9 parallel-computing-numerical-methods positions at BIOMEDICAL SCIENCES RESEARCH CENTRE "ALEXANDER FLEMING" in Australia
Sort by
Refine Your Search
-
Category
-
Program
-
Field
-
cooperating with each other, but in many cases competing for individual gains. This structure may not always work for the benefit of science. The purpose of this project is to use game theory and computational
-
events with the GOTO telescope network. Projects focussing on thermonuclear bursts will involve analysis of new and archival data from satellite-based X-ray telescopes, and running numerical models
-
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
-
for indigenising the curriculum across the Faculty’s Schools (Architecture, Design and Planning, Chemical Engineering, Civil Engineering, Electrical Engineering and Computer Science, and Mechanical and Mining
-
AUSTRALIAN NATIONAL UNIVERSITY (ANU) | Canberra, Australian Capital Territory | Australia | 3 months ago
award through the Science in Australia Gender Equity (SAGE) program, and a platinum member of the Australian Disability Network. We welcome applications from people of all backgrounds and identities
-
that shows you are from a regional or remote location. Payment Method Payments will be made directly into recipient's nominated bank account in the following instalments: The scholarship will be paid over
-
working options, health and wellbeing programs, a heavily discounted Study for Staff program, on‑campus childcare, affordable parking, salary packaging, and cultural leave. UQ is committed to Aboriginal and
-
and be undertaking research in a field related to neurodegenerative diseases in the year for which the scholarship is awarded Not hold a Research Training Program (RTP) Scholarship (Stipend) or a
-
I work on the study of massive and supermassive stars (10-100,000 solar masses); the first generations of stars in the universe (Pop III stars); evolution of rotating massive stars and the spin of their remnants (including predictions for GW sources); mixing and transport processes in the...