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The First Wall

Material Science at the Edge of a Star

The greatest barrier to clean energy isn't the sun—it's the container we build to hold it.

Strategic Objectives

• Master the metallurgy of refractory metals like tungsten and beryllium.

• Understand the atomic-level degradation caused by intense neutron flux.

• Explore cutting-edge solutions for heat exhaust and thermal management.

• Identify the material breakthroughs required for the success of ITER and DEMO.

The Core Challenge

Nuclear fusion promises infinite power, but the 'first wall' materials currently melt, erode, and fail under the most extreme conditions in the known universe.

01

The Fusion Environment

02

The First Wall Architecture

03

Beryllium: The Low-Z Candidate

04

Tungsten: The Refractory Giant

05

Heat Flux Fundamentals

06

Physical Sputtering Mechanisms

07

Chemical Erosion Dynamics

08

Neutron Irradiation Effects

09

Helium Embrittlement

10

Thermal Shock and Fatigue

11

Tritium Retention and Inventory

12

Plasma-Facing Components (PFCs)

13

Advanced Refractory Alloys

14

Liquid Metal Walls

15

Surface Microstructure Evolution

16

Material Characterization Techniques

17

The Role of Neutron Sources

18

Joining Dissimilar Materials

19

Computational Materials Science

20

The ITER Research Plan

21

The Road to DEMO

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