PhD Position in Final Stages of Massive Stars: Gamma-Ray Bursts, Supernovae, and Kilonovae Monash University in Australia

This PhD position at Monash University offers an exciting opportunity to investigate the dramatic final stages of massive stars, focusing on their explosive deaths as gamma-ray bursts, supernovae, and kilonovae. The research is led by Dr Manisha Shrestha, whose work combines multi-wavelength observational data with advanced simulations to unravel the mysteries of stellar evolution and cosmic transients. Students will have the chance to participate in international collaborations such as OzGrav Centre of Excellence for Gravitational-wave Discovery, Distance Less than 40 Mpc, SAGUARO, and the Global Supernova Project.

Potential student projects include constraining the mass loss rate of red supergiant stars immediately before explosion, exploring astrophysical channels that produce r-process elements, and connecting the properties of long-duration gamma-ray bursts with their associated supernovae. The research environment is highly collaborative, offering access to cutting-edge observational facilities and simulation tools.

Applicants should have a strong academic background in physics, astronomy, or a related discipline, with experience in observational data analysis or computational simulations considered advantageous. A bachelor's or master's degree is required, and candidates must meet Monash University's English language proficiency standards. Funding details are not specified in the position description, so applicants are encouraged to inquire directly with Dr Shrestha for further information.

The application process involves visiting the Monash University Physics postgraduate project page and submitting an application via the provided link. For additional project arrangements or questions, candidates may contact Dr Manisha Shrestha by email. This position is ideal for students passionate about astrophysics, stellar evolution, and the study of explosive cosmic phenomena.