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RH

Raphael Hirschi

0000-0001-8764-6522
astro-ph.SRastro-ph.HEastro-phastro-ph.GAnucl-exnucl-thphysics.flu-dynastro-ph.COastro-ph.IMgr-qc

On Valency

published · living versions
W_waqfzrqh·v1 · currentpublished
Catching Element Formation In The Act
with Chris L. Fryer, Frank Timmes, Aimee L. Hungerford, Aaron Couture +214
1 version
W_5z6v2j4d·v1published
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit

Preprints & journals

164 papers in the corpus · 2003–2026
Structure of Convective-Reactive Zone in a Supernova Progenitor2610.01239v1 · M. Mocak, C. Meakin, F. Rizzuti et al.2026 · 0 citationsarXiv
Stellar Yields of Rapidly Rotating Population III Stars for the High Redshift Universe2609.21939v1 · Devesh Nandal, Konstantinos Topalakis, Vasilisa Sergienko et al.2026 · 0 citationsarXiv
3D simulations of a complete convective silicon shell burning phase2608.04954v1 · V. Varma, R. Hirschi, F. Rizzuti et al.2026 · 0 citationsarXiv
Fast-spinning massive black holes from slowly rotating low-metallicity stars: Implications for GW2311232606.04428v2 · N. H. Ismail, N. Yusof, R. Hirschi et al.2026 · 0 citationsarXiv
The Beauty of k2: Probing Stellar Interiors Using Apsidal Motion. I. The Benchmark Massive Binary HD 1522482605.21236v2 · Sophie Rosu, Luca Sciarini, Sylvia Ekstrom et al.2026 · 0 citationsarXiv
Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics2604.12672v2 · G. Leidi, A. Holas, K. Vitovsky et al.2026 · 0 citationsarXiv
Drawing the line between explosion and collapse in electron-capture supernovae -- I. Impact of conductive flame speeds and ignition conditions on the explosion mechanism2601.16918v1 · Alexander Holas, Samuel W. Jones, Friedrich K. Roepke et al.2026 · 3 citationsarXiv
The Impact of Initial Mass Dependent Convective Boundary Mixing on the Structure and Fates of Massive Stars2512.11728v1 · Emily E. Whitehead, Raphael Hirschi, Vishnu Varma et al.2025 · 6 citationsarXiv
Apsidal Motion in O-Star Binaries: GENEC rotating binary models put to the k2-test2510.26306v1 · Sophie Rosu, Luca Sciarini, Sylvia Ekstrom et al.2025 · 0 citationsarXiv
3D Synthetic Convective Velocity Fields to Initialise Core-Collapse Supernova Simulations from 1D Progenitors2510.21611v1 · Vishnu Varma, Bernhard Mueller, Raphael Hirschi2025 · 1 citationMon Not R Astron Soc (2025) 3846-3855
The fate of rotating massive stars across cosmic times2508.21233v2 · R. Hirschi, K. Goodman, G. Meynet et al.2025 · 7 citationsarXiv
Discovery of a new transitional type of evolved massive stars with hard ionizing flux2508.18410v1 · Andreas A.C. Sander, Roel R. Lefever, Joris Josiek et al.2025 · 0 citationsarXiv
Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs2508.15079v1 · Umberto Battino, James Keegans, Megan Allen et al.2025 · 0 citationsA&A 703, A44 (2025)
The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity2504.18621v1 · Erin R. Higgins, Jorick S. Vink, Raphael Hirschi et al.2025 · 5 citationsA&A 699, A71 (2025)
Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network2408.03368v2 · Adam Griffiths, Miguel-'A Aloy, Raphael Hirschi et al.2024 · 4 citationsA&A 693, A93 (2025)
Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations2407.15544v1 · Federico Rizzuti, Raphael Hirschi, Vishnu Varma et al.2024 · 23 citationsarXiv
New Wolf-Rayet wind yields and nucleosynthesis of Helium stars2407.07983v1 · Erin R. Higgins, Jorick S. Vink, Raphael Hirschi et al.2024 · 1 citationarXiv
Grids of stellar models with rotation VIII: Models from 1.7 to 500 M⊙M_\odot at metallicity Z=10−5Z = 10^{-5}2407.06739v2 · Yves Sibony, Kendall G. Shepherd, Norhasliza Yusof et al.2024 · 1 citationarXiv
3D simulations of convective shell Neon-burning in a massive star2405.21033v1 · C. Georgy, F. Rizzuti, R. Hirschi et al.2024 · 0 citationsarXiv
Experimental Determination of α Widths of ^21Ne Levels in the Region of Astrophysical Interest: New ^17O+α Reaction Rates and Impact on the Weak s Process.38759192 · Hammache, F, Adsley, P, Lamia, L et al.2024 · 4 citationsPhysical review letters. 2024;132(18):182701
Rapidly rotating Population III stellar models as a source of primary nitrogen2404.16512v2 · Sophie Tsiatsiou, Yves Sibony, Devesh Nandal et al.2024 · 24 citationsA&A 687, A307 (2024)
Very Massive Star Models: I. Impact of Rotation and Metallicity and Comparisons with Observations2309.00062v2 · S. Martinet, G. Meynet, S. Ekstrom et al.2023 · 26 citationsA&A 679, A137 (2023)
Stellar Wind Yields of Very Massive Stars2308.10941v1 · Erin R. Higgins, Jorick S. Vink, Raphael Hirschi et al.2023 · 31 citationsarXiv
