A metal foam, as one might expect, is a dispersion of gas bubbles
in a metallic bulk material. These extremely lightweight materials (density of around 0.25 g/cm3) have some
very promising properties; including high specific stiffness,
very good energy-absorption, low thermal conductivity and outstanding absorption of
electromagnetic waves. Because of these interesting properties, metal foams have a number of potential applications - such as
crash protection material for cars, building material for wall cladding and sound-proofing.

One way of achieving this is to produce a precursor material, such as aluminium mixed with a small amount of titanium hydride (0.5 wt% of TiH2). Once heated up in the region of 660°C the aluminium melts and becomes liquid, while the TiH2, known as the blowing agent, decomposes to release hydrogen gas. This gas thus forms the bubbles and creates a highly porous structure.
The characterisation of metal foams, in terms of morphology and properties, has received much attention in recent years. However, little research has appeared which tackles the true mechanisms of metal foam formation - that is to say, how the foam emerges from the liquid, how it changes with time and how gravity influences the mechanisms of foam formation.

In order to get a better understanding of the various mechanisms of foam growth, coalescence and gravity-induced liquid drainage, a number of scientists are now investigating inside metal foams using X-ray radioscopy and ultrasound techniques. These in-situ techniques allow one to see inside the material and observe the internal configuration of the metal foam in real-time - something that was previously impossible.
