activity
20102026
most citedThe R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit

583 citations · 1.5k across the 21 of their papers we have counts for

collaborators

22 papers

nucl-th2026

Systematic study of macroscopic interaction models and short-range effects in fusion

Azni Abdul Aziz, Norhasliza Yusof

The fusion reaction is central to stellar carbon burning, yet its cross section at astrophysical energies remains uncertain and theoretical extr…

hep-ph2025

Electromagnetic probes as signatures for a first-order QCD phase transition

Mohamad Lukman Aidid Mohd Yusoff, Norhasliza Yusof, Hasan Abu Kassim +5

We investigate dimuon production in the context of a first-order phase transition in QCD matter using a chiral fluid dynamics model. This approach incorporates non-equilibrium effe…

astro-ph.SR2024★ 1 cited

Grids of stellar models with rotation VIII: Models from 1.7 to 500 at metallicity

Yves Sibony, Kendall G. Shepherd, Norhasliza Yusof +12

Grids of stellar evolution models with rotation using the Geneva stellar evolution code (Genec) have been published for a wide range of metallicities. We introduce the last remaini…

astro-ph.SR2022★ 13 cited

Very massive star winds as sources of the short-lived radioactive isotope Al

S. Martinet, G. Meynet, D. Nandal +7

The Al short-lived radioactive nuclide is the source of the observed galactic diffuse -ray emission at 1.8 MeV. While different sources of Al have been explored, s…

astro-ph.GA2022★ 68 cited

Grids of stellar models with rotation VI: Models from 0.8 to 120 at a metallicity Z = 0.006

Patrick Eggenberger, Sylvia Ekström, Cyril Georgy +14

Context: Grids of stellar models, computed with the same physical ingredients, allow one to study the impact of a given physics on a broad range of initial conditions and are a key…

astro-ph.SR2022★ 50 cited

Grids of stellar models with rotation VII: Models from 0.8 to 300 M at super-solar metallicity (Z = 0.020)

Norhasliza Yusof, Raphael Hirschi, Patrick Eggenberger +11

We present a grid of stellar models at super-solar metallicity (Z = 0.020) extending the previous grids of Geneva models at solar and sub-solar metallicities. A metallicity of Z =…