This decommissioned ERA site remains active temporarily to support our final migration steps to https://ualberta.scholaris.ca, ERA's new home. All new collections and items, including Spring 2025 theses, are at that site. For assistance, please contact erahelp@ualberta.ca.
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Unique cellular interactions between the obligate intracellular bacteria Wolbachia pipientis and its insect host
DownloadFall 2011
Wolbachia are maternally inherited obligate intracellular bacteria found in arthropods, where they induce feminization, male-killing, parthenogenesis, and cytoplasmic incompatibility (CI). CI is conditional male sterility, in which Wolbachia-infected males successfully mate with infected females,...
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Fall 2009
Integrations over the unitary group are required in many applications including the joint eigenvalue distributions of the Wishart matrices. In this thesis, a universal integration framework is proposed to use the character expansions for any unitary integral with general rectangular complex...
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Unity, Diversity, Anonymity: An ethno-linguistic portrait of the Spanish speaking population of Edmonton, AlbertaUnidad, diversidad, anonimidad: un retrato etnolingüístico de la población hispanohablante de Edmonton, Alberta, Canadá
DownloadFall 2009
This thesis describes the role of Spanish as a common language in the construction of social networks among the diverse Spanish-speaking population of Edmonton, Alberta, Canada. Analysis of the data confirms the low public visibility of the community observed initially, despite the even larger...
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Universal Control and Management Strategies for Micro-Grid-Based Smart Grids Using Synchronous Converters
DownloadFall 2014
The energy sector is moving into the era of distributed generation (DG) and micro-grids (MGs). This research focuses on development of a new family of control and management strategies for integration of micro-grids with numerous voltage source converters and synchronous generators in smart...
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Fall 2022
Neutron stars are interesting due to their extremely large densities (∼ 1015 g/cm^3), and also because the accretion of matter from a companion star can spin them up to very high frequencies (∼716 Hz based on observations ). When we study black holes (BH), the only thing that we have to worry...