His main research concerns Astrophysics, Nuclear physics, Nucleosynthesis, Neutron and Hartree–Fock method. His Astrophysics research includes elements of Astronomy and Nuclear reaction. His work on r-process is typically connected to Reaction rate as part of general Nucleosynthesis study, connecting several disciplines of science.
His Hartree–Fock method study integrates concerns from other disciplines, such as Electronic correlation, Nuclear force, Computational physics and Pairing. The study incorporates disciplines such as Mass formula, Particle physics and Atomic physics in addition to Pairing. He has included themes like Ejecta, Equation of state and Nucleon in his Neutron star study.
His primary areas of study are Nuclear physics, Astrophysics, Nucleosynthesis, Neutron and Neutron star. His research integrates issues of Radiative transfer and Atomic physics in his study of Nuclear physics. His study brings together the fields of Astronomy and Astrophysics.
His Nucleosynthesis research is multidisciplinary, incorporating elements of Ejecta and Nuclide. His Neutron research includes themes of Hartree–Fock method, Nuclear structure and Resonance. His Neutron star research focuses on Equation of state and how it relates to Dense matter.
The scientist’s investigation covers issues in Nucleosynthesis, Nuclear physics, Astrophysics, Neutron and Stars. When carried out as part of a general Nucleosynthesis research project, his work on r-process is frequently linked to work in Reaction rate, therefore connecting diverse disciplines of study. His Nuclear physics study combines topics in areas such as Dipole and Radiative transfer.
His Astrophysics research is multidisciplinary, relying on both Spectral line, Neutrino and Magic number. His Neutron research is multidisciplinary, incorporating perspectives in Nuclear structure, Proton and Isotope. In his study, which falls under the umbrella issue of Neutron star, Star and Theoretical physics is strongly linked to Symmetry.
Stéphane Goriely spends much of his time researching Neutron, Nucleosynthesis, Nuclear physics, Astrophysics and Dipole. The various areas that he examines in his Neutron study include Absorption, Atomic physics, Nuclear astrophysics and Isotope. His study on Nucleosynthesis is mostly dedicated to connecting different topics, such as Neutron star.
His Nuclear physics study combines topics from a wide range of disciplines, such as Magnetic dipole and Kinetic energy. Astrophysics connects with themes related to Nuclear reaction in his study. His Dipole research also works with subjects such as
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
RIPL – Reference Input Parameter Library for Calculation of Nuclear Reactions and Nuclear Data Evaluations
R. Capote;M. Herman;M. Herman;P. Obložinský;P. Obložinský;P.G. Young.
Nuclear Data Sheets (2009)
The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
Marcel Arnould;Stéphane Goriely;Kohji Takahashi.
Physics Reports (2007)
The p-process of stellar nucleosynthesis: astrophysics and nuclear physics status
Marcel Arnould;Stéphane Goriely.
Physics Reports (2003)
R-Process Nucleosynthesis in Dynamically Ejected Matter of Neutron Star Mergers
Stephane Goriely;Andreas Bauswein;H.-Thomas Janka.
arXiv: Solar and Stellar Astrophysics (2011)
A Hartree-Fock Nuclear Mass Table
S. Goriely;F. Tondeur;J.M. Pearson.
Atomic Data and Nuclear Data Tables (2001)
First Gogny-Hartree-Fock-Bogoliubov nuclear mass model.
Stéphane Goriely;Stéphane Hilaire;Michel Girod;S. Péru.
Physical Review Letters (2009)
SYSTEMATICS OF DYNAMICAL MASS EJECTION, NUCLEOSYNTHESIS, AND RADIOACTIVELY POWERED ELECTROMAGNETIC SIGNALS FROM NEUTRON-STAR MERGERS
Andreas Bauswein;Stéphane Goriely;Hans-Thomas Janka.
The Astrophysical Journal (2013)
Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII. Stiffness and stability of neutron-star matter
S. Goriely;N. Chamel;J. M. Pearson.
Physical Review C (2010)
Improved microscopic nuclear level densities within the Hartree-Fock-Bogoliubov plus combinatorial method
Stéphane Goriely;Stéphane Hilaire;Arjan J. Koning.
Physical Review C (2008)
Skyrme-Hartree-Fock-Bogoliubov nuclear mass formulas: crossing the 0.6 MeV accuracy threshold with microscopically deduced pairing.
S. Goriely;N. Chamel;J. M. Pearson.
Physical Review Letters (2009)
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