Journals Articles Conferences News About CLP
Submit a paper Email Alert
Search
Search
Articles
Journals
News
Advanced Search
Top Searches
2D MaterialsTransformation opticsQuantum PhotonicsSmall lasersSemiconductor UV PhotonicsSupersymmetric microring laser arrays

NUCLEAR TECHNIQUES, Volume. 46, Issue 8, 080002(2023)

Nuclear astrophysics research based on HI-13 tandem accelerator

Jiayinghao LI, Yunju LI*, Zhihong LI, Youbao WANG, Yangping SHEN, Bing GUO, and Weiping LIU
Author Affiliations
  • China Institution of Atomic Energy, Beijing 102413, China
    • show less
    AbstractGet PDF(in Chinese)
    Figures&Tables (18)
    Equations (0)
    References (54)
    Tools
    Paper Information
    Topics
    References(54)

    [1] Bai X X, Liu W P, Qin J C et al. A facility for production and utilization of radioactive beams[J]. Nuclear Physics A, 588, c273-c276(1995).

    [2] Liu W P, Bai X X, Zhou S H et al. Angular distribution for the 7Be(d, n)8B reaction at Ec.m.=5.8 MeV and the S17(0) factor for the 7Be(p, γ)8B reaction[J]. Physical Review Letters, 77, 611-614(1996).

    [3] Li Z H, Guo B, Yan S Q et al. The 13N(d, n)14O reaction and the astrophysical 13N(p, γ)14O reaction rate[J]. Physical Review C, 74, 5801-5807(2006).

    [4] Li Z H, Liu W P, Bai X X et al. The 8Li(d, p)9Li reaction and the astrophysical 8Li(n, γ)9Li reaction rate[J]. Physical Review C, 71, 2801-2805(2005).

    [5] Decrock P, Delbar T, Duhamel P et al. Determination of the 13N(p, γ)14O reaction cross section using a 13N radioactive ion beam[J]. Physical Review Letters, 67, 808-811(1991).

    [6] Delbar T, Galster W, Leleux P et al. Investigation of the 13N(p, γ)14O reaction using 13N radioactive ion beams[J]. Physical Review C, 48, 3088-3096(1993).

    [7] Chupp T E, Kouzes R T, McDonald A B et al. Total width of the 5.17 MeV 1- state in 14O and the hot-CNO cycle[J]. Physical Review C, Nuclear Physics, 31, 1023-1025(1985).

    [8] Fernandez P B, Adelberger E G, Garcia A. γwidth of the unbound 5.17 MeV level of 14O and the hot CNO cycle[J]. Physical Review C, 40, 1887-1900(1989).

    [9] Smith M S, Magnus P V, Hahn K I et al. Gamma width of 14O* (5.17 MeV) and the stellar 13N(p, γ)14O reaction rate[J]. Physical Review C, 47, 2740-2750(1993).

    [10] Magnus P V, Adelberger E G, García A. The hot CNO cycle 13N(p, γ) resonance energy and the 18Ne mass[J]. Physical Review C, 49, R1755-R1758(1994).

    [11] Motobayashi T, Takei T, Kox S et al. Determination of the astrophysical 13N(p, γ)14O cross section through the Coulomb dissociation method[J]. Physics Letters B, 264, 259-263(1991).

    [12] Kiener J, Lefebvre A, Aguer P et al. Determination of the 13N(p, γ)14O reaction rate through the Coulomb break-up of a 14O radioactive beam[J]. Nuclear Physics A, 552, 66-81(1993).

    [13] Decrock P, Gaelens M, Huyse M et al. Study of the 13N(d,n)14O reaction cross section and its astrophysical implications for the 13N proton capture reaction[J]. Physical Review C, Nuclear Physics, 48, 2057-2067(1993).

    [14] Tang X D, Azhari A, Fu C B et al. Determination of the direct capture contribution for 13N(p, γ)14O from the 14O→13N+p asymptotic normalization coefficient[J]. Physical Review C, 69, 055807(2004).

    [15] Liu W P, Li Z H, Bai X X et al. Determination of 11C(p,γ)12N astrophysical S-factor via measurement of 11C(d, n)12N reaction[J]. Nuclear Physics A, 728, 275-284(2003).

    [16] Zeng S, Liu W P, Li Z H et al. Measurement of 2H(8Li,9Be)n reaction relevant to primordial nucleosynthesis[J]. Chinese Physics Letters, 22, 2219-2221(2005).

