In preparation
Here are the lectures from the 5th Russbach Workshop on Nuclear Astrophysics.
If your lecture or talk is not available, please send us an E-Mail with the talk/lecture so that we can publish it here.
The list is in alphabetical order and does not correspond to the workshop program.
Author |
Title |
|---|---|
| L. Buchmann | The TRIUMF-ISAC facility |
| J.-C. Dalouzy | Spectroscopy of 19Ne -search for a new astrophysically important 1/2+ state |
| R. Diehl | Gamma-Ray Astronomy |
| M. El Eid | Reflection on the s-process in massive stars |
| M. El Eid | The 6 numbers - Shaping of the Universe |
| A. Frebel | What old stars tell us about the infant Universe |
| R. Gallino | 1. Galactic production of s-elements and 2. How to derive solar system r-process residuals |
| A. Herlert | High-precision mass measurements of short-lived nuclei |
| L. Husti | Ba-stars - theoretical interpretation |
| I. Ivans | Spectroscopic observations and abundance determinations of ancient stars |
| I. Ivans | Observation of r-rich stars |
| J. Jose | 10 Gyr of classical Nova explosions |
| J. Jose | X-ray bursts |
| F. Käppeler | s-Process nucleosynthesis - an introduction |
| F. Käppeler | The s-process in massive stars - new experimental data and further needs |
| K.-L. Kratz | Th,U chronometers and correlated production of Pb, Bi |
| K.-L. Kratz | r-Process I: With the waiting-point approach from B2FH to yesterday |
| K.-L. Kratz | r-Process II: Results from the HEW SNII model |
| K.-L. Kratz | HEW model predictions vs. Halo-star observations |
| M. Liebendoerfer | Neutrino transport for efficient 3D Supernova models |
| S. Marrone | |
| L. Mashonkina | |
| P. Mohr | |
| S. Palmerini | |
| B. Pfeiffer | Kann uns der Himmel auf den Kopf fallen? Außerirdische Einflüsse auf Klimaänderungen? |
| B. Pfeiffer | History of Astrophysics: From the Pythagoreans to Nucleosynthesis |
| O. Sorlin | The N=28 shell closure |
| O. Sorlin | Research program in astrophysics at GANIL |
| J. Stone | Nuclear mass models |
| N. Stone | Pathological physics is alive and well |
| N. Stone | Summary |