Abstract
We present 12C+12C direct fusion measurements with STELLA UK-FATIMA, that reach into the region of astrophysics interest relevant to massive stars (M ≈ 25) using self-supporting thin rotating carbon foils [1]. We demonstrate that detecting gammas and light charged particles in coincidence with nanosecond timing is key for effective background reduction achieving reliable measurements in the sub-nanobarn range. We give details about core developments of the detection apparatus as well as the coincidence-analysis procedure of low count statistics. The present data largely follows the phenomenological hindrance interpolation and shows indication for resonant behaviour at the lowest energy explored.
Original language | English |
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Number of pages | 4 |
DOIs | |
Publication status | Published - 24 Feb 2022 |
Event | 16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 - Chengdu, China Duration: 21 Sept 2021 → 25 Sept 2021 |
Conference
Conference | 16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 |
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Country/Territory | China |
City | Chengdu |
Period | 21/09/21 → 25/09/21 |
Bibliographical note
Publisher Copyright:© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).