Element synthesis in stars

@article{Thielemann2001ElementSI,
  title={Element synthesis in stars},
  author={F. Thielemann and Franziska Brachwitz and Ch. Freiburghaus and E. Kolbe and Gabriel Mart{\'i}nez-Pinedo and Thomas Rauscher and F. Rembges and W. Raphael Hix and Matthias Liebendoerfer and Anthony Mezzacappa and Karl Ludwig Kratz and Bernd Pfeiffer and Karlheinz Langanke and Ken’ichi Nomoto and Stephan Rosswog and Hendrik Schatz and Michael Wiescher},
  journal={Progress in Particle and Nuclear Physics},
  year={2001},
  volume={46},
  pages={5-22}
}

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References

SHOWING 1-10 OF 111 REFERENCES
Nuclear structure studies at ISOLDE and their impact on the astrophysical r-process
The focus of the present review is the production of the heaviest elements in nature via the r-process. A correct understanding and modeling requires the knowledge of nuclear properties far from
Nucleosynthesis in Neutrino-Driven Winds. I. The Physical Conditions
During the first 20 s of its life, the enormous neutrino luminosity of a neutron star drives appreciable mass loss from its surface. Previous investigations have shown that this neutrino-driven wind
r‐Process Abundances and Chronometers in Metal‐poor Stars
Rapid neutron-capture (i.e., r-process) nucleosynthesis calculations, employing internally consistent and physically realistic nuclear physics input (quasi-particle random-phase approximation (QRPA)
The r-process and neutrino-heated supernova ejecta
As a neutron star is formed by the collapse of the iron core of a massive star, its Kelvin-Helmholtz evolution is characterized by the release of gravitational binding energy as neutrinos. The
Evolution of Proto-Neutron Stars
We study the thermal and chemical evolution during the Kelvin-Helmholtz phase of the birth of a neutron star, employing neutrino opacities that are consistently calculated with the underlying
An approximation for the rp-process
Hot (explosive) hydrogen burning, or the rapid proton capture process (rp-process), occurs in a number of astrophysical environments. Novae and X-ray bursts are the most prominent ones, but accretion
The astrophysical r-process: A comparison of calculations following adiabatic expansion with classical calculations based on neutron densities and temperatures
The rapid neutron-capture process (r-process) encounters unstable nuclei far from β-stability. Therefore its observable features, like the abundances, witness (still uncertain) nuclear structure as
The reaction rate sensitivity of nucleosynthesis in type II supernovae
We explore the sensitivity of the nucleosynthesis of intermediate mass elements (28 � A < ∼80) in supernovae derived from massive stars to the nuclear reaction rates employed in the model. Two
Production of heavy elements in inhomogeneous cosmologies
The incorporation of quantum chromodynamics into big bang cosmology predicts that the universe shifted from a quark-gluon plasma to a meson gas when it was roughly 10 μs old. If this change is due to
...
...