posted on 2026-01-07, 04:41authored byValentina Di Marco
This thesis explores one of the most exciting frontiers in astrophysics: the search for gravitational waves, ripples in space and time created by the collision of supermassive black holes in distant galaxies. The work uses pulsar timing arrays, a network of extremely precise cosmic clocks, to distinguish genuine gravitational wave signals from background noise and instrumental effects that can mimic them. By testing and refining detection methods, the research shows how to avoid false alarms and how to extract reliable information from these faint cosmic hum. The results strengthen the foundations of this new window on the universe and its most powerful events.
History
Campus location
Australia
Principal supervisor
Eric Thrane
Additional supervisor 1
Ryan Shannon
Additional supervisor 2
Andrew Zic
Year of Award
2026
Department, School or Centre
Physics and Astronomy
Course
Doctor of Philosophy
Degree Type
DOCTORATE
Faculty
Faculty of Science
Rights Statement
The author retains copyright of this thesis. It must only be used for personal non-commercial research, education and study. It must not be used for any other purposes and may not be transmitted or shared with others without prior permission. For further terms use the In Copyright link under the License field.