    [17] Guo B, Li Z H, Liu W P et al. The 8Li(d,p)9Li reaction and astrophysical 8B(p,γ)9C reaction rate[J]. Nuclear Physics A, 761, 162-172(2005).

    [18] GUO Bing, LIU Weiping, LI Zhihong et al. Measurement of angular distribution for 11C(d,n)12N reaction and determination of asymptotic normalization coefficient for the virtual decay 12N→11C+p[J]. Atomic Energy Science and Technology, 39, 118-123(2005).

    [19] Guo B, Li Z H. Determination of astrophysical 13N(p,γ)14O S-factors from the asymptotic normalization coefficient of 14 →13C+n[J]. Chinese Physics Letters, 24, 65-68(2007).

    [20] GUO Bing, LI Zhihong, LIU Weiping et al. Study of halo for the ground state and proton widths for the first two excited states of 27P[J]. High Energy Physics and Nuclear Physics, 30, 183-185(2006).

    [21] Li Z H, Liu W P, Bai X X et al. First observation of neutron-proton halo structure for the 3.563 MeV 0+ state in 6Li via 1H(6He,6Li)n reaction[J]. Physics Letters B, 527, 50-54(2002).

    [22] Li Z H, Liu W P, Bai X X et al. Search for the halo effect in the 1H(6He,6Li)n reaction[J]. Chinese Physics Letters, 19, 306-308(2002).

    [23] Wang Y B, Wang B X, Qin X et al. 13N+p elastic resonance scattering via a thick-target method[J]. Physical Review C, 77, 044304(2008).

    [24] Wang Y B, Qin X, Wang B X et al. Simulation and analysis of 13N+p elastic resonance scattering[J]. Chinese Physics C, 33, 181-186(2009).

    [25] Jin S J, Wang Y B, Wang B X et al. Excited states in 18Ne studied via 17F+p[J]. Chinese Physics Letters, 27, 032102(2010).

    [26] Li Z C, Cheng Y H, Yan C et al. Beijing Q3D magnetic spectrometer and its applications[J]. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 336, 150-161(1993).

    [27] Li Z H, Li E T, Guo B et al. First measurement of the 2H(6He,7Li)n angular distribution and proton spectroscopic factor in 7Li[J]. The European Physical Journal A, 44, 1-5(2010).

    [28] Li Z H, Su J, Guo B et al. Determination of the 12C(p, γ)13N reaction rates from the 12C(7Li, 6He)13N reaction[J]. Science China Physics, Mechanics and Astronomy, 53, 658-663(2010).

    [29] Li Y J, Li Z H, Li E T et al. New determination of the astrophysical 13C(p, γ)14N S(E) factors and reaction rates via the 13C(7Li,6He)14N reaction[J]. The European Physical Journal A, 48, 13(2012).

    [30] Li Z H, Li Y J, Su J et al. New determination of the proton spectroscopic factor in 9Be from the 13C(9Be,8Li)14N angular distribution[J]. Physical Review C, 87, 017601(2013).

    [31] Su J, Li Z H, Guo B et al. Astrophysical reaction rates of the 8Li(p,γ)9Beg.s. direct capture reaction[J]. Chinese Physics Letters, 23, 55-57(2006).

    [32] Li Y J, Li Z H, Li E T et al. Indirect measurement of the 57.7 keV resonance strength for the astrophysical γ-ray source of the 25Mg(p,γ)26Al reaction[J]. Physical Review C, 102, 025804(2020).

    [33] Guo B, Li Z H, Li Y J et al. Spectroscopic factors for low-lying 16N levels and the astrophysical 15N(n,γ)16N reaction rate[J], 89, 2801-2805(2014).

    [34] Wu Z D, Guo B, Li Z H et al. Proton widths of the low-lying 16F states from the 15N(7Li,6Li)16N reaction[J]. Physical Review C, 89, 4315-4310(2014).

    [35] Gan L, Sun H B, Li Z H et al. Experimental study of the spectroscopic factors of 90–97Zr[J]. Physical Review C, 97, 064614(2018).

    [36] Gan L, Sun H B, Li Z H et al. Experimental study of the spectroscopic factors of 116–125Sn[J]. Physical Review C, 101, 014612(2020).

    [37] Su J, Li Z H, Guo B et al. Neutron spectroscopic factors of 7Li and astrophysical 6Li(n,γ)7Li reaction rates[J]. Chinese Physics Letters, 27, 052101(2010).

