Items where Author is "Hirschi, R."
Number of items: 19.
Article
Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations. (2024)
F. Rizzuti,
R. Hirschi,
V. Varma,
W. D. Arnett,
C. Georgy,
C. Meakin,
M. Mocák,
A. J. St. Murphy
and
T. Rauscher
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3D simulations of a neon burning convective shell in a massive star. (2024)
C. Georgy,
F. Rizzuti,
R. Hirschi,
V. Varma,
W. D. Arnett,
C. Meakin,
M. Mocak,
A. St J. Murphy
and
T. Rauscher
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The Nuclear Reaction Network WinNet. (2023)
M. Reichert,
C. Winteler,
O. Korobkin,
A. Arcones,
J. Bliss,
M. Eichler,
U. Frischknecht,
C. Fröhlich,
R. Hirschi,
M. Jacobi,
J. Kuske,
G. Martínez-Pinedo,
D. Martin,
D. Mocelj,
T. Rauscher
and
F.-K. Thielemann
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Uncertainties in νp-process nucleosynthesis from Monte Carlo variation of reaction rates. (2019)
N. Nishimura,
T. Rauscher,
R. Hirschi,
G. Cescutti,
A. St J. Murphy
and
C. Fröhlich
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Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations. (2018)
G. Cescutti,
R. Hirschi,
N. Nishimura,
J. W. den Hartogh,
T. Rauscher,
A. St J. Murphy
and
S. Cristallo
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Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations. (2018)
N. Nishimura,
T. Rauscher,
R. Hirschi,
A. St J. Murphy,
G. Cescutti
and
C. Travaglio
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Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations. (2016)
T. Rauscher,
N. Nishimura,
R. Hirschi,
G. Cescutti,
A. St J. Murphy
and
A. Heger
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Constraints on rotational mixing from surface evolution of light elements in massive stars. (2010)
U. Frischknecht,
R. Hirschi,
G. Meynet,
S. Ekstroem,
C. Georgy,
T. Rauscher,
C. Winteler
and
Friedrich-Karl Thielemann
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Nuclear physics : A key ingredient in astrophysical modeling. (2005)
Friedrich-Karl Thielemann,
D. Argast,
F. Brachwitz,
J. L. Fisker,
Carla Froehlich,
R. Hirschi,
E. Kolbe,
D. Mocelj
and
T. Rauscher
Other
Abundance uncertainties obtained with the PIZBUIN framework for Monte Carlo reaction rate variations. (2018)
T. Rauscher,
N. Nishimura,
G. Cescutti,
R. Hirschi
and
A. St J. Murphy
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Sensitivity to neutron captures and β-decays of the enhanced s-process in rotating massive stars at low metallicities. (2018)
N. Nishimura,
R. Hirschi
and
T. Rauscher
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The s-process nucleosynthesis : Impact of the uncertainties in the nuclear physics determined by monte carlo variations. (2017)
G. Cescutti,
N. Nishimura,
R. Hirschi,
T. Rauscher,
J. W. den Hartogh
and
A. St J. Murphy
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Impacts of nuclear-physics uncertainty in stellar temperatures on the s-process nucleosynthesis. (2017)
N. Nishimura,
G. Cescutti,
R. Hirschi,
T. Rauscher,
J. Den Hartogh
and
A. St J. Murphy
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Production Uncertainties of p-Nuclei in the γ-Process in Massive Stars Using a Monte Carlo Approach. (2017)
T. Rauscher,
N. Nishimura,
R. Hirschi,
G. Cescutti,
A. St J. Murphy
and
A. Heger
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Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars. (2016)
T. Rauscher,
N. Nishimura
and
R. Hirschi
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Silicon carbide grains of type C provide evidence for the production of the unstable isotope Si in supernovae. (2013)
M. Pignatari,
E. Zinner,
M.G. Bertolli,
R. Trappitsch,
P. Hoppe,
T. Rauscher,
C. Fryer,
F. Herwig,
R. Hirschi,
F.X. Timmes
and
F.-K. Thielemann
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Impact of rotation on the weak s-process. (2011)
U. Frischknecht,
R. Hirschi,
T. Rauscher
and
Friedrich-Karl Thielemann
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Boron depletion in 9 to 15 M(circle dot) stars with rotation. (2010)
U. Frischknecht,
R. Hirschi,
G. Meynet,
S. Ekstroem,
C. Georgy,
T. Rauscher,
C. Winteler
and
F-K. Thielemann
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Production of intermediate-mass and heavy nuclei. (2007)
Friedrich-Karl Thielemann,
Carla Froehlich,
R. Hirschi,
M. Liebendoerfer,
I. Dillmann,
D. Mocelj,
T. Rauscher,
G. Martinez-Pinedo,
K. Langanke,
K. Farouqi,
K.L. Kratz,
B. Pfeiffer,
I. Panov,
D. K. Nadyozhin,
S. Blinnikov,
E. Bravo,
W. R. Hix,
P. Hoflich
and
N. T. Zinner