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Full-Text Articles in Physical Sciences and Mathematics
Radio Insights Into Gamma-Ray Mysteries, Seth M. Bruzewski
Radio Insights Into Gamma-Ray Mysteries, Seth M. Bruzewski
Physics & Astronomy ETDs
In the time since its launch, the \textit{Fermi Gamma-Ray Space Telescope} has provided new and unparalleled views of the $\gamma$-ray sky, dramatically increasing our understanding of sources of high-energy radiation. During that same time, however, its ``unassociated'' sources have provided a consistent mystery: approximately one third of the modern gamma-ray sky remains completely unaccounted for in other electromagnetic regimes. While some of the fainter sources simply pose challenges in achieving the necessary signal-to-noise ratio, others are well constrained and have resisted traditional investigations for years, and in some cases, for over a decade. Radio astronomy has traditionally been the best …
Using Natural Phenomena To Study The Ionosphere, Joseph Benjamin Malins
Using Natural Phenomena To Study The Ionosphere, Joseph Benjamin Malins
Physics & Astronomy ETDs
This dissertation explores novel techniques for observing the ionosphere using natural signals. The ionosphere is a region of plasma hundreds of kilometers above the Earth that affects communication and remote sensing applications across the world. Traditional techniques for observing the ionosphere involve using man made radio signals, either to reflect the signal at HF frequencies or to pass several signals through the ionosphere and compare the difference the ionosphere makes in the signals. However, such techniques are limited by the ability of equipment to produce these signals and by the numerous laws and regulations governing transmission of signals in the …
Searching For Supermassive Binary Black Holes And Their Gravitational Waves, Karishma Bansal
Searching For Supermassive Binary Black Holes And Their Gravitational Waves, Karishma Bansal
Physics & Astronomy ETDs
The recent discovery of gravitational waves (GWs) by the LIGO collaboration has opened a new observing window on the universe, but it is limited to the GWs in the frequency range of 10-1000 Hz. The main motivation of this thesis is to consider the possibility of detecting low frequency (nHz) GWs. In the pursuit of these waves, we need to understand their source of origin and build a detector with the required sensitivity. Low-frequency waves are expected as a result of coalescing binary supermassive black holes (SMBBHs). We hope to detect these waves in the near future using pulsar timing …