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Constraining the 12C+12C fusion cross section for astrophysics

Bucher, B.; Fang, X.; Tang, X.D.; Tan, W.P.; Almaraz-Calderon, S.; Alongi, A.; Ayangeakaa, A.D.; Beard, M.; Best, A.; Browne, J.; Cahillane, C.; Couder, M.; Dahlstrom, E.; Davies, P.; DeBoer, R.; Kontos, A.; Lamm, L.; Long, A.; Lu, W.; Lyons, S.; Ma, C.; Moncion, A.; Notani, M.; Patel, D.; Paul, N.; Pignatari, M.; Roberts, A.; Robertson, D.; Smith, K.; Stech, E.; Talwar, R.; Thomas, S.; Wiescher, M.

Authors

B. Bucher

X. Fang

X.D. Tang

W.P. Tan

S. Almaraz-Calderon

A. Alongi

A.D. Ayangeakaa

M. Beard

A. Best

J. Browne

C. Cahillane

M. Couder

E. Dahlstrom

P. Davies

R. DeBoer

A. Kontos

L. Lamm

A. Long

W. Lu

S. Lyons

C. Ma

A. Moncion

M. Notani

D. Patel

N. Paul

M. Pignatari

A. Roberts

D. Robertson

K. Smith

E. Stech

R. Talwar

S. Thomas

M. Wiescher



Contributors

R. Schwengner
Editor

K. Zuber
Editor

Abstract

The 12 C+ 12 C reaction is one of the single most important nuclear reactions in astrophysics. It strongly influences late evolution of massive stars as well as the dynamics of type Ia supernovae and x-ray superbursts. An accurate estimation of the cross section at relevant astrophysical energies is extremely important for modeling these systems. However, the situation is complicated by the unpredictable resonance structure observed at higher energies. Two recent studies at Notre Dame have produced results which help reduce the uncertainty associated with this reaction. The first uses correlations with the isotope fusion systems, 12 C+ 13 C and 13 C+ 13 C, to establish an upper limit on the resonance strengths in 12 C+ 12 C. The other focuses on the specific channel 12 C+ 12 C→ 23 Mg+n and its low-energy measurement and extrapolation which is relevant to s-process nucleosynthesis. The results from each provide important constraints for astrophysical models.

Citation

Bucher, B., Fang, X., Tang, X., Tan, W., Almaraz-Calderon, S., Alongi, A., …Wiescher, M. (2015). Constraining the 12C+12C fusion cross section for astrophysics. EPJ Web of Conferences, 93, 03009. https://doi.org/10.1051/epjconf/20159303009

Journal Article Type Conference Paper
Acceptance Date Jun 5, 2015
Online Publication Date May 28, 2015
Publication Date 2015
Deposit Date Jun 28, 2018
Publicly Available Date Jul 13, 2018
Journal EPJ Web of Conferences
Print ISSN 2100-014X
Electronic ISSN 2100-014X
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 93
Article Number 03009
Pages 03009
ISBN 9782759817948
DOI https://doi.org/10.1051/epjconf/20159303009
Public URL https://hull-repository.worktribe.com/output/558419
Publisher URL https://www.epj-conferences.org/articles/epjconf/abs/2015/12/epjconf_cgs2015_03009/epjconf_cgs2015_03009.html

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Copyright Statement
© Owned by the authors, published by EDP Sciences, 2015





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