Indirect determination of the astrophysical S factor for the Li6 ( p,γ)Be7 reaction using the asymptotic normalization coefficient method

Kiss, G. G.; La Cognata, M.; Yarmukhamedov, R.; Tursunmakhatov, K. I.; Wiedenhöver, I.; Baby, L. T.; Cherubini, S.; Cvetinović, A.; D'Agata, G.; Figuera, P.; Guardo, G. L.; Gulino, M.; Hayakawa, S.; Indelicato, I.; Lamia, L.; Lattuada, M.; Mudò, F.; Palmerini, S.; Pizzone, R. G.; Rapisarda, G. G.; Romano, S.; Sergi, M. L.; Spartà, R.; Spitaleri, C.; Trippella, O.; Tumino, A.; Anastasiou, M.; Kuvin, S. A.; Rijal, N.; Schmidt, B.; Igamov, S. B.; Sakuta, S. B.; Fülöp, Zs; Gyürky, Gy; Szücs, T.; Halász, Z.; Somorjai, E.; Hons, Z.; Mrázek, J.; Tribble, R. E.; Mukhamedzhanov, A. M.

doi:10.1103/physrevc.104.015807

Title: Indirect determination of the astrophysical S factor for the Li 6 ( p , γ ) Be 7 reaction using the asymptotic normalization coefficient method

Journal Article · Thu Jul 29 00:00:00 EDT 2021 · Physical Review. C

DOI:https://doi.org/10.1103/physrevc.104.015807· OSTI ID:1850053

Kiss, G. G. ^[1];

^[2]; Yarmukhamedov, R. ^[3]; Tursunmakhatov, K. I. ^[4]; Wiedenhöver, I. ^[5]; Baby, L. T. ^[5]; Cherubini, S. ^[6]; Cvetinović, A. ^[2]; D'Agata, G. ^[7]; Figuera, P. ^[2]; Guardo, G. L. ^[6]; Gulino, M. ^[8]; Hayakawa, S. ^[9]; Indelicato, I. ^[6]; Lamia, L. ^[10]; Lattuada, M. ^[6]; Mudò, F. ^[6]; Palmerini, S. ^[11]; Pizzone, R. G. ^[2]; Rapisarda, G. G. ^[6] more »

Inst. for Nuclear Research (ATOMKI), Debrecen (Hungary)
Lab. Nazionali del Sud - INFN, Catania (Italy)
Uzbekistan Academy of Sciences, Tashkent (Uzbekistan)
Uzbekistan Academy of Sciences, Tashkent (Uzbekistan); Gulistan State Univ. (Uzbekistan)
Florida State Univ., Tallahassee, FL (United States)
Lab. Nazionali del Sud - INFN, Catania (Italy); Univ. di Catania (Italy)
Nuclear Physics Inst. of the Czech Academy of Sciences, Rez (Czech Republic)
Lab. Nazionali del Sud - INFN, Catania (Italy); Univ. di Enna "Kore" (Italy)
Univ. of Tokyo, Saitama (Japan)
Lab. Nazionali del Sud - INFN, Catania (Italy); Univ. di Catania (Italy); Centro Siciliano di Fisica Nucleare e Struttura della Materia (CSFNSM), Catania (Italy)
Univ. di Perugia (Italy); Istituto Nazionale di Fisica Nucleare, Perugia (Italy)
National Research Center “Kurchatov Institute”, Moscow (Russia)
Texas A & M Univ., College Station, TX (United States)

The ⁶Li(p,γ) ⁷Be cross section influences a variety of astrophysical scenarios, including big-bang and stellar nucleosynthesis. In recent years, conflicting results of direct measurements have been published, reporting contradictory low-energy trends. To shed light on the contradiction between the existing data sets, the reaction was studied using the asymptotic normalization coefficient (ANC) technique which was up-to-now never used for this reaction. To derive the ANC, the ⁶Li(³He,d) ⁷Be transfer reaction, studied at the Department of Physics and Astronomy of the University of Catania and at the John. D. Fox Superconducting Accelerator Laboratory at Florida State University, was re-analyzed, focusing on the proton transfer mechanism [the α transfer process is discussed by Kiss et al. [Phys. Lett. B 807, 135606 (2020)]. Here, the energy of the ³He beam impinging on a ⁶Li target was E_lab = 3 MeV and E_lab = 5 MeV. The yield of the emitted deuterons was measured with high precision by using silicon ΔE – E telescopes.

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Research Organization:: Texas A & M Univ., College Station, TX (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: FG02-93ER40773; NA0003841

OSTI ID:: 1850053

Journal Information:: Physical Review. C, Vol. 104, Issue 1; ISSN 2469-9985

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Title: Indirect determination of the astrophysical S factor for the Li 6 ( p , γ ) Be 7 reaction using the asymptotic normalization coefficient method

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