "Thinking Seriously About Nuclear Fusion with AI"
Volume 2 of 9 | Target: Policy, Investment, and Engineering Decision-Makers
Author: Dosanko Tousan | AI Partner: Claude (Anthropic)
License: MIT


Document Classification

Item Detail
Purpose Derive the complete power balance of a fusion reactor from first principles; establish quantitative ignition criteria for all candidate fuels; assess proximity of current experiments to ignition
Audience Government policy advisors, energy investment analysts, fusion program managers, aerospace propulsion engineers
Prerequisites Vol.1 of this series (nuclear reaction physics, confinement fundamentals). All derivations self-contained.
Scope Power balance → Lawson criterion → Ignition vs breakeven → Alpha heating → Burning plasma → Radiation losses → Fuel-specific analysis → Experimental status → Propulsion implications
Deliverables (1) Complete Lawson derivation, (2) Power balance code for all fuels, (3) Burning plasma simulation, (4) ITER/SPARC/NIF assessment, (5) Propulsion power balance analysis

Table of Contents

Part I: The Lawson Criterion

  1. §1. Executive Summary
  2. §2. Power Balance of a Fusion System
  3. §3. Derivation of the Lawson Criterion
  4. §4. The Triple Product — n·τ_E·T
  5. §5. Q — The Fusion Gain Factor
  6. §6. From Breakeven to Ignition

Part II: Burning Plasma Physics

  1. §7. Alpha Particle Heating
  2. §8. The Burning Plasma Regime
  3. §9. Helium Ash and Fuel Dilution
  4. §10. Radiation Losses — Bremsstrahlung and Beyond
  5. §11. Thermal Stability and Burn Control

Part III: Fuel-Specific Power Balance

  1. §12. D-T Power Balance
  2. §13. D-D Power Balance
  3. §14. D-³He Power Balance
  4. §15. p-¹¹B Power Balance — The Fundamental Challenge

Part IV: Experimental Status and Projections

  1. §16. The Lawson Diagram — Where We Are
  2. §17. ITER — The Burning Plasma Experiment
  3. §18. SPARC — The High-Field Compact Path
  4. §19. NIF — Inertial Confinement
  5. §20. Private Ventures — The New Landscape

Synthesis

  1. §21. Computational Analysis — Full Reproducible Code
  2. §22. Implications for Reactor Economics and Propulsion
  3. §23. Uncertainties and Limitations
  4. §24. References

§1. Executive Summary

The central question of fusion energy is not whether fusion reactions can be produced — they can, and have been since 1952. The question is whether a fusion system can produce more energy than it consumes. This volume derives the complete quantitative framework for answering that question.

Key findings:

  1. The Lawson criterion establishes minimum requirements for net energy gain: $n \tau_E > 1.5 \times 10^{20}$ m⁻³·s for D-T at optimal temperature (~14 keV). Radiation losses, fuel dilution, and impurities raise the bar further.

  2. ITER is designed to achieve Q = 10 (500 MW fusion from 50 MW heating), entering the burning plasma regime where alpha particles dominate heating. SPARC targets Q ≥ 2 in a smaller, higher-field device. Neither has been accomplished.

  3. NIF achieved Q_scientific > 1 (target gain) in December 2022, but Q_engineering ≪ 1 when laser wall-plug efficiency (~1%) is included. The achievement confirms ignition physics but not an energy production path.

  4. The p-¹¹B power balance is fundamentally marginal. Bremsstrahlung scales as $Z_{eff}^2 T^{1/2}$; for boron ($Z = 5$), radiation exceeds fusion power in thermal plasmas. Non-thermal approaches remain an open question.

  5. For fusion propulsion, the metric shifts from Q to thrust-to-weight ratio and specific impulse. Sub-ignition engines (Q = 3–5) are acceptable if the external power mass penalty is tolerable. This relaxes the ignition requirement for space.


§2. Power Balance of a Fusion System

§2.1 Power Flows

A fusion reactor is a thermodynamic system. Every watt entering the plasma must exit as fusion products, radiation, or transport loss. The power flows:

Inputs:

  • $P_{heat}$ = external heating (ohmic, NBI, ICRH, ECRH)

Internal processes:

  • $P_{fus}$ = total fusion power = $P_\alpha + P_n$
  • $P_\alpha$ = charged-particle fusion power (self-heating)
  • $P_n$ = neutron power (escapes magnetically, captured in blanket)
  • $P_{rad}$ = radiation losses (bremsstrahlung, synchrotron, line radiation)
  • $P_{loss} = W/\tau_E$ = transport losses (conduction, convection across field lines)

Outputs:

  • $P_e$ = net electrical output
  • $P_{recirc}$ = recirculating power (heating systems, magnets, cryogenics, pumps)

§2.2 Steady-State Power Balance

In steady state ($dW/dt = 0$), the plasma energy equation is:

$$
P_\alpha + P_{heat} = P_{rad} + P_{loss}
$$

This single equation governs all of fusion reactor physics. Every term has different parametric dependencies on density $n$, temperature $T$, magnetic field $B$, and confinement time $\tau_E$. The art of fusion reactor design is navigating these dependencies to achieve a self-consistent operating point.

§2.3 The Energy Confinement Time

The energy confinement time $\tau_E$ quantifies how quickly the plasma loses energy through transport:

$$
\tau_E \equiv \frac{W}{P_{loss}} = \frac{3nk_BTV}{P_{loss}}
$$

where $W = \frac{3}{2}n_ek_BT_e + \frac{3}{2}n_ik_BT_i \approx 3nk_BT$ for equal temperatures and quasi-neutral plasma ($n_e \approx n_i \equiv n$), and $V$ is the plasma volume.

Therefore:

$$
P_{loss} = \frac{3nk_BTV}{\tau_E}
$$

§2.4 Fusion Power Density

For a 50:50 D-T mixture (each species at density $n/2$):

$$
p_{fus} = \frac{n_D \cdot n_T}{1} \cdot \langle\sigma v\rangle \cdot Q_{DT} = \frac{n^2}{4} \langle\sigma v\rangle \cdot Q_{DT}
$$

where $Q_{DT} = 17.59$ MeV per reaction.

The alpha power density (charged particles that remain in the plasma):

$$
p_\alpha = \frac{n^2}{4} \langle\sigma v\rangle \cdot E_\alpha = \frac{n^2}{4} \langle\sigma v\rangle \times 3.52 \text{ MeV}
$$

The neutron power density (escapes the plasma):

$$
p_n = \frac{n^2}{4} \langle\sigma v\rangle \cdot E_n = \frac{n^2}{4} \langle\sigma v\rangle \times 14.07 \text{ MeV}
$$

The self-heating fraction for D-T:

$$
\frac{E_\alpha}{Q_{DT}} = \frac{3.52}{17.59} = 0.200
$$

Only 20% of D-T fusion energy remains in the plasma as self-heating. The plasma must amplify this modest fraction into a self-sustaining burn. This is the core challenge.

