DR. NORHASLIZA BINTI YUSOF
Department of Physics
Faculty of Science
norhaslizayum.edu.myView CV | |
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Biography | |
Dr. Norhasliza Yusof is a senior lecturer in the Department of Physics at the University of Malaya, specializing in computational physics, stellar evolution, and nuclear astrophysics. She earned her PhD and MSc in Theoretical Nuclear Astrophysics, as well as a BSc in Applied Physics, all from the University of Malaya. Additionally, she was awarded the prestigious Commonwealth Split-Site PhD Scholarship, which allowed her to conduct part of her doctoral research at Keele University, enhancing her expertise in astrophysics and fostering international collaboration. Her research focuses on the evolution and fate of very massive stars, the impact of rotation on stellar models, and neutrino emissions in massive stars. Notable publications include studies on the R136 star cluster, which hosts several stars exceeding the previously accepted 150 solar mass limit, and the development of grids of stellar models with rotation at various metallicities. Dr. Yusof is an active member of the International Astronomical Union, contributing to Divisions G (Stars and Stellar Physics) and H (Interstellar Matter and Local Universe). She leads the Theoretical Physics Group at the University of Malaya, mentoring students and collaborating with international researchers. Her work has been recognized with awards such as the the Top Ten Entries in the 2016 Taylor & Francis Commonwealth Scholar Best Journal Article Prize. Through her research and dedication, Dr. Yusof continues to advance the field of astrophysics and inspire future scientists. |
Publication
Finance
Project Title | Progress | Status |
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Neutrino Luminosity On The Hertzprung-russell Diagram And Its Impact To The Neutrino Terrestrial Detection |
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Near Eddington Limit Mass Loss For Every Massive Stars |
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Steller Modelling For Supersolar Stars |
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Dark energy stars in the context of black holes - The physical profiles
Grids of stellar models with rotation VII: models from 0.8 to 300 M-circle dot at supersolar metallicity (Z=0.020)
Very massive star winds as sources of the short-lived radioactive isotope Al-26
The neutrino emission from thermal processes in very massive stars in the local universe
Evolution of solar-like stars. HA Kassim, N Yusof, M Idris and ZA Motahar
Stellar Models with Rotation at High Metallicitiy
Energy Loss of Neutrinos in 20 Msun and 40 Msun Massive Stars
The Exponential S-Factor in the PP Chain
Solar Neutrino Fluxes Using The Exponential S-Factor