• [1]

    J. Cheng et al., Annual Review of Nuclear and Particle Science 67, 231-251 (2017)

  • [2]

    K. Kang et al., Status and prospects of a deep underground laboratory in china, in: Journal of Physics: Conference Series, Vol. 203, IOP Publishing, 2010, p. 012028

  • [3]

    Q. Yue et al., Phys. Rev. D 90, 091701 (2014)

  • [4]

    M. Xiao et al., First dark matter search results from the PandaX-I experiment, Science China Physics, Mechanics and Astronomy 57, 2024–2030 (2014)

  • [5]

    L. Wang et al., First results on 76Ge neutrinoless double beta decay from CDEX-1 experiment, Science China Physics, Mechanics and Astronomy 60(7), 071011(2017)

  • [6]

    X. Chen et al., Sci. China Phys. Mech. Astron. 60(6), 061011 (2017)

  • [7]

    J. F. Beacom et al., Chinese Physics C 41(2), 023002 (2017)

  • [8]

    L. Wan et al., Phys. Rev. D 95, 053001 (2017)

  • [9]

    O. Šrámek et al., Phys. Rev. D 6, 33034 (2016)

  • [10]

    Y. Wu et al., Chinese Physics C 37(8), 086001 (2013)

  • [11]

    L. Mayor, Physics World 28(5), 28-28 (2015)

  • [12]

    D. Mei and A. Hime, Phys. Rev. D 73, 053004 (2006)

  • [13]

    M. Agostini et al., Sensitivity to neutrinos from the solar CNO cycle in Borexino (2020), arXiv: 2005.12829

  • [14]

    K. Abe et al., Phys. Rev. D 94, 052010 (2016)

  • [15]

    Y. Zhang et al., Phys. Rev. D 93, 012004 (2016)

  • [16]

    Z. Wang et al., Nucl. Instrum. Methods A 855, 81-87 (2017)

  • [17]

    M. Li et al., Nucl. Instrum. Methods A 830, 303-308 (2016)

  • [18]

    Z. Guo et al., Astropart. Phys. 109, 33-40 (2019)

  • [19]

    S. Agostinelli et al., Nucl. Instrum. Methods A 506(3), 250-303 (2003)

  • [20]

    J. Allison et al., IEEE Transactions on Nuclear Science 53, 270-278 (2006)

  • [21]

    T. G. Farr et al., The shuttle radar topography mission, Reviews of Geophysics 45 (2007)

  • [22]

    D. R. Lide, CRC handbook of chemistry and physics, Vol. 97, CRC press, 2016

  • [23]

    M. Guan et al., A parametrization of the cosmic-ray muon flux at sea-level (2015), arXiv: 1509.06176

  • [24]

    S. Cecchini and M. Sioli, Cosmic ray muon physics, in: Non-accelerator particle astrophysics, Proceedings, 5th ICTP School, 1998, pp. 201–217

  • [25]

    G. Bellini et al., Journal of Cosmology and Astroparticle Physics 05, 015 (2012)

  • [26]

    E.-I. Esch et al., Nucl. Instrum. Methods A 538(1-3), 516-525 (2005)

  • [27]

    S. Kamat, Extending the sensitivity to the detection of WIMP dark matter with an improved understanding of the limiting neutron backgrounds, Ph.D. thesis, Case Western Reserve University (2005)

  • [28]

    M. Robinson et al., Nucl. Instrum. Methods A 511(3), 347-353 (2003)

  • [29]

    B. Aharmim et al., Phys. Rev. D 80, 012001 (2009)

  • [30]

    K. Eguchi et al., Phys. Rev. Lett. 90, 021802 (2003)

  • [31]

    C. Berger et al., Phys. Rev. D 40, 2163-2171 (1989)