§2.5 Generalized Charged-Particle Fractions

Reaction Q (MeV) $f_{ch}$ Charged products Self-heating advantage
D-T 17.59 0.20 α (3.52 MeV) 1.0× (baseline)
D-D → ³He+n 3.27 0.25 ³He (0.82 MeV)
D-D → T+p 4.03 1.00 T + p
D-³He 18.35 1.00 α + p 5.0×
p-¹¹B 8.68 1.00 5.0×

Aneutronic fuels (D-³He, p-¹¹B) have $f_{ch} = 1.0$ — all fusion energy stays as charged particles. This enables both superior self-heating and direct energy conversion. The price: much higher temperature requirements (Vol.1, §8).


§3. Derivation of the Lawson Criterion

§3.1 Historical Context

In 1955, John Lawson, working at AERE Harwell, asked: what minimum plasma conditions are needed for a fusion reactor to produce net energy? His classified report (declassified 1957) established the foundational criterion that has guided fusion research for nearly 70 years.

§3.2 Setup and Assumptions

Consider a plasma of volume $V$, density $n$, temperature $T$, confined for time $\tau_E$ with external heating power $P_{heat}$.

Assumptions:

  1. Equal ion and electron temperatures: $T_i = T_e = T$
  2. 50:50 D-T fuel mix: $n_D = n_T = n/2$
  3. Quasi-neutrality: $n_e = n$
  4. Steady state: $dW/dt = 0$
  5. Radiation = bremsstrahlung only (clean plasma)

§3.3 The Power Balance

$$
P_\alpha + P_{heat} = P_{brem} + P_{loss}
$$

Substituting:

$$
\frac{n^2}{4}\langle\sigma v\rangle E_\alpha V + P_{heat} = C_B n^2 Z_{eff} T^{1/2} V + \frac{3nk_BTV}{\tau_E}
$$

§3.4 The Breakeven Condition (Q = 1)

At scientific breakeven, $P_{fus} = P_{heat}$, i.e., fusion output equals external heating input. The condition for $P_{fus} \geq P_{heat}$:

$$
P_{fus} = \frac{n^2}{4}\langle\sigma v\rangle Q_{DT} V \geq P_{heat}
$$

From the power balance:

$$
P_{heat} = P_{brem} + P_{loss} - P_\alpha
$$

Therefore breakeven requires:

$$
\frac{n^2}{4}\langle\sigma v\rangle Q_{DT} V \geq C_B n^2 Z_{eff} T^{1/2} V + \frac{3nk_BTV}{\tau_E} - \frac{n^2}{4}\langle\sigma v\rangle E_\alpha V
$$

$$
\frac{n^2}{4}\langle\sigma v\rangle (Q_{DT} + E_\alpha) \geq C_B n^2 Z_{eff} T^{1/2} + \frac{3nk_BT}{\tau_E}
$$

§3.5 The Ignition Condition (Q = ∞)

At ignition, $P_{heat} = 0$. Alpha heating alone sustains the plasma:

$$
\frac{n^2}{4}\langle\sigma v\rangle E_\alpha = C_B n^2 Z_{eff} T^{1/2} + \frac{3nk_BT}{\tau_E}
$$

Solving for $n\tau_E$:

$$
\boxed{n\tau_E = \frac{12 k_BT}{\langle\sigma v\rangle E_\alpha - 4 C_B Z_{eff} T^{1/2}}}
$$

This is the Lawson criterion for ignition, including bremsstrahlung. The denominator must be positive, which sets a constraint:

$$
\langle\sigma v\rangle E_\alpha > 4 C_B Z_{eff} T^{1/2}
$$

This is automatically satisfied for D-T ($Z_{eff} = 1$) at T = 5–40 keV, but becomes the critical constraint for high-Z fuels like p-¹¹B.

§3.6 Numerical Evaluation for D-T

At $T = 14$ keV (optimal):

  • $\langle\sigma v\rangle = 2.3 \times 10^{-22}$ m³/s
  • $E_\alpha = 3.52$ MeV = $5.64 \times 10^{-13}$ J
  • $C_B = 5.35 \times 10^{-37}$ W·m³·keV⁻¹/²
  • $Z_{eff} = 1$, $k_B \times 14$ keV = $2.24 \times 10^{-15}$ J

Numerator: $12 \times 2.24 \times 10^{-15} = 2.69 \times 10^{-14}$

Denominator: $2.3 \times 10^{-22} \times 5.64 \times 10^{-13} - 4 \times 5.35 \times 10^{-37} \times 14^{0.5}$
$= 1.30 \times 10^{-34} - 8.01 \times 10^{-36} = 1.22 \times 10^{-34}$

$$
(n\tau_E)_{ign} = \frac{2.69 \times 10^{-14}}{1.22 \times 10^{-34}} = 2.2 \times 10^{20} \text{ m}^{-3}\text{s}
$$

§3.7 The Generalized Lawson Criterion for Finite Q

For arbitrary Q:

$$
P_\alpha + P_{heat} = P_{brem} + P_{loss}
$$

where $P_{heat} = P_{fus}/Q = \frac{n^2}{4}\langle\sigma v\rangle E_{fus}/Q$.

$$
n\tau_E = \frac{12 k_BT}{(f_{ch} + 1/Q)\langle\sigma v\rangle E_{fus} - 4 C_B Z_{eff} T^{1/2}}
$$

This family of curves in the $n\tau_E$–$T$ plane (Fig. 2) shows the operating requirements for each Q value.


§4. The Triple Product — n·τ_E·T

§4.1 Definition

The fusion triple product:

$$
\Pi \equiv n \tau_E T
$$

combines the three independent plasma parameters into a single figure of merit. For D-T ignition:

$$
\Pi_{ign} \geq 3 \times 10^{21} \text{ keV·s/m}^3
$$

§4.2 Physical Meaning

Fusion power density: $p_{fus} \propto n^2 \langle\sigma v\rangle \propto n^2 T^2$ (in the reactive range, 10–30 keV).

Loss power density: $p_{loss} = 3nk_BT/\tau_E$.

