Ядерна фізика та енергетика Nuclear Physics and Atomic Energy   ISSN: 1818-331X (Print), 2074-0565 (Online)   Publisher: Institute for Nuclear Research of the National Academy of Sciences of Ukraine   Languages: Ukrainian, English   Periodicity: 4 times per year   Open access peer reviewed journal

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X. Tang¹, B. Bucher¹, X. Fang¹, M. Notani¹, W. P. Tan¹, Y. Li^1,3, P. Mooney¹, H. Esbensen², C. L. Jiang², K. E. Rehm², C. J. Lin³, E. Brown<sup>4

1</sup>Department of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame, IN, USA
²Physics Division, Argonne National Laboratory, Argonne, IL, USA
³China Institute of Atomic Energy, Beijing, China
⁴Department of Physics and Astronomy, National Superconducting Cyclotron Laboratory, and the Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan, USA

Abstract: The ¹²C + ¹²C fusion reaction is one of the most important reactions in the stellar evolution. Due to its complicated reaction mechanism, there is great uncertainty in the reaction rate which limits our understanding of various stellar objects, such as explosions on the surface of neutron stars, white dwarf (type Ia) supernovae, and massive stellar evolution. In this paper, I will review the challenges in the study of carbon burning. I will also report recent results from our studies: 1) an upper limit for the ¹²C + ¹²C fusion cross sections, 2) measurement of the ¹²C + ¹²C at deep sub-barrier energies, 3) a new measurement of the ¹²C (¹²C , n) reaction. The outlook for the studies of the astrophysical heavy-ion fusion reactions will also be presented.

Keywords: ¹²C + ¹²C, fusion reaction, stellar evolution.

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