Direct Measurement of Carbon Fusion at Astrophysical Energies with Gamma-Particle Coincidences

M. Heine*, G. Fruet, S. Courtin, D. G. Jenkins, P. Adsley, A. Brown, R. Canavan, W. N. Catford, E. Charon, D. Curien, S. Della Negra, J. Duprat, F. Hammache, J. Lesrel, G. Lotay, A. Meyer, E. Monpribat, D. Montanari, L. Morris, M. MoukaddamJ. Nippert, Zs Podolyák, P. H. Regan, I. Ribaud, M. Richer, M. Rudigier, R. Shearman, N. de Séréville, C. Stodel

*Corresponding author for this work

Research output: Contribution to conferencePaperpeer-review

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 languageEnglish
Number of pages4
DOIs
Publication statusPublished - 24 Feb 2022
Event16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 - Chengdu, China
Duration: 21 Sept 202125 Sept 2021

Conference

Conference16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021
Country/TerritoryChina
CityChengdu
Period21/09/2125/09/21

Bibliographical note

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© 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/).

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