This PhD opportunity at Monash University, supervised by Professor Amanda Karakas within the Centre of Excellence for Astrophysics in 3D (ASTRO 3D), focuses on stellar astrophysics, particularly the study of low and intermediate-mass stars. The research group investigates stars with masses similar to or slightly larger than the Sun, exploring their evolution, nucleosynthesis, and the origin of elements in the Universe.

Students will engage in numerical simulations and theoretical studies to address fundamental questions such as the origin of carbon and other elements, the processes occurring during the red giant phase, and the impact of binary companions on stellar evolution and element production. Projects include studying weak CN stars in the Magellanic Clouds, stellar mergers, the effects of new carbon burning rates on the AGB-supernovae mass boundary, and the connection between novae and Type Ia supernovae. Collaborative opportunities exist with Professors Ilya Mandel and Alexander Heger.

As part of ASTRO 3D, students will interact with astronomers across Australia and internationally, gaining exposure to diverse fields such as cosmology, galaxy evolution, and advanced computational astrophysics. The group environment is supportive and research-driven, offering access to cutting-edge resources and expertise.

Applicants should have a strong background in physics, astronomy, or related fields, with experience in computational or theoretical methods being advantageous. English language proficiency is required. For further details or to discuss alternative project arrangements, prospective students are encouraged to contact Prof Amanda Karakas directly.

To apply, visit the Monash University Physics postgraduate project portal and review the available PhD positions. Prepare your academic transcripts, CV, and a statement of research interests. Early contact with the supervisor is recommended to tailor the project to your interests and background.