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supergiant stars right before the explosion Searching different astrophysical channels that produce r-process elements Connecting the properties of long-duration gamma-ray bursts and associated supernovae web
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proficiency skills, to undertake a PhD in the Faculty of Arts are available at www.arts.monash.edu/graduate-research/application-process/ . Applicants should familiarise themselves with these requirements
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: Prospective applicants must hold current registration as a Registered Nurse with AHPRA and satisfy Monash University PhD entry requirements as outlined in the Monash Graduate Research Admission Procedure
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I offer projects broadly related to supernova explosions and the final stages in the lives of massive stars. Specific topics of interest include fluid dynamics processes in stellar explosions and
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is open to negotiation within the Initiative’s aims, and may include (for example): a focused study of antisemitism in a defined period (e.g., Federation to WWII; post-war Australia; late-20th century
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Process: To submit an Expression of Interest (EOI), please: Check your eligibility. Ensure you meet Monash University’s minimum entry requirements for a PhD and English Language Proficiency standards
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research spanning policy, society and sustainability Experience working with policy actors or applied research contexts How to Apply This position has a two-stage selection process. Stage 1: Expression of
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are supported by quantum mechanical theoretical formalisms. Our fundamental findings yield promise for future applications in electronics, optoelectronics, spintronics, information processing and storage, sensing
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spectroscopy and Gaia data of star clusters to decipher the mystery of the Lithium-rich giant stars" (with Prof John Lattanzio) "The origin of the heavy elements: Computer simulations of neutron-capture
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of living evidence in APTs. Activities will involve conducting a needs analysis and process map of potential high-value decision points within APTs that would benefit from living evidence. The student will