ab initio methods is presented. The used approaches are No-Core Shell Model and Cluster Channels Orthogonal Functions Method. The scheme also contains elements of R-matrix theory and procedures for extrapolating various data obtained in ab initio computations. The developed approach as a whole allows one not only to calculate the astrophysical S-factor and all nuclear characteristics that determine its value, but also to evaluate the reliability of the obtained results and to identify the dominant reaction mechanisms against a background of insignificant ones. The high accuracy of the obtained results and has been demonstrated."> Study of radiative proton capture by the <sup>7</sup>Be nucleus with the use of <i>ab initio</i> approaches -
  • [1]

    E. Tel, M. Sahan, I. H. Sarpunet al., EPJ Web of Conferences128, 01005 (2016)

  • [2]

    S. Fukuda,et al., Phys. Rev. Lett.86, 5651 (2001), arXiv: hep-ex/0103032

  • [3]

    Q. Ahmad,et al., Phys. Rev. Lett.87, 071301 (2001), arXiv: nucl-ex/0106015

  • [4]

    Ralph W., Nuclear Physics15, 411 (1960)

  • [5]

    P. D. Parker, Phys.Rev.150, 851 (1966)

  • [6]

    R. W. Kavanagh, T. A. Tombrello, J. M. Mosheret al., Bull. Am. Phys. Soc.14, 1209 (1969)

  • [7]

    F. J. Vaughn, R. A. Chalmers, D. Kohler, L. F. Chase, Phys. Rev. C2, 1657 (1970)

  • [8]

    B. W. Filippone, A. J. Elwyn, C. N. Davidset al., Phys. Rev. C28, 2222 (1983)

  • [9]

    L.T. Baby,et al., Phys. Rev. Lett.90, 022501 (2003)

  • [10]

    A. R. Junghans, K. A. Snover, E. C. Mohrmannet al., Phys. Rev. C81, 012801 (2010)

  • [11]

    R. H. Cyburt, B. Davids, and B. K. Jennings, Phys. Rev. C70, 045801 (2004)

  • [12]

    L. Trache, F. Carstoiu, C. A. Gagliardiet al., Nucl. Phys. A718, 493 (2003)

  • [13]

    A. M. Shirokov, I. J. Shin, Y. Kimet al., Phys. Lett. B761, 87 (2016)

  • [14]

    R. Machleidt, D. R. Entem, Phys. Rep.503, 1 (2011)

  • [15]

    D. R. Entem, R. Machleidt, Phys. Rev. C66, 014002 (2002)

  • [16]

    A. M. Shirokov, J. P. Vary, A. I. Mazuret al., Phys. Lett. B644, 33 (2007)

  • [17]

    C. Stump, J. Braun, R. Roth, Phys. Rev. C93, 021301 (2016)

  • [18]

    G. Papadimitriou, J. Rotureau, N. Michelet al., Phys. Rev. C88, 044318 (2013)

  • [19]

    S. C. Pieper, R. B. Wiringa, Ann. Rev. Nucl. Part. Sci.51, 53 (2001)

  • [20]

    H. Kummela, K. H. Luhrmann, J. Zabolitzky, Phys. Rep.36, 1 (1978)

  • [21]

    S. Quaglioni, P. Navratil, Phys. Rev. C79, 044606 (2009)

  • [22]

    S. Baroni, P. Navratil, S. Quaglioni, Phys. Rev. C87, 034326 (2013)

  • [23]

    T. Neff, H. Feldmeier, Int. J. Mod. Phys. E17, 2005 (2008)

  • [24]

    A. Adahchour, P. Descouvemont, Nucl. Phys. A813, 252 (2008)

  • [25]

    K. Arai, P. Descouvemont, D. Baye, W. Catford, Phys. Rev. C68, 014310 (2003)

  • [26]

    Y. Kanada-Enyo, H. Horiuchi, Prog. Theor. Phys. Suppl.142, 205 (2001)

  • [27]

    A.S. Solovyev, S.Y. Igashov, Phys. Rev. C96, 064605 (2017)

  • [28]