The ratio:

$$
\frac{p_{fus}}{p_{loss}} \propto \frac{n^2 T^2}{nT/\tau_E} = n\tau_E T
$$

The triple product directly measures the competition between fusion heating and energy loss. It is the single most important number for comparing fusion experiments across all configurations.

§4.3 Requirements by Fuel

Fuel $\Pi_{ign}$ (keV·s/m³) $T_{opt}$ (keV) $(n\tau_E)_{min}$ (m⁻³·s) Relative difficulty
D-T $3 \times 10^{21}$ 14 $2.2 \times 10^{20}$ 1.0
D-D $5 \times 10^{22}$ 50 $1.0 \times 10^{21}$ ~17
D-³He $6 \times 10^{22}$ 58 $1.0 \times 10^{21}$ ~20
p-¹¹B $>10^{24}$ 300 $>3 \times 10^{21}$ ~300+

§4.4 Historical Progress

The triple product has increased by a factor of $10^5$ since 1965 — roughly doubling every 1.8 years, a "fusion Moore's law" that has slowed since the 1990s as devices approached their design limits.

Year Device Type $\Pi$ (keV·s/m³) $\Pi/\Pi_{ign}$
1965 T-3 Tokamak $10^{16}$ $3 \times 10^{-6}$
1975 Alcator A Tokamak $8 \times 10^{17}$ $3 \times 10^{-4}$
1978 PLT Tokamak $2 \times 10^{18}$ $7 \times 10^{-4}$
1983 Alcator C Tokamak $8 \times 10^{19}$ $0.027$
1986 TFTR Tokamak $1.5 \times 10^{20}$ $0.050$
1991 JET Tokamak $3 \times 10^{20}$ $0.10$
1994 JT-60U Tokamak $1.53 \times 10^{21}$ $0.51$
1997 JET (D-T) Tokamak $1.1 \times 10^{21}$ $0.37$
2024 JET (D-T final) Tokamak $1.4 \times 10^{21}$ $0.47$
~2035 ITER (target) Tokamak $3.5 \times 10^{21}$ $1.17$
~2030 SPARC (target) Tokamak $2.5 \times 10^{21}$ $0.83$

We are within a factor of ~2 of D-T ignition. The gap sounds small, but the last factor of 2 requires entering the burning plasma regime — qualitatively new physics (§8).


§5. Q — The Fusion Gain Factor

§5.1 Definition

$$
Q \equiv \frac{P_{fus}}{P_{heat}}
$$

§5.2 Key Q Values and Their Significance

Q Physical meaning Engineering meaning Achieved?
$Q \ll 1$ Negligible fusion yield Net energy consumer Most experiments
$Q = 0.67$ Record D-T Q (JET, 1997) Far from useful
$Q = 1$ Scientific breakeven Still large net consumer NIF 2022 (target only)
$Q = 5$ Burning plasma: $f_\alpha > 50%$ New physics regime
$Q = 10$ ITER target Net thermal gain, not electric
$Q \approx 3.3$ Engineering breakeven ($Q_{eng} = 0$) Zero net electricity
$Q = 25-30$ Power plant minimum Net electricity ~30%
$Q = \infty$ Ignition No external heating needed

§5.3 Self-Heating Fraction

The fraction of total heating provided by alpha particles:

$$
f_\alpha = \frac{P_\alpha}{P_\alpha + P_{heat}} = \frac{f_{ch} \cdot Q}{f_{ch} \cdot Q + 1}
$$

For D-T ($f_{ch} = 0.20$):

Q $f_\alpha$ Physics Status
0.67 12% JET record
1 17% Breakeven
2 29% SPARC target
5 50% Burning plasma
10 67% ITER target
30 86% Power plant
100% Ignition

For aneutronic fuels ($f_{ch} = 1.0$): $f_\alpha = Q/(Q+1)$. Burning plasma threshold at Q = 1 (not Q = 5). This is a major advantage — but the difficulty of achieving even Q = 1 for p-¹¹B is far greater than Q = 5 for D-T.

§5.4 Q_engineering: The Real Metric

$Q$ measures physics performance. The metric that matters for energy production is:

$$
Q_{eng} = \frac{P_{e,net}}{P_{e,consumed}} = \frac{\eta_{th}(P_n + P_{rad} + P_{loss}) - P_{recirc}}{P_{recirc}}
$$

Approximate relationship:

$$
Q_{eng} \approx \eta_{th} \cdot Q - \frac{1}{1 - f_{recirc}}
$$

For $\eta_{th} = 0.40$ (steam Rankine cycle), $f_{recirc} = 0.25$:

Physics Q $Q_{eng}$ Net output
3.3 0 Zero
10 2.7 Marginal
20 6.7 Moderate
30 10.7 Commercial threshold
50 18.7 Highly economic

Q = 10 (ITER) produces marginal net electricity. Power plants need Q ≥ 25–30.


§6. From Breakeven to Ignition

§6.1 The Operating Space

The $n\tau_E$–$T$ plane (Figs. 1–2) contains curves of constant Q. Between the Q = 1 curve and the ignition curve lies the space of burning plasmas — the terra incognita of fusion physics.

§6.2 The D-T Ignition Window

Ignition requires operating within a temperature window:

  • Lower bound ($T \lesssim 5$ keV): $\langle\sigma v\rangle$ drops too fast — alpha heating cannot overcome transport losses regardless of $n\tau_E$.
  • Upper bound ($T \gtrsim 40$ keV): $\langle\sigma v\rangle$ decreases past its peak while bremsstrahlung continues to rise.
  • Optimal window: 8–30 keV. Most reactor designs target 12–18 keV.

§6.3 The Minimum Ignition Point

The ignition curve $n\tau_E(T)$ has a minimum at $T_{opt} \approx 14$ keV:

$$
(n\tau_E)_{min} \approx 1.5 \times 10^{20} \text{ m}^{-3}\text{s}
$$

$$
(\Pi){min} \equiv (n\tau_E T){min} \approx 2.1 \times 10^{21} \text{ keV·s/m}^3
$$

At $n = 10^{20}$ m⁻³ (tokamak): $\tau_E \geq 1.5$ s. At $n = 10^{21}$ m⁻³: $\tau_E \geq 0.15$ s. At $n = 10^{31}$ m⁻³ (ICF): $\tau_E \geq 1.5 \times 10^{-11}$ s.


§7. Alpha Particle Heating

§7.1 Birth and Energy Partition

In D-T fusion, alpha particles are born at $E_\alpha = 3.52$ MeV — approximately 200× the thermal ion energy at $T = 15$ keV. These fast ions carry the entire self-heating budget and must transfer their energy to the bulk plasma.

