Gravitational Wave Detectors
1979
As outlined in the preceding talk by Dr Thorne, there are many possible sources of
gravitational radiation, ranging from the interactions of supermassive black holes
to supernova explosions of stars. Detection of such radiation could give information
which cannot be obtained otherwise, for example on events occurring in the cores
of stellar systems, and could also provide important clues on the existence, nature
and behaviour of black holes.
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