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Searching for neutrino emissions from the Galactic Center region
Dissertation   Open access

Searching for neutrino emissions from the Galactic Center region

Xinyue Kang
Doctor of Philosophy (Ph.D.), Drexel University
Sep 2024
DOI:
https://doi.org/10.17918/00010739
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Abstract

Neutrino astrophysics Deep space--Galactic center
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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