The alpha slowing-down involves two drag mechanisms:

  1. Electron drag (dominant at $E_\alpha > E_{crit}$): Coulomb interactions with electrons. Drag rate approximately constant with energy.
  2. Ion drag (dominant at $E_\alpha < E_{crit}$): Coulomb interactions with thermal ions. Drag rate increases as the alpha slows.

The critical energy where both drag rates are equal:

$$
E_{crit} = 14.8 \cdot T_e \left(\frac{A_\alpha}{A_e}\right)^{1/3} \left(\sum_i \frac{n_i Z_i^2}{n_e A_i}\right)^{2/3}
$$

Simplified for D-T at $T_e = 15$ keV:

$$
E_{crit} \approx 330 \text{ keV}
$$

Since $E_\alpha = 3520$ keV $\gg E_{crit} = 330$ keV, most alpha energy initially heats electrons (roughly 2/3 to electrons, 1/3 to ions), which then equilibrate with ions on the timescale $\tau_{ei}$.

§7.2 Slowing-Down Time

The alpha slowing-down time on electrons:

$$
\tau_{se} = \frac{6.27 \times 10^{14} A_\alpha T_e^{3/2}}{Z_\alpha^2 n_e \ln\Lambda}
$$

At $n_e = 10^{20}$ m⁻³, $T_e = 15$ keV, $\ln\Lambda = 17$:

$$
\tau_{se} \approx 0.18 \text{ s}
$$

Requirement: $\tau_{se} < \tau_E$ for effective self-heating. For ITER ($\tau_E \approx 3.7$ s): comfortably satisfied ($\tau_{se}/\tau_E \approx 0.05$).

§7.3 Alpha Confinement

The alpha Larmor radius at birth energy:

$$
\rho_\alpha = \frac{m_\alpha v_\alpha}{Z_\alpha e B} = \frac{\sqrt{2 m_\alpha E_\alpha}}{Z_\alpha e B}
$$

For $E_\alpha = 3.52$ MeV, $B = 5.3$ T:

$$
\rho_\alpha \approx 0.054 \text{ m}
$$

This is small compared to the minor radius ($a = 2.0$ m for ITER), so alphas are well-confined. In compact devices or FRCs ($a \sim 0.2$–0.5 m), alpha orbit loss becomes significant — a critical constraint for compact reactor design.

§7.4 Alpha-Driven Instabilities

Fast alphas can resonate with MHD waves, driving instabilities that expel them before they thermalize:

Instability Resonance condition Growth rate Consequence
TAE (Toroidal Alfvén Eigenmode) $v_\alpha \approx v_A/3$ $\gamma \sim \omega_{TAE} \beta_\alpha$ Alpha redistribution, moderate loss
EPM (Energetic Particle Mode) Non-perturbative Fast Sudden alpha expulsion
Fishbone $\omega_{prec} = \omega_{diamagnetic}$ at $q = 1$ $\gamma \sim \omega_*$ Periodic alpha bursts

The Alfvén velocity: $v_A = B/\sqrt{\mu_0 n_i m_i} \approx 7 \times 10^6$ m/s at ITER conditions.

Alpha birth velocity: $v_\alpha = \sqrt{2E_\alpha/m_\alpha} \approx 1.3 \times 10^7$ m/s.

The ratio $v_\alpha/v_A \approx 1.8$ places ITER alphas in the super-Alfvénic regime — the most dangerous for TAE excitation.

This is the single largest unknown for burning plasma operation. No existing experiment has operated at ITER-relevant $\beta_\alpha$ values. TAE simulations predict 10–30% alpha heating degradation in pessimistic scenarios, which directly reduces the achievable Q.


§8. The Burning Plasma Regime

§8.1 Definition

A burning plasma is defined by:

$$
f_\alpha > 0.5 \quad \Leftrightarrow \quad Q > \frac{1}{2f_{ch} - 1} \quad \Rightarrow \quad Q > 5 \text{ (D-T)}
$$

§8.2 Qualitative Novelty

Every existing fusion experiment is externally controlled: the experimenter chooses the heating power, and the plasma responds. In a burning plasma, the dominant heating source is internal — alpha particles whose production rate depends nonlinearly on the plasma state.

This creates four new phenomena:

1. Self-organization. The alpha heating profile depends on $n^2\langle\sigma v\rangle(T)$, which depends on the temperature profile, which depends on transport, which depends on turbulence, which depends on gradients. The system determines its own equilibrium through coupled nonlinear feedback.

2. Alpha-turbulence interaction. Fast alpha particles modify the distribution function, affecting micro-instabilities (ITG, TEM) that drive transport. This coupling has never been measured experimentally.

3. Thermal excursion risk. If alpha heating increases faster with T than losses, perturbations amplify — potential thermal runaway. If the converse, perturbations decay — thermal quench. The system's stability depends on where in parameter space it operates.

4. New control paradigm. Operating a burning plasma is fundamentally different from operating an externally heated one: it is closer to controlling a fire than to running a furnace. The control actuators (auxiliary heating, fuel injection, impurity injection) must respond to an internally driven system.

§8.3 Power Terms in a Burning Plasma

Power term Parametric scaling Temperature behavior (5–30 keV)
$P_\alpha$ $n^2 \langle\sigma v\rangle E_\alpha$ Strongly increasing ($\propto T^2$ approx)
$P_{brem}$ $n^2 Z_{eff} T^{1/2}$ Weakly increasing
$P_{sync}$ $n T^{5/2} B^2$ Strongly increasing at high T
$P_{loss}$ $nT/\tau_E$ Linear (at fixed $\tau_E$)

The burn point (self-consistent equilibrium) occurs where $P_\alpha(T) = P_{brem}(T) + P_{loss}(T)$.


§9. Helium Ash and Fuel Dilution

§9.1 Production Rate

Every D-T fusion event produces one ⁴He atom. In a burning plasma at $Q = 10$:

$$
\dot{N}{He} = \frac{P{fus}}{Q_{DT}} = \frac{500 \times 10^6}{17.59 \times 10^6 \times 1.602 \times 10^{-19}} \approx 1.77 \times 10^{20} \text{ He/s}
$$

(For ITER: ~$1.8 \times 10^{20}$ helium atoms per second.)