3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star2305.13912v1 · F. Rizzuti, R. Hirschi, W. D. Arnett et al.2023 · 22 citationsarXiv
The nuclear reaction network WinNet2305.07048v2 · M. Reichert, C. Winteler, O. Korobkin et al.2023 · 41 citationsarXiv
Spin-down and reduced mass loss in early-type stars with large-scale magnetic fields2211.07060v1 · Z. Keszthelyi, A. de Koter, Y. Gotberg et al.2022 · 2 citationsarXiv
The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities2209.06350v2 · Z. Keszthelyi, A. de Koter, Y. Gotberg et al.2022 · 28 citationsarXiv
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars2207.03223v2 · F. Rizzuti, R. Hirschi, C. Georgy et al.2022 · 22 citationsarXiv
The impact of 17^{17}O+α+\alpha reaction rate uncertainties on the s-process in rotating massive stars2206.04167v1 · J. Frost-Schenk, P. Adsley, A.M. Laird et al.2022 · 13 citationsarXiv
Very massive star winds as sources of the short-lived radioactive isotope 26^{26}Al2205.15184v1 · S. Martinet, G. Meynet, D. Nandal et al.2022 · 13 citationsA&A 664, A181 (2022)
The p-process in exploding rotating massive stars2203.16380v1 · A. Choplin, S. Goriely, R. Hirschi et al.2022 · 30 citationsA&A 661, A86 (2022)
Grids of stellar models with rotation VI: Models from 0.8 to 120 M⊙M_\odot at a metallicity Z = 0.0062201.12262v2 · Patrick Eggenberger, Sylvia Ekstrom, Cyril Georgy et al.2022 · 66 citations2021, A&A 652, A137
Grids of stellar models with rotation VII: Models from 0.8 to 300 M⊙_\odot at super-solar metallicity (Z = 0.020)2201.08645v1 · Norhasliza Yusof, Raphael Hirschi, Patrick Eggenberger et al.2022 · 50 citationsarXiv
Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes2111.01165v2 · R. Andrassy, J. Higl, H. Mao et al.2021 · 21 citationsA&A 659, A193 (2022)
UVES analysis of red giants in the bulge globular cluster NGC 65222107.08746v1 · B. Barbuy, E. Cantelli, L. Muniz et al.2021 · 16 citationsarXiv
Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star2107.02199v1 · L. Horst, R. Hirschi, P. V. F. Edelmann et al.2021 · 19 citationsA&A 653, A55 (2021)
Evolution of Wolf-Rayet stars as black hole progenitors2105.12139v1 · Erin R. Higgins, Andreas A.C. Sander, Jorick S. Vink et al.2021 · 43 citationsarXiv
Convective core entrainment in 1D main sequence stellar models2103.06196v2 · L. J. A. Scott, R. Hirschi, C. Georgy et al.2021 · 59 citationsarXiv
Convective core sizes in rotating massive stars: I. Constraints from solar metallicity OB field stars2103.03672v1 · S. Martinet, G. Meynet, S. Ekstrom et al.2021 · 47 citationsA&A 648, A126 (2021)
Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo2101.05345v1 · F. Rizzuti, G. Cescutti, F. Matteucci et al.2021 · 31 citationsarXiv
Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity2012.07420v1 · Laura J. Murphy, Jose H. Groh, Sylvia Ekstrom et al.2020 · 56 citationsarXiv
Is GW190521 the merger of black holes from the first stellar generations?2009.06585v2 · Eoin J. Farrell, Jose H. Groh, Raphael Hirschi et al.2020 · 97 citationsarXiv
Relative Importance of Convective Uncertainties in Massive Stars2006.01877v2 · Etienne A. Kaiser, Raphael Hirschi, W. David Arnett et al.2020 · 69 citationsarXiv
Re-evaluation of the 22^{22}Ne(α,γ\alpha,\gamma)26^{26}Mg and 22^{22}Ne(α,n\alpha,n)25^{25}Mg reaction rates2005.14482v2 · Philip Adsley, Umberto Battino, Andreas Best et al.2020 · 58 citationsarXiv
Nucleosynthesis in early rotating massive stars and chemical composition of CEMP stars2001.02341v1 · Arthur Choplin, Raphael Hirschi2020 · 9 citationsarXiv
The Formation of a 70 Msun Black Hole at High Metallicity1911.12357v4 · K. Belczynski, R. Hirschi, E.A. Kaiser et al.2019 · 61 citationsarXiv
A direct measurement of the 17O(a,g)21Ne reaction in inverse kinematics and its impact on heavy element production1910.00870v1 · M.P. Taggart, C. Akers, A.M. Laird et al.2019 · 7 citationsPhysics Letters B 798 (2019) 134894
The contribution from rotating massive stars to the enrichment in Sr and Ba of the Milky Way1909.04378v1 · Federico Rizzuti, Gabriele Cescutti, Francesca Matteucci et al.2019 · 24 citationsarXiv
Impact of Uncertainties in Astrophysical Reaction Rates on Nucleosynthesis in the νp\nu p Process1909.03235v2 · T. Rauscher, N. Nishimura, G. Cescutti et al.2019 · 3 citationsJPS Conf. Proc. 31 (2020) 011026
The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints1908.09160v1 · J.W. den Hartogh, R. Hirschi, M. Lugaro et al.2019 · 22 citationsA&A 629, A123 (2019)
Career total: at least 350 works. 164 are in this corpus.Showing the 50 most recent.

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