Supernovae theory: Study of electro-weak processes during gravitational collapse of massive stars
Explore this paper's citation graph
- Type
- preprint
- Published
- 2010-10-18
- Cited by
- 4
- References
- 238
- Access
- Open access
- OpenAlex
- https://openalex.org/W5543364
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:169599483
Keywords
Humanities, Physics, Philosophy
References
- The Physics of Stars
- Effets du milieu sur la propagation des neutrinos dans la matière nucléaire
- Principles of stellar evolution and nucleosynthesis
- The Nuclear Many-Body Problem
- A and V
- An Introduction to the Study of Stellar Structure
- Handbook of Mathematical Functions with Formulas
- Presupernova evolution and explosion of massive stars
- Quantum Theory of Many-Particle Systems
- The Great Supernova of 1987 a
- On Godunov-type methods for gas dynamics
- Difference methods for initial-value problems
- Foundations of Radiation Hydrodynamics
- The Supernovae
- Collective Motion
- Simulation of Astrophysical Fluid Flow
- Superfluidity in Nuclear Matter
- Methods of Numerical Integration
- Open issues in core collapse supernova theory
- AIP Conference Proceedings
Cited by
- Effects of the temperature dependence of the in-medium nucleon mass on core-collapse supernovae
- Distribution of nuclei in equilibrium stellar matter from the free-energy density in a Wigner-Seitz cell
- Impact of electron capture rates for nuclei far from stability on core-collapse supernovae
- Mass measurements towards doubly magic 78Ni: Hydrodynamics versus nuclear mass contribution in core-collapse supernovae