11 high-performance-computing positions at BIOMEDICAL SCIENCES RESEARCH CENTRE "ALEXANDER FLEMING" in Australia
Sort by
Refine Your Search
-
Listed
-
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
-
exposed to laser-accelerated intense proton beams. Primarily, the tasks are to be done by means of analytical calculations and high-performance computing simulations in a strong link with the industrial
-
-accelerated intense proton beams. Primarily, the tasks are to be done by means of analytical calculations and high-performance computing simulations in a strong link with the industrial partner (HB11 Energy
-
Learning Enhancement Team. In this role, you will provide high-level administrative and professional support for innovative teaching and learning projects, working closely with the Senior Educational
-
to JCU Entry options Application due dates Fees and financial support Information for High School students International students Mature students Indigenous Australians Parents and guardians Schools and
-
role of noncoding RNAs during flavivirus infection. The role contributes to high-impact research focused on viral infection outcomes, antiviral responses, and viral pathogenesis. Working within
-
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
-
engineering with a strong background in electromagnetic methods and data analysis who can contribute towards our program of research. This exciting opportunity involves conducting research
-
with external parties. Demonstrated high level of computer literacy and/or database skills, preferably large, complex databases and a demonstrated ability to adapt to new IT environments. Demonstrated
-
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...