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Study of O-16(C-12, alpha Ne-20)alpha for the investigation of carbon-carbon fusion reaction via the Trojan Horse Method
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SYSNO ASEP 0468703 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Study of O-16(C-12, alpha Ne-20)alpha for the investigation of carbon-carbon fusion reaction via the Trojan Horse Method Author(s) Rapisarda, G. G. (IT)
Spitaleri, C. (IT)
Bordeanu, C. (RO)
Hons, Zdeněk (UJF-V) RID, ORCID
Kiss, G. G. (HU)
La Cognata, M. (IT)
Mrázek, Jaromír (UJF-V) RID, ORCID, SAI
Nita, C. (RO)
Pantelica, D. (RO)
Petrascu, H. (RO)
Pizzone, R. G. (IT)
Romano, S. (IT)
Szucs, T. (HU)
Trache, L. (US)
Tumino, A. (IT)
Velisa, G. (RO)Number of authors 16 Article number UNSP 012024 Source Title Journal of Physics Conference Series, 8th European Summer School on Experimental Nuclear Astrophysics (Santa Tecla School), 703. - Bristol : IOP Publishing Ltd., 2016 - ISSN 1742-6588 Number of pages 4 s. Publication form Print - P Action 8th European Summer School on Experimental Nuclear Astrophysics (Santa Tecla School) Event date 13.09.2015 - 20.09.2015 VEvent location Sicily Country IT - Italy Event type EUR Language eng - English Country GB - United Kingdom Keywords Fusion reactions ; Thermonuclear reactions Astrophysical energies ; carbon carbons ; Massive stars ; Trojan horse methods Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics Institutional support UJF-V - RVO:61389005 UT WOS 000389583400024 EID SCOPUS 84964829106 DOI https://doi.org/10.1088/1742-6596/703/1/012024 Annotation Carbon-carbon fusion reaction represents a nuclear process of great interest in astrophysics, since the carbon burning is connected with the third phase of massive stars (M > 8 M circle dot) evolution. In spite of several experimental works, carbon-carbon cross section has been measured at energy still above the Gamow window moreover data at low energy present big uncertainty. In this paper we report the results about the study of the reaction O-6(C-12, alpha Ne-20)alpha as a possible three -body process to investigate C-12(C-12,alpha)(20) Ne at astrophysical energy via Trojan Horse Method (THM). This study represent the first step of a program of experiments aimed to measure the C-12+C-12 cross section at astrophysical energy using the THM. Workplace Nuclear Physics Institute Contact Markéta Sommerová, sommerova@ujf.cas.cz, Tel.: 266 173 228 Year of Publishing 2017
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