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Raphael Hirschi

Professor of Physics

Keele University

United Kingdom

Research Interests

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Articles (20)

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2026

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Collaborators (10)

Roel Lefever

Heidelberg University

GERMANY

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Andreas A C Sander

Professor

Kiel University

GERMANY

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Georges Meynet

University of Geneva

SWITZERLAND

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Philip Adsley

Assistant Professor

Texas A&M University

UNITED STATES

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Sylvia Ekstöm

Associate Professor

University of Geneva

SWITZERLAND

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Ken Shen

University of California

UNITED STATES

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Rosario Gianluca Pizzone

Docenti di ruolo di IIa fascia

University of Catania

ITALY

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Norhasliza Yusof

Senior Lecturer

University of Malaya

MALAYSIA

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V Varma

Keele University

UNITED KINGDOM

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James Keegans

Teaching Fellow

University of Hull

UNITED KINGDOM

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Raphael Hirschi

Research Interests

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Articles (20)

Drawing the line between explosion and collapse in electron-capture supernovae

The beauty of k2: Probing stellar interiors using apsidal motion

Fast-spinning massive black holes from slowly rotating low-metallicity stars: Implications for GW231123

The impact of initial mass dependent convective boundary mixing on the structure and fates of massive stars

Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network

Trans-Fe elements from type Ia supernovae

Discovery of a transitional type of evolved massive star with a hard ionizing flux

3D synthetic convective velocity fields to initialize core-collapse supernova simulations from 1D progenitors

The fate of rotating massive stars across cosmic times

The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity

Experimental Determination of α Widths of Ne21 Levels in the Region of Astrophysical Interest: New O17+α Reaction Rates and Impact on the Weak s Process

Stellar Evolution and Convection in 3D Hydrodynamic Simulations of a Complete Burning Phase

Grids of stellar models with rotation: VIII. Models from 1.7 to 500 M$_\ensuremath⊙$ at metallicity Z = 10$^‑5$

New Wolf-Rayet wind yields and nucleosynthesis of Helium stars

Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations

3D simulations of a neon burning convective shell in a massive star

Rapidly rotating Population III stellar models as a source of primary nitrogen

Constraining physical processes in pre-supernovae massive star evolution

Entrainment in 3D hydrodynamics simulations of neon burning

Very Massive Stars: Near and Far

Collaborators (10)

Roel Lefever

Andreas A C Sander

Georges Meynet

Philip Adsley

Sylvia Ekstöm

Ken Shen

Rosario Gianluca Pizzone

Norhasliza Yusof

V Varma

James Keegans

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