Gravitational-Wave Detection Using Pulsars: Status of the Parkes Pulsar Timing Array Project
The first direct detection of gravitational waves may be made through observations of pulsars. The principal aim of pulsar timing-array projects being carried out worldwide is to detect ultra-low frequency gravitational waves (f ~10-9-10-8 Hz). Such waves are expected to be caused by coalescing supe...
| Main Authors: | , , , , , , |
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| Format: | Journal Article |
| Published: |
CSIRO
2009
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| Subjects: | |
| Online Access: | http://hdl.handle.net/20.500.11937/17672 |