The Galactic Center, home to the supermassive black hole Sagittarius A*, has long intrigued astrophysicists due to its dynamic environment and diverse astrophysical objects. High-energy gamma-ray observations by H.E.S.S. suggest sources emitting up to PeV energies, prompting searches for high-energy neutrinos to confirm hadronic acceleration. Recent high-energy neutrino emissions detected by the IceCube Neutrino Observatory from the Galactic Plane have further heightened interest in this region. This thesis presents a specialized neutrino dataset designed for the Galactic Center, optimized to detect softer spectrum sources and confined to a narrow sky region. This dataset, distinct from previous IceCube datasets, aims to achieve an elevated per-steradian event rate for the Galactic Center by excluding data from the rest of the sky, leading to a higher signal rate. This also leads to a higher background rate, therefore, to counter this, a more sensitive, time-dependent single-flare search is employed, targeting the Galactic Center, particularly for flare durations of less than one hour with a power law spectral index of 2.7.
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Title
Searching for Neutrino Emissions from the Galactic Center Region
Creators
Xinyue Kang
Contributors
Naoko Kurahashi Neilson (Advisor)
Awarding Institution
Drexel University
Degree Awarded
Doctor of Philosophy (Ph.D.)
Publisher
Drexel University; Philadelphia, Pennsylvania
Number of pages
x, 53 pages
Resource Type
Dissertation
Language
English
Academic Unit
College of Arts and Sciences; Physics; Drexel University
Other Identifier
991021903507804721
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