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Skip to Search Results- 2Achal, Roshan
- 2Anagaw, Amsalu Y.
- 2Antolak, John Anthony.
- 2Avendano Nandez, Jose L
- 2Chen, Ke
- 2Chen, Yunfeng
- 14Particles (Nuclear physics)
- 10Geophysics
- 10Inversion
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Results for "departments_tesim:"Department of Physics""
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A Study of the Detection of Long-Lived Charged Particles With an Auxiliary Detector Above the ATLAS Muon Spectrometer (ADAM)
DownloadFall 2023
The Auxiliary Detector above the ATLAS Muon spectrometer (ADAM) is a proposed particle detector. Its function is to detect the decay products of beyond the standard model (BSM) particles produced in the 14 TeV proton-proton collisions at the Large Hadron Collider (LHC) which evade detection by...
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Magnetotelluric Investigations of the Tintina Fault Zone for Geothermal Exploration at Watson Lake, Yukon
DownloadFall 2023
Geothermal energy is being investigated as a renewable source of electricity and heat production for communities in northern Canada. The successful development of a geothermal energy project requires three key components: (1) there must be a source of sufficient heat at near-surface depths....
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Physical Interpretation of Radiative Corrections: Electron g -2, Lamb Shift, and the D-term
DownloadFall 2023
Gravitational interaction of particles is understood in terms of energy-momentum tensor (EMT) which gives information regarding the fundamental properties of a particle like mass and spin. When the matrix element of the energy-momentum tensor is written in terms of EMT form factors, we get an...
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Fall 2023
This thesis aims to provide a method to include the effect of the gravitational fields of binary systems when simulating them with one-dimensional stellar evolution codes. We also apply this method to simulate the evolution of binary systems until the donor fills its Roche Lobe. The first part of...
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The Missing Supernova Remnant Problem: Searching for Galactic Supernova Remnants with EMU & POSSUM
DownloadFall 2023
Supernova remnants (SNRs) are an important part of the stellar feedback cycle that regulates star formation and influences the evolution of galaxies. They disperse the heavy elements formed in the cores of massive stars back into the interstellar medium, are responsible for forming and destroying...
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Clusters, Clouds, and Correlations: Relating Young Clusters to Giant Molecular Clouds in M33 and M31
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Using young clusters and giant molecular clouds (GMCs), we constrain timescales and distances involved in the star formation process in the Triangulum (M33) and Andromeda (M31) galaxies. The young star clusters come from the PHATTER catalogue, with 1214 clusters in M33 and the PHAT catalogue,...
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Fall 2023
The IceCube neutrino observatory is a gigaton Cherenkov detector located at the geographic south pole. The experiment is designed to detect neutrinos originating from the atmosphere and astrophysical objects over a huge energy range from 10 GeV to 10 PeV. Information about the interacting...
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Searches for Magnetic Monopoles and Highly Ionising Particles at 13 TeV at the LHC with MoEDAL
DownloadFall 2023
The standard model of particle physics describes the experimental data collected to date remarkably well. However, this theory (the standard model of particle physics) does not provide a complete description of reality. What is dark matter and what is the origin of dark matter? How do we explain...
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Numerical investigation of the superfluid transition in low dimensions and in anisotropic systems
DownloadSpring 2023
The main theme of this thesis is the superfluid transition in reduced dimensions and in anisotropic and inhomogeneous systems. Using state-of-the-art computational methodology, we carry out large-scale, numerically exact computer simulations to study this topic, making use of classical and...
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Spring 2023
The study of energetic particles of solar and cosmic origin, and those accelerated in the planetary magnetopause, is integral to our developing understanding of the physical processes affecting space radiation in near-Earth space, interplanetary space, and Earth's upper atmosphere. In particular,...