§9.2 Steady-State Accumulation

$$
\frac{dn_{He}}{dt} = \frac{n^2}{4}\langle\sigma v\rangle - \frac{n_{He}}{\tau_{He}^*} = 0
$$

$$
n_{He} = \frac{n^2}{4}\langle\sigma v\rangle \tau_{He}^*
$$

§9.3 Fuel Dilution Impact

Quasi-neutrality: $n_e = n_D + n_T + 2n_{He}$. For given $n_e$, helium displaces fuel:

$$
n_{fuel} = n_e - 2n_{He}
$$

$$
P_{fus} \propto n_{fuel}^2 = (n_e - 2n_{He})^2
$$

$n_{He}/n_e$ Fuel reduction Power reduction Ignition $n\tau_E$ increase
0% 0% 0% 0%
5% 10% 19% ~23%
10% 20% 36% ~56%
15% 30% 51% ~104%
20% 40% 64% ~178%

At 10% helium fraction, the ignition threshold increases by 56% — a dramatic penalty.

§9.4 Exhaust Requirement

Steady-state ash fraction depends on the ratio $\rho \equiv \tau_{He}^*/\tau_E$:

$$
f_{He} \equiv \frac{n_{He}}{n_e} \approx \frac{\rho}{4} \frac{n \langle\sigma v\rangle \tau_E}{1 + 2\rho n\langle\sigma v\rangle\tau_E/4}
$$

For acceptable dilution ($f_{He} < 10%$), the requirement is approximately:

$$
\frac{\tau_{He}^*}{\tau_E} \lesssim 5-10
$$

Achieving this ratio demands efficient divertor operation — one of the most challenging engineering problems in fusion.


§10. Radiation Losses — Bremsstrahlung and Beyond

§10.1 Bremsstrahlung

Electrons decelerated in ion Coulomb fields emit bremsstrahlung radiation. This is the irreducible minimum radiation loss.

$$
p_{brem} = C_B n_e^2 Z_{eff} T_e^{1/2} \quad \text{where } C_B = 5.35 \times 10^{-37} \text{ W·m³·keV}^{-1/2}
$$

D-T at 15 keV, $n = 10^{20}$, $Z_{eff} = 1$:

$$
p_{brem} = 5.35 \times 10^{-37} \times 10^{40} \times 1 \times 3.87 = 2.07 \text{ kW/m}^3
$$

Compare with fusion power density: $p_{fus} \approx 183$ kW/m³. Ratio: $p_{fus}/p_{brem} \approx 88$. Bremsstrahlung is ~1% of fusion power — manageable for D-T.

§10.2 Impurity Radiation

Impurities catastrophically amplify radiation losses:

$$
Z_{eff} = \frac{\sum_j n_j Z_j^2}{n_e}
$$

Impurity Z At 1% concentration Impact on ignition
He (ash) 2 $Z_{eff}$ = 1.04 Minimal
Be (first wall) 4 $Z_{eff}$ = 1.16 Small
C (divertor) 6 $Z_{eff}$ = 1.36 Moderate
Fe (vessel) 26 $Z_{eff}$ = 3.25 Severe
W (divertor) 74 $Z_{eff}$ = 6.8 at 0.1% Catastrophic

Tungsten at 0.01% concentration ($n_W/n_e = 10^{-4}$): $\Delta Z_{eff} \approx 0.55$, and line radiation from partially-ionized tungsten at edge temperatures (1–5 keV) can exceed bremsstrahlung by 10–100×.

ITER uses a tungsten divertor. Controlling tungsten concentration to $< 10^{-5}$ is a critical operational requirement.

§10.3 Synchrotron Radiation

Electrons gyrating in $B$ emit synchrotron (cyclotron) radiation:

$$
p_{sync} = \frac{e^4 n_e B^2 T_e}{6\pi \epsilon_0 m_e^3 c^5} G(T, R_{wall}, a/R)
$$

where $G$ accounts for plasma reabsorption and wall reflection (typically $G \approx 0.1$–0.5).

For D-T at ITER conditions: $p_{sync}/p_{brem} \approx 0.1$. Minor.

For p-¹¹B at 300 keV, 12 T: $p_{sync}/p_{brem} \approx 0.3$–1.0. Significant additional loss.

§10.4 Summary: The Radiation Wall

Mechanism D-T (15 keV) D-³He (60 keV) p-¹¹B (300 keV)
Bremsstrahlung ~1% $P_{fus}$ ~110% $P_{fus}$ ~2300% $P_{fus}$
Synchrotron ~0.1% ~5% ~30-100%
Radiation/Fusion ratio ~1% ~115% ~2400%
Ignition feasible? Yes Marginal No (thermal)

p-¹¹B faces a radiation wall 23× higher than its fusion output. This is the Rider limit. No amount of improved confinement can overcome it for thermal plasmas — the radiation is an intrinsic property of the fuel.


§11. Thermal Stability and Burn Control

§11.1 Stability Criterion

A burning plasma is thermally stable at temperature $T_0$ if:

$$
\left.\frac{\partial}{\partial T}(P_\alpha - P_{loss} - P_{rad})\right|_{T_0} < 0
$$

If positive → perturbation amplifies (unstable). If negative → perturbation damps (stable).

§11.2 Analysis

$P_\alpha \propto \langle\sigma v\rangle \propto T^\nu$ where $\nu$ varies with T:

T range (keV) $\nu = d\ln\langle\sigma v\rangle/d\ln T$ Stability
5–10 ~4 Strongly unstable
10–15 ~2 Unstable
15–25 ~1 Marginally stable
25–40 ~0 to negative Stable

$P_{loss} \propto T^1$ (at constant $n, \tau_E$). $P_{brem} \propto T^{0.5}$.

Combined: stability requires $\nu < 1 + \epsilon$ (where $\epsilon$ accounts for radiation and scaling dependencies). Optimal: operate at 15–25 keV, on the high-T side of the reactivity peak.

§11.3 Burn Control Methods

Method Mechanism Response time Risk
NBI power Adjust beam injection ~1 s Slow for thermal excursions
ECRH/ICRH RF heating modulation ~0.1 s Faster, more precise
Fuel puffing Change $n$ → $P_{fus} \propto n^2$ ~0.5 s Affects confinement
Impurity injection Increase $P_{rad}$ ~0.1 s Fuel dilution risk
Pellet injection Localized density/cooling ~0.01 s MHD perturbation
Kill switch Massive gas injection ~10 ms Disruption risk

ITER's burn pulse (~400 s) provides time for active feedback. The thermal excursion timescale is ~$\tau_E \approx 3.7$ s — manageable but not generous.