    K. Fossez, N. Michel, M. Ploszajczaket al., Phys. Rev. C91, 034609 (2015)

  • [29]

    L. Anh, M. Loc., Phys. Rev. C106, 1 014605 (2022)

  • [30]

    L. Asgari, and H. Sadeghi, Pramana-J. Phys.98, 50 (2024)

  • [31]

    R. Higa, P. Premarathna, and G. Rupak, arXiv: 2010.13003v2

  • [32]

    P. Navratil, K. Kravvaris, P. Gysberset al., J. Phys.: Conf. Ser.2586, 012062 (2023)

  • [33]

    D. M. Rodkin, and Yu. M. Tchuvil'sky, Phys. Rev. C103, 024304 (2021)

  • [34]

    D. M. Rodkin, and Yu. M. Tchuvil'sky, JETP Letters119(10), 739 (2024)

  • [35]

    D. M. Rodkin, and Yu. M. Tchuvil'sky, Int. J. Mod. Phys. E33(11), 2441008 (2024)

  • [36]

    D. M. Rodkin, and Yu. M. Tchuvil'sky, Int. J. Mod. Phys. E33(12), 2441019 (2024)

  • [37]

    Yu. F. Smirnov, Nucl. Phys.39, 346 (1962)

  • [38]

    O. F. Nemets, V. G. Neudachin, A. E. Rudchiket al.Nuclear Clusters in Atomic Nuclei and Multinucleon Transfer Reactions(Kiev: Naukova Dumka, Kiev, 1988)

  • [39]

    D. M. Rodkin, Yu. M. Tchuvilsky, Chin. Phys. C44, 12410 (2020)

  • [40]

    H. J. Mang, Z. Phys.148, 582 (1957)

  • [41]

    M. H. Macfarlane, J. B. French, Rev. Mod. Phys.32, 567 (1960)

  • [42]

    T. Fliessbach, H. J. Mang, Nucl. Phys. A32, 75 (1976)

  • [43]

    R. G. Lovas, R. J. Liotta, A. Insoliaet al., Phys. Rep.294, 265 (1998)

  • [44]

    S. G. Kadmensky, S. D. Kurgalin, Yu. M. Tchuvil'sky,, Phys. Part. Nucl.38, 699 (2007)

  • [45]

    A. Volya, and Yu. M. Tchuvil'sky, Phys. Rev. C91, 044319 (2015)

  • [46]

    A. Volya, and Yu. M. Tchuvil'sky, Phys. At. Nucl.79, 772 (2016)

  • [47]

    D. M. Rodkin, and Yu. M. Tchuvil'sky, Phys. Rev. C104, 044323 (2021)

  • [48]

    D. Odell, C. Brune, D. Phillipset al., Front. Phys.10, 888476 (2022)

  • [49]

    Calvin W. Johnsonet al., arXiv: 1801.08432

  • [50]

    I. J. Shin, Y. Kim, P. Maris, J. P. Varyet al., J. Phys. G: Nucl. Part. Phys.44, 075103 (2017)

  • [51]

    M. C. Atkinson, K. Kravvaris, S. Quaglioniet al., Phys. Lett B860, 139189 (2025)

  • [52]

    B. A. Brown, Lecture Notes inNuclear Structure Physics(East Lansing: Michigan State University, 2011)

  • [53]

    D. M. Rodkin, Yu. M. Tchuvilsky, J. of Phys.: Conf. Ser.2586, 012046 (2023)

  • [54]

    D. R. Tilley, J. H. Kelley, J. L. Godwinet al., Nucl. Phys.155, A745 (2004)

  • [55]

    N. K. Timofeyuk, Phys. Rev. C81, 064306 (2010)

  • [56]

    V. Z. Goldberg, G. V. Rogachev, M. S. Golovkoet al., JETP Lett.67(12), 1013 (1998)

  • [57]

    D. M. Rodkin, Yu. M. Tchuvilsky, Phys. Rev. C106, 034305 (2022)

  • [58]

    P. Maris and J. P. Vary, Int. J. Mod. Phys. E22, 1330016 (2013)

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