Sort by
Refine Your Search
-
Listed
-
Category
-
Employer
-
Field
-
Change lives and change the world with an impactful PhD as a component of the Long-term Trials of Drought Resilient Farming Practices Grants, Future Drought Fund (Australian Government) project
-
Eligibility Essential eligibility criteria include: A Honours or Masters degree with a thesis component in a relevant public health, medical, nursing, allied health field or digital health communication field
-
Fellowship at LMU Munich, and a postdoc position at RMIT University. My nanophotonics research seeks to uncover the underlying physics in structured light-matter interactions at nanoscale. We aim to develop
-
known as Team COMPAS -- includes a number of amazing undergraduate and graduate students, postdocs, alumni, and other fantastic collaborators. Please contact me if you are interested in joining our group
-
theoretical colleagues. All research takes place within our dynamic particle physics research group with academics and postdocs, as well as graduate and undergraduate students. Some work will be purely
-
I supervise a wide range of projects stellar astronomy. They include modelling stars in 1D or 3D, deciphering the origin of the elements (stellar nucleosynthesis), and observing using optical
-
strengthen their applications by demonstrating strong research potential, which may include: Completion of a degree with a substantial research component (at least 25%), such as an Honours degree or higher
-
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
-
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
-
; trying to understand why certain elements are more abundant than others; or how the different populations of stars in globular clusters arose. How can we better approximate mixing during core He burning