§12. D-T Power Balance

§12.1 ITER Reference Case

$n = 10^{20}$ m⁻³, $T = 15$ keV, $\tau_E = 3.7$ s, $V = 830$ m³, $B = 5.3$ T:

Power Formula Value (MW)
$P_{fus}$ $\frac{n^2}{4}\langle\sigma v\rangle Q_{DT} V$ 500
$P_\alpha$ $0.20 \times P_{fus}$ 100
$P_n$ $0.80 \times P_{fus}$ 400
$P_{heat}$ $P_{fus}/Q$ 50
$P_{brem}$ $C_B n^2 T^{0.5} V$ ~5
$P_{sync}$ (subdominant) ~0.5
$P_{loss}$ $3nk_BTV/\tau_E$ ~145

Check: $P_\alpha + P_{heat} = 150$ MW. $P_{loss} + P_{brem} + P_{sync} = 150.5$ MW. ✓

§12.2 Energy Flow to Electricity

$$
P_{thermal} = P_n + P_{brem} + P_{loss} = 400 + 5 + 145 = 550 \text{ MW}
$$

$$
P_e = \eta_{th} \times P_{thermal} = 0.40 \times 550 = 220 \text{ MW}
$$

$$
P_{recirc} \approx \frac{P_{heat}}{\eta_{heat}} + P_{cryo} + P_{aux} \approx \frac{50}{0.50} + 30 + 20 = 150 \text{ MW}
$$

$$
P_{net} = 220 - 150 = 70 \text{ MW}
$$

At Q = 10, a D-T tokamak barely produces net electricity. This confirms ITER's role as a physics demonstrator, not a power plant prototype.

§12.3 Power Plant Scaling

A 1 GW_e plant requires $P_{fus} \approx 3000$ MW.

Approach B (T) $p_{fus}$ (MW/m³) Volume (m³) $R_0$ (m)
ITER-like 5.3 0.6 5000 ~9
SPARC/ARC 12 8.3 360 ~4
Next-gen HTS 20 65 46 ~2.5

The $p_{fus} \propto B^4$ scaling (at constant β) drives the entire compact reactor revolution. Doubling B reduces volume by 16×.


§13. D-D Power Balance

§13.1 Combined Reactions

$$
D + D \rightarrow \begin{cases} {}^3\text{He} (0.82) + n (2.45) & [50%] \ T (1.01) + p (3.02) & [50%] \end{cases}
$$

The tritium from the second branch burns in secondary D-T reactions, boosting effective yield:

$$
Q_{eff} \approx 3.65 + 0.5 \times 17.59 \times f_{burnup} \approx 7.5 \text{ MeV}
$$

§13.2 Power Density Comparison

At optimal $T = 50$ keV: $p_{fus,DD}/p_{fus,DT} \approx 0.04$. D-D produces ~4% of D-T power density.

Ignition triple product: ~17× harder than D-T. A D-D reactor requires either massive scale or breakthrough confinement.

Advantages: No tritium breeding. Unlimited fuel. Lower-energy neutrons (2.45 MeV vs 14 MeV) → less structural damage.


§14. D-³He Power Balance

§14.1 The Ideal Aneutronic Fuel

$Q = 18.35$ MeV, $f_{ch} = 1.0$. All energy in charged particles. Direct energy conversion at 60–80% efficiency is theoretically possible.

§14.2 Power Balance at 60 keV

At $n = 10^{20}$ m⁻³, $T = 60$ keV, $Z_{eff} = 1.3$:

$$
p_{fus} \approx 49 \text{ kW/m}^3, \quad p_{brem} \approx 54 \text{ kW/m}^3
$$

Bremsstrahlung ≈ fusion power. The margin is razor-thin. Any impurities, non-ideal confinement, or synchrotron radiation tips the balance negative.

§14.3 The D-D Side Reaction

A D-³He plasma contains deuterium, which undergoes D-D reactions producing neutrons. At optimal ratio $n_{^3He}/n_D = 1$: neutron contamination ~3%. The plasma is ~97% aneutronic.

§14.4 The ³He Supply Problem

Source Reserves Extraction cost Infrastructure needed
Terrestrial (tritium decay) ~8 kg/yr Moderate Tritium reactors
Lunar regolith 10⁶–10⁹ tonnes Very high Lunar mining base
Jupiter atmosphere Effectively unlimited Extreme Interplanetary flight

Circular dependency: Need D-³He engine to get ³He. Bootstrap with D-T propulsion → lunar mining → D-³He.


§15. p-¹¹B Power Balance — The Fundamental Challenge

§15.1 The Reaction

$$
p + {}^{11}B \rightarrow 3 , {}^4\text{He} \quad (Q = 8.68 \text{ MeV, fully aneutronic})
$$

Abundant terrestrial fuel (boron: 10 ppm in Earth's crust, seawater), zero neutrons, all charged products. If achievable, it solves every engineering problem of fusion simultaneously.

§15.2 The Quantitative Reality

At $T = 300$ keV, optimal mixture $n_p = 5n_B$ (charge balance $n_e = n_p + 5n_B = 10n_B$), $Z_{eff} = 3.0$:

Fusion power density:

$$
p_{fus} = n_p n_B \langle\sigma v\rangle Q_{pB} = \frac{5n_e}{6} \cdot \frac{n_e}{6} \cdot 3 \times 10^{-22} \cdot 8.68 \times 1.6 \times 10^{-13}
$$

At $n_e = 10^{20}$: $p_{fus} \approx 12$ kW/m³

Bremsstrahlung power density:

$$
p_{brem} = C_B n_e^2 Z_{eff} T^{0.5} = 5.35 \times 10^{-37} \times 10^{40} \times 3.0 \times 17.3
$$

$p_{brem} \approx 278$ kW/m³

Ratio: $p_{brem}/p_{fus} \approx 23$. The radiation wall is 23× higher than the fusion source.

Adding synchrotron ($\sim 30$–100 kW/m³ at 300 keV, 12 T): total radiation ~310–380 kW/m³ vs 12 kW/m³ fusion.

§15.3 The Rider Limit — Formal Statement

Rider (1997) proved that for a thermal (Maxwellian) p-¹¹B plasma, no combination of temperature and density achieves net energy gain when bremsstrahlung is properly accounted for. The power balance constraint:

$$
\frac{p_{fus}}{p_{brem}} = \frac{n_p n_B \langle\sigma v\rangle Q_{pB}}{C_B n_e^2 Z_{eff} T^{1/2}} < 1 \quad \text{for all } T
$$

The maximum of $\langle\sigma v\rangle / T^{1/2}$ is insufficient to overcome the $Z_{eff}$ amplification.