    [38] Li E T, Li Z H, Li Y J et al. Proton spectroscopic factor of the 12C ground state from the 12C(11B,12C)11B elastic transfer reaction[J]. Physical Review C, 90, 067601(2014).

    [39] Kubono S, Abe K, Kato S et al. Determination of the subthreshold state contribution in 13C(α,n)16O, the main neutron-source reaction for the s process[J]. Physical Review Letters, 90, 062501(2003).

    [40] Johnson E D, Rogachev G V, Mukhamedzhanov A M et al. Astrophysical reaction rate for the neutron-generator reaction 13C(α,n)16O in asymptotic giant branch stars[J]. Physical Review Letters, 97, 192701(2006).

    [41] Pellegriti M G, Hammache F, Roussel P et al. Indirect study of the 13C(α,n)16O reaction via the 13C(7Li,t)17O transfer reaction[J]. Physical Review C, 77, 2801-2805(2008).

    [42] Guo B, Li Z H, Lugaro M et al. New determination of the 13C(α,n)16O reaction rate and its influence on the s-process nucleosynthesis in AGB stars[J]. The Astrophysical Journal Letters, 756, 193(2012).

    [43] Costantini H, Formicola A, Imbriani G et al. LUNA: a laboratory for underground nuclear astrophysics[J]. Reports on Progress in Physics, 72, 086301(2009).

    [44] Kurath D. Alpha-structure amplitudes for the 1p shell[J]. Physical Review C, 7, 1390-1395(1973).

    [45] Rudchik A A, Rudchik A T, Kozeratska G M et al. 7Li+11B elastic and inelastic scattering in a coupled-reaction-channels approach[J]. Physical Review C, 72, 034608(2005).

    [46] Shen Y P, Guo B, Ma T L et al. First experimental constraint of the spectroscopic amplitudes for the α-cluster in the 11B ground state[J]. Physics Letters B, 797, 134820(2019).

    [47] Weaver T A, Woosley S E. Nucleosynthesis in massive stars and the 12C(α, γ)16O reaction rate[J]. Physics Reports, 227, 65-96(1993).

    [48] Magnus P V, Adelberger E G, García A. The hot CNO cycle 13N(p,γ) resonance energy and the 18Ne mass[J]. Physical Review C, 49, R1755-R1758(1994).

    [49] Motobayashi T, Takei T, Kox S et al. Determination of the astrophysical 13N(p,γ)14O cross section through the Coulomb dissociation method[J]. Physics Letters B, 264, 259-263(1991).

    [50] Kiener J, Lefebvre A, Aguer P et al. Determination of the astrophysical 13N(p,γ)14O reaction rate through the Coulomb break-up of a 14O radioactive beam[J]. Nuclear Physics A, 552, 66-81(1993).

    [51] Decrock P, Gaelens M, Huyse M et al. Study of the 13N(d,n)14O reaction cross section and its astrophysical implications for the 13N proton capture reaction[J]. Physical Review C, Nuclear Physics, 48, 2057-2067(1993).

    [52] Shen Y P, Guo B, de Boer R J et al. Constraining the external capture to the 16O ground state and the E2 S factor of the 12C(α,γ)16O reaction[J]. Physical Review Letters, 124, 162701(2020).

    [53] de Boer R J, Görres J, Wiescher M et al. The 12C(α,γ)16O reaction and its implications for stellar helium burning[J]. Reviews of Modern Physics, 89, 035007(2017).

    [54] Shen Y P, Guo B, de Boer R J et al. New determination of the 12C(α, γ)16O reaction rate and its impact on the black-hole mass gap[J]. The Astrophysical Journal Letters, 945, 41(2023).

    Tools

    Get Citation

    Copy Citation Text

    Jiayinghao LI, Yunju LI, Zhihong LI, Youbao WANG, Yangping SHEN, Bing GUO, Weiping LIU. Nuclear astrophysics research based on HI-13 tandem accelerator[J]. NUCLEAR TECHNIQUES, 2023, 46(8): 080002

    Download Citation

    EndNote(RIS)BibTexPlain Text
    Set citation alerts for article
    Save article for my favorites
    Paper Information

    Category: Research Articles

    Received: Jun. 21, 2023

    Accepted: --

    Published Online: Sep. 19, 2023

    The Author Email:

    DOI:10.11889/j.0253-3219.2023.hjs.46.080002

    Topics

    laser devices and laser physics
    Lasers and Laser Optics
    Laser physics
    laser manufacturing
    Instrumentation, Measurement and Metrology