of the ore columbite in the British Museum in London and isolated
from it the new element. He named it columbium, but it was
rediscovered nearly 50 years later and called niobium, now its
standard name. Niobium has the highest transition temperature of
any element (9.3K) and it turns out that alloys of it give some of the
most useful superconductors. In 1941, niobium carbide was
discovered to be a superconductor at 16K, the record at the time,
and therefore it seemed that useful superconductors might be
found by choosing the right alloy. But how to choose? Although
there are only a certain number of chemical elements, the number
of possible chemical compounds or alloy compositions is virtually
unlimited. This is because there are countless ways of combining
elements in different proportions. To make progress in this area
required a special type of mind.
Bernd Matthias was born in Frankfurt and studied at ETH in
Zurich in the late 1930s, doing a doctorate with the Swiss physicist
Paul Scherrer during the Second World War. He came to the
United States in 1947 and spent the rest of his life working in
various laboratories, including in Chicago, Bell Labs, Los Alamos,
and San Diego. His passion was the quest to discover new
materials and he pursued this quest with energy, ingenuity, and
zeal. Matthias wanted to find which of the many different possible
alloy compositions would provide useful superconductors. To
participate in this new field of research, you need to have an
instinctive knowledge of chemistry and be skilled at various
techniques of chemical preparation. There were so many
compositions to search through, it cannot be done at random;
Matthias had to trust his instincts.
Bernd Matthias was deeply distrustful of theorists. He was a very
late convert to the BCS theory (not really accepting it until many
years after everyone else had) and was very aggressive about
anything he thought smacked of theoretical jiggery-pokery (he was
particularly antagonistic to the idea of ‘organic superconductors’,
which were first being talked about in the 1960s [see Chapter 8 and 9],
91
Before the breakthrough