The knowledge of the production of extinct radioactivities like 92Nb and 146Sm by photodisintegration processes in ccSN and SNIa models is essential for interpreting abundances in meteoritic material and for Galactic Chemical Evolution (GCE). The 92Mo/92Nb and 146Sm/144Sm ratios provide constraints for GCE and production sites. We present results for SNIa with emphasis on nuclear uncertainties.
|Title of host publication||Proceedings of Science|
|Publisher||Proceedings of Science (PoS)|
|Publication status||Published - 31 Dec 2014|
|Event||13th Nuclei in the Cosmos, NIC 2014 - Debrecen, Hungary|
Duration: 7 Jul 2014 → 11 Jul 2014
|Conference||13th Nuclei in the Cosmos, NIC 2014|
|Period||7/07/14 → 11/07/14|