§15.4 Potential Escape Routes

Approach Mechanism Key paper Assessment
Beam-target Fast protons on cold boron; $T_e$ stays low Rostoker (1993) Promising but beam power is expensive
Resonance at 148 keV Concentrate ions at ¹²C* resonance Hora et al. (2017) Requires non-Maxwellian control
Laser-driven Picosecond laser ignites p-¹¹B target HB11 Energy Very early stage
Spin-polarized Aligned nuclear spins increase $\sigma$ by ~50% Kulsrud (1982) Depolarization in plasma unsolved
Direct conversion Recover bremsstrahlung as electricity 10–30% recovery; helps but doesn't close gap

§15.5 The Honest Bottom Line

For power plants: p-¹¹B ignition in thermal plasmas is physics-impossible. Non-thermal approaches face the thermalization problem: ion-ion collision times at relevant densities are ~microseconds, meaning any non-Maxwellian distribution relaxes to thermal equilibrium faster than it can be sustained by injection.

For propulsion (Vol.7): The calculus shifts. A spacecraft engine:

  1. Can tolerate $Q < \infty$ (carry external power; accept Q = 2–5)
  2. Benefits enormously from zero neutrons (no shielding mass)
  3. Needs charged products for magnetic nozzle thrust
  4. Operates at lower density (relaxes some constraints)

The path to a p-¹¹B engine may exist even if a p-¹¹B power plant does not. This asymmetry is the key insight driving TAE Technologies' strategy.


§16. The Lawson Diagram — Where We Are

§16.1 Distance to Ignition

Device Year $n\tau_ET$ (keV·s/m³) $\Pi/\Pi_{ign}$ Gap factor
T-3 (USSR) 1965 $10^{16}$ $3 \times 10^{-6}$ 300,000×
PLT (Princeton) 1978 $2 \times 10^{18}$ $7 \times 10^{-4}$ 1,500×
TFTR 1986 $1.5 \times 10^{20}$ 0.05 20×
JT-60U 1994 $1.53 \times 10^{21}$ 0.51
JET (D-T) 1997 $1.1 \times 10^{21}$ 0.37 2.7×
JET (D-T final) 2024 $1.4 \times 10^{21}$ 0.47 2.1×
ITER target ~2035 $3.5 \times 10^{21}$ 1.17
SPARC target ~2030 $2.5 \times 10^{21}$ 0.83 1.2×

The last factor of 2 has taken 30 years (1994–2024) and billions of dollars. ITER and SPARC aim to close it in the 2030s.


§17. ITER — The Burning Plasma Experiment

§17.1 Parameters

Parameter Value Significance
$R_0$ 6.2 m Largest tokamak ever
$a$ 2.0 m
$V$ 830 m³ ~500× SPARC
$B_0$ 5.3 T Nb₃Sn superconductor
$I_p$ 15 MA Largest plasma current
$P_{fus}$ target 500 MW
$P_{heat}$ 50 MW NBI + ICRH + ECRH
Q target ≥ 10 First burning plasma
$\tau_E$ target 3.7 s
Pulse 400 s (inductive)

§17.2 What ITER Demonstrates

  1. First burning plasma in history ($f_\alpha > 0.50$)
  2. Alpha confinement and TAE stability at reactor $\beta_\alpha$
  3. Helium ash transport and exhaust at self-heated conditions
  4. Disruption mitigation at 350 MJ stored energy
  5. Tritium breeding blanket modules (6 test modules)
  6. Long-pulse superconducting operation

§17.3 What ITER Does Not Demonstrate

  1. Net electricity (no turbine)
  2. Tritium self-sufficiency (test blankets only)
  3. Material endurance at reactor-relevant neutron fluence
  4. Continuous steady-state operation
  5. Commercial economics

§17.4 Risk Assessment

Risk Probability Impact Mitigation
Further schedule delay High Schedule Parallel private programs
Q < 10 (alpha transport) Medium Physics Adjusted heating scenarios
Disruption at full parameters Medium Hardware SPI mitigation system
Tritium supply shortage Low–Medium Operations Canadian/Korean supply agreements
Cost overrun beyond €25B High Political Sunk cost commitment

§18. SPARC — The High-Field Compact Path

§18.1 The HTS Magnet Revolution

REBCO (Rare-Earth Barium Copper Oxide) high-temperature superconducting tape enables $B_{coil} \approx 20$ T. Since $p_{fus} \propto \beta^2 B^4$:

$$
\frac{p_{fus,SPARC}}{p_{fus,ITER}} \approx \left(\frac{12.2}{5.3}\right)^4 \approx 28
$$

28× higher power density in a device that fits in a gymnasium.

§18.2 Comparison

Parameter SPARC ITER Ratio
$R_0$ 1.85 m 6.2 m 0.30
$a$ 0.57 m 2.0 m 0.29
$B_0$ 12.2 T 5.3 T 2.3
$V$ 27 m³ 830 m³ 0.033
$P_{fus}$ ~140 MW 500 MW 0.28
$P_{fus}/V$ 5.2 MW/m³ 0.6 MW/m³ 8.7
Q target ≥ 2 ≥ 10

SPARC achieves 28% of ITER's fusion power in 3.3% of the volume. If successful, it validates the ARC power plant design (Q ≥ 25, $P_e$ = 525 MW, demountable magnets).


§19. NIF — Inertial Confinement

§19.1 Achievement

December 5, 2022: 3.15 MJ fusion from 2.05 MJ laser energy on target.

$$
Q_{target} = \frac{3.15}{2.05} = 1.54
$$

§19.2 The Efficiency Gap

NIF's 192 beams consume ~300 MJ electrical energy. Laser wall-plug efficiency: ~1%.

$$
Q_{wall-plug} = \frac{3.15}{300} \approx 0.01
$$

For ICF energy production: need 10–15% efficient lasers (diode-pumped) AND target gains of 50–100 AND 10 Hz repetition rate (consuming ~10⁶ targets/day).

§19.3 Assessment

NIF demonstrated the physics of ignition. The engineering path to ICF energy requires advances in all three axes: laser efficiency (~10×), target gain (~50×), repetition rate (~10⁶×). This is a different challenge from magnetic confinement and is pursued by companies like Focused Energy and First Light Fusion.


§20. Private Ventures — The New Landscape

§20.1 The Investment Surge

As of 2025, over $7 billion in private fusion investment. This changes the funding structure from government-monopoly to public-private partnership.

§20.2 Major Approaches

Company Concept Fuel target Investment Claimed timeline
CFS (SPARC/ARC) HTS tokamak D-T ~$2B Pilot plant ~2030s
TAE Technologies FRC + NBI D-T → p-¹¹B ~$1.2B Grid power ~2030s
Helion Energy Pulsed FRC, direct conversion D-³He ~$0.6B Demo ~2028
General Fusion Magnetized target fusion D-T ~$0.4B Demo ~2027
Zap Energy Sheared-flow Z-pinch D-T ~$0.2B Demo ~2030
First Light Projectile ICF D-T ~$0.1B Pilot ~2030s

§20.3 Critical Assessment

Advantages of private: Speed, innovation, capital efficiency, accountability.
Missing: Neutron testing facilities, tritium supply chain, regulatory framework, materials database.

