the quantum story
xviii
particle of the gravitational force. This early promise faded, however, as
different variants of superstring theory emerged and it lost any sense of
uniqueness. Around the same time, the canonical approach was resur-
rected in the form of loop quantum gravity. Superstring theory experi-
enced something of a renaissance in March 1995, in the second superstring
revolution, and today dominates contemporary theoretical physics.
But there is growing impatience with the superstring programme’s
obsession with obscure hidden dimensions and its inability to make any
kind of testable prediction. As has happened so often in its glorious 110-
year history, quantum theory is once again in crisis. This section closes
with an exploration of the role that interpretation, an obsession among
physicists since the theory’s inception, might still have yet to play.
The book concludes optimistically with, if you will, a quantum of sol-
ace. It has cost £3.5 billion and frustratingly blew up days after it was fi rst
switched on in September 2008, but the Large Hadron Collider (LHC)
at CERN in Geneva gives some hope of resolving the current crisis. At
worst, the LHC will simply confi rm the existence of the Higgs boson,
validating the mechanism of spontaneous symmetry-breaking, explain-
ing how particles acquire mass, and putting the icing on the cake of the
Standard Model. At worst, the LHC will provide answers.
At best, the LHC will turn up some bizarre new experimental facts; facts
that simply can’t be accommodated in the current quantum fi eld theories
that constitute the Standard Model, and the crisis will deepen. Physics will
then truly come alive once again. Only from the depths of despair are we
likely to see the breakthroughs needed to propel quantum theory on the
next stage of its journey. At best, the LHC will beg questions.
Many of the ‘moments’ I have chosen to describe in this book suggest
themselves as unambiguously key events in quantum theory’s history.
Others are a little less obvious and some have been chosen in an effort
to maintain narrative consistency and fl ow. Whilst I make no apologies
for my choices, I am very conscious of the risk that, taken together, these
moments may be perceived to describe a smooth, irresistible progression
towards some inexorable scientifi c truth.
This is just not how science works. It has not been possible to describe
here all the blind alleys, the dead ends, the theories that dominated for