Measuring the 15O(α, γ)19Ne reaction in Type I X-ray bursts using the GADGET II TPC: Hardware

Tyler Wheeler, A. Adams, J. Allmond, H. Alvarez Pol, E. Argo, Y. Ayyad, D. Bardayan, D. Bazin, T. Budner, A. Chen, K. Chipps, B. Davids, J. Dopfer, M. Friedman, H. Fynbo, R. Grzywacz, J. Jose, J. Liang, R. Mahajan, S. PainD. Pérez-Loureiro, E. Pollacco, A. Psaltis, S. Ravishankar, A. Rogers, L. Schaedig, L. J. Sun, J. Surbrook, L. Weghorn, C. Wrede

Research output: Contribution to conferencePaperpeer-review

1 Scopus citations

Abstract

Sensitivity studies have shown that the 15O(α, γ)19Ne reaction is the most important reaction rate uncertainty affecting the shape of light curves from Type I X-ray bursts. This reaction is dominated by the 4.03 MeV resonance in 19Ne. Previous measurements by our group have shown that this state is populated in the decay sequence of 20Mg. A single 20Mg(βpα)15O event through the key 15O(α, γ)19Ne resonance yields a characteristic signature: the emission of a proton and alpha particle. To achieve the granularity necessary for the identification of this signature, we have upgraded the Proton Detector of the Gaseous Detector with Germanium Tagging (GADGET) into a time projection chamber to form the GADGET II detection system. GADGET II has been fully constructed, and is entering the testing phase.

Original languageAmerican English
DOIs
StatePublished - 24 Feb 2022
Event16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 - Chengdu, China
Duration: 21 Sep 202125 Sep 2021

Conference

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

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/).

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