For several decades since its inception, Einstein's general theory of
relativity stood somewhat aloof from the rest of physics. Paradoxically,
the attributes which normally boost a physical theory - namely, its
perfection as a theoreti- cal framework and the extraordinary
intellectual achievement underlying i- prevented the general theory from
being assimilated in the mainstream of physics. It was as if
theoreticians hesitated to tamper with something that is manifestly so
beautiful. Happily, two developments in the 1970s have narrowed the gap.
In 1974 Stephen Hawking arrived at the remarkable result that black
holes radiate after all. And in the second half of the decade, particle
physicists discovered that the only scenario for applying their grand
unified theories was offered by the very early phase in the history of
the Big Bang universe. In both cases, it was necessary to discuss the
ideas of quantum field theory in the background of curved spacetime that
is basic to general relativity. This is, however, only half the total
story. If gravity is to be brought into the general fold of theoretical
physics we have to know how to quantize it. To date this has proved a
formidable task although most physicists would agree that, as in the
case of grand unified theories, quantum gravity will have applications
to cosmology, in the very early stages of the Big Bang universe. In
fact, the present picture of the Big Bang universe necessarily forces us
to think of quantum cosmology.