10–11 Sept 2009
Max-Planck Institut fuer Extraterrestrische Physik (MPE)
Europe/Berlin timezone

Opportunities of in-beam experiments for the astrophysical p process

10 Sept 2009, 16:45
30m
Seminar room 1.18 (Max-Planck Institut fuer Extraterrestrische Physik (MPE))

Seminar room 1.18

Max-Planck Institut fuer Extraterrestrische Physik (MPE)

TU Munich Campus Garching D-85748 Garching

Speaker

Jens Hasper (Institut fuer Kernphysik, Universitaet zu Koeln, 50937 Koeln, Germany)

Description

The p-process is the most promising astrophysical scenario for the nucleosynthesis of about 35 proton-rich nuclei referred to as p nuclei. This process involves an extensive reaction network of about 2000 nuclei and more than 20000 reactions, especially photodisintegration reactions, under explosive physical conditions. The huge number of reaction rates are mainly adopted from Hauser-Feshbach calculations. Hence, experimental data are essential to put stringent constraints on the nuclear models required for these calculations. It is the major aim of ex- perimental p-process studies to improve descriptions for optical model potentials, nuclear level densities and photon strength functions. Experiments on (p,gamma) and (alpha,gamma) reactions are a dedicated approach to study these nuclear properties at astrophysically relevant energies and, thus, a large number of these experiments have been performed in the last years. Despite these efforts, the data base is still not sufficient to derive reliable global nuclear models for reaction-rate calculations, and additional data have to be provided. In this contribution, we will give an overview of different experimental methods that have been applied so far to study proton- and alpha-induced capture reactions. The advantages and limitations of both the activation and in-beam technique will be discussed. In this context, we will present the gamma-detector array HORUS at the ion TANDEM accelerator of the University of Cologne, which allows to perform highly-sensitive in-beam experiments on reactions of astro- physical interest. An outlook will be given on the unique experimental opportunities for future p-process studies that are provided by this sophisticated facility. This project is supported by the DFG under contract ZI 510/5-1.

Author

Jens Hasper (Institut fuer Kernphysik, Universitaet zu Koeln, 50937 Koeln, Germany)

Co-authors

A. Zilges (Institut fuer Kernphysik, Universitaet zu Koeln, 50937 Koeln, Germany) J. Endres (Institut fuer Kernphysik, Universitaet zu Koeln, 50937 Koeln, Germany) M. Buessing (Institut fuer Kernphysik, Universitaet zu Koeln, 50937 Koeln, Germany) M. Elvers (Institut fuer Kernphysik, Universitaet zu Koeln, 50937 Koeln, Germany)

Presentation materials