Sort by
Refine Your Search
-
-ray speckle-based imaging, a simple and flexible technique using just a piece of sandpaper as an optical element to access the phase-contrast and dark-field image modalities. Using this method, I
-
qualitative, quantitative, mixed, or interdisciplinary methods. Possible PhD directions include (for example): antisemitism in news media, online platforms, and public discourse (content/discourse analysis
-
; contemporary roots) institutional histories (political parties, unions, churches, education systems, universities, government agencies) historical analysis of antisemitic discourse in Australian print culture
-
project. The details of the PhD project are open to negotiation, but it may involve media content analysis, community surveys, and interviews with key stakeholders such as community members, industry and
-
approved by both GLaWAC and Professor David at Monash. Applications that focus on specialised topics such as those relating to archaeological faunal remains, geoarchaeology, stone artefact analysis
-
cosmolgy, galaxy evoltion and stellar astrophysics. Students in my group primarily perform numerical simulations of stars, in order to study broad questions related to the origin of the elements in
-
supergiant stars right before the explosion Searching different astrophysical channels that produce r-process elements Connecting the properties of long-duration gamma-ray bursts and associated supernovae web
-
stellar interiors, birth properties of black holes and neutron stars, supernova light curves and spectra, gravitational waves, neutrino astrophysics, the production of heavy elements stellar explosions, and
-
develop skills in artistic research methodologies, interdisciplinary research processes, and qualitative analysis, benefiting from expert supervision from research leaders in music, creative collaboration
-
of their remnants (including predictions for GW sources); mixing and transport processes in the stellar interior; nucleosynthesis and the origin of elements, including galacto-chemical evolution - which elements