Optimal strategy: Private builds compact reactors; government provides materials/tritium/regulatory infrastructure.


§21. Computational Analysis — Full Reproducible Code

§21.1 Environment

Python 3.10+
numpy >= 1.24
scipy >= 1.10
matplotlib >= 3.7

§21.2 Figures Generated

The companion code (executed during article generation) produces 6 figures:

  1. Fig. 1 — Lawson Diagram: $n\tau_E$ vs $T$ for D-T, D-D, D-³He, p-¹¹B ignition curves with experimental data points and ITER/SPARC targets.

  2. Fig. 2 — Q Contours: Constant-Q curves (Q = 1, 2, 5, 10, 20, 50, ∞) in the $n\tau_E$–$T$ plane for D-T, showing the operating space and experimental progress.

  3. Fig. 3 — Triple Product History: 60 years of progress from T-3 (1965) to ITER target, showing the "fusion Moore's law" and the remaining gap to ignition.

  4. Fig. 4 — Power Balance Comparison: Side-by-side bar charts of fusion power, charged-particle heating, bremsstrahlung, and transport losses for D-T (15 keV), D-³He (60 keV), and p-¹¹B (300 keV). Quantifies the radiation wall.

  5. Fig. 5 — Self-Heating Fraction: $f_\alpha$ vs Q for D-T and aneutronic fuels, marking JET, NIF, and ITER operating points.

  6. Fig. 6 — Burn Simulation: Left panel: temperature evolution from $T_0 = 8$ keV for Q = 5, 10, 30, 100. Right panel: $P_\alpha$, $P_{brem}$, $P_{loss}$ vs temperature showing the ignition crossover.

Complete source code (MIT license) available in the article's GitHub repository. All figures reproducible with python vol2_figures.py.


§22. Implications for Reactor Economics and Propulsion

§22.1 The Economic Equation

$$
LCOE = \frac{C_{capital} \cdot CRF + C_{O&M}}{P_{net} \cdot CF \cdot 8760}
$$

where $CRF$ = capital recovery factor, $CF$ = capacity factor.

For fusion to compete with fission (~$60–80/MWh) or renewables+storage (~$40–80/MWh), the requirements are:

  • $Q \geq 25$ (minimize recirculating power)
  • $CF > 0.85$ (steady-state preferred → stellarators or advanced tokamaks)
  • Compact design ($C_{capital} < $10B$) → HTS magnets

§22.2 Propulsion: A Different Optimization

For propulsion, the figure of merit is specific power $\alpha$ (W/kg):

$$
\alpha = \frac{f_{ch} \cdot \eta_{nozzle} \cdot P_{fus}}{M_{reactor} + M_{shield} + M_{power}}
$$

Engine $I_{sp}$ (s) $\alpha$ (kW/kg) Best mission
Chemical (LH2/LOX) 450 10,000 LEO, inner planets
Nuclear thermal 900 100 Mars
D-T fusion 100,000 1–10 Outer planets
D-³He fusion 300,000 1–10 Interstellar precursor
p-¹¹B fusion 500,000 0.5–5 Deep space (if feasible)

A sub-ignition p-¹¹B engine (Q = 3) with direct conversion ($\eta = 60%$) and no neutron shielding could outperform a D-T ignited engine on net thrust-to-weight — because the shielding mass saved exceeds the external power source mass. This reversal only applies to space, not ground power.


§23. Uncertainties and Limitations

  1. Alpha transport in burning plasmas is extrapolated from sub-reactor experiments. TAE/EPM instabilities may reduce self-heating efficiency by 10–30% in ITER.
  2. IPB98(y,2) confinement scaling has ~15% scatter. ITER Q predictions range from ~7 to ~15.
  3. p-¹¹B reactivity parameterization is approximate. Resonance structure at 148 and 620 keV is simplified.
  4. Helium ash transport modeling assumes neoclassical behavior; anomalous helium transport is poorly characterized.
  5. NIF target physics details are partially classified.
  6. Private company timelines are self-reported. Independent verification is limited.
  7. Synchrotron radiation at $T > 100$ keV depends on wall reflectivity and plasma opacity — poorly constrained parameters.
  8. Economic projections assume learning-curve cost reductions that have not been demonstrated for fusion.

§24. References

  1. Lawson, J.D. (1957). "Some criteria for a power producing thermonuclear reactor." Proc. Phys. Soc. B, 70, 6.
  2. Freidberg, J.P. (2007). Plasma Physics and Fusion Energy. Cambridge University Press.
  3. Wurzel, S.E. & Hsu, S.C. (2022). "Progress toward fusion energy breakeven." Phys. Plasmas, 29, 062103.
  4. ITER Physics Expert Groups (1999). "Energetic ions." Nuclear Fusion, 39, 2471.
  5. Fasoli, A. et al. (2007). "Energetic ions." Nuclear Fusion, 47, S264.
  6. Heidbrink, W.W. (2008). "Alfvén instabilities from energetic particles." Phys. Plasmas, 15, 055501.
  7. Rider, T.H. (1997). "Fundamental limitations on fusion systems." Phys. Plasmas, 4, 1039.
  8. Nevins, W.M. (1998). "Confinement for advanced fuels." J. Fusion Energy, 17, 25.
  9. Keilhacker, M. et al. (1999). "D-T in JET." Nuclear Fusion, 39, 209.
  10. Abu-Shawareb, H. et al. (2024). "Target gain > 1." Phys. Rev. Lett., 132, 065102.
  11. Creely, A.J. et al. (2020). "SPARC overview." J. Plasma Physics, 86, 865860502.
  12. Binderbauer, M.W. et al. (2015). "High-performance FRC." Phys. Plasmas, 22, 056110.
  13. Gota, H. et al. (2021). "C-2W overview." Nuclear Fusion, 61, 106039.
  14. Putvinski, S.V. et al. (2019). "pB11 reactivity revisited." Nuclear Fusion, 59, 076018.

Series Navigation
[← Vol.1: Nuclear Physics & Confinement] | Vol.2: Ignition, Burn & Power Balance | [Vol.3: Materials, Tritium & Engineering →]

MIT License. Reproduce, extend, critique freely.
All code reproducible. All claims verifiable.

Truth belongs to no one.

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