• [1]

    E. G. Adelberger et al., Rev. Mod. Phys. 70, 1265 (1998), arXiv:astro-ph/9805121

  • [2]

    S. Turck-Chieze et al., Astrophys. J. Lett. 555, L69 (2001)

  • [3]

    E. G. Adelberger et al., Rev. Mod. Phys. 83, 195 (2011), arXiv:1004.2318 [nucl-ex]

  • [4]

    N. Vinyoles, A. M. Serenelli, F. L. Villante et al., Astrophys. J. 835, 202 (2017), arXiv:1611.09867 [astro-ph.SR]

  • [5]

    P. C. de Holanda and A. Y. Smirnov, LMA MSW solution of the solar neutrino problem and first KamLAND results, JCAP 02 , 001 (2003), arXiv:hep-ph/0212270

  • [6]

    P. Anselmann et al. (GALLEX), Phys. Lett. B 285, 376 (1992)

  • [7]

    J. N. Abdurashitov et al. (SAGE), Phys. Lett. B 328, 234 (1994)

  • [8]

    G. Bellini et al. (BOREXINO), Nature 512, 383 (2014)

  • [9]

    M. Agostini et al. (BOREXINO), Nature 562, 505 (2018)

  • [10]

    Y. Meng et al. (PandaX-4T), Phys. Rev. Lett. 127, 261802 (2021), arXiv:2107.13438 [hep-ex]

  • [11]

    D. S. Akerib et al. (LZ), Phys. Rev. D 101, 052002 (2020), arXiv:1802.06039 [astro-ph.IM]

  • [12]

    E. Aprile et al. (XENON),Projected WIMP sensitivity of the XENONnT dark matter experiment, JCAP 11 , 031 (2020), arXiv:2007.08796[physics.ins-det]

  • [13]

    W. Ma et al. (PandaX), Phys. Rev. Lett. 130, 021802 (2023), arXiv:2207.04883 [hep-ex]

  • [14]

    E. Aprile et al. (XENON), Phys. Rev. Lett. 126, 091301 (2021), arXiv:2012.02846 [hep-ex]

  • [15]

    X. Zhou et al. (PandaX-II), Chin. Phys. Lett. 38, 011301 (2021), arXiv:2008.06485 [hep-ex]

  • [16]

    E. Aprile et al. (XENON), Phys. Rev. D 102, 072004 (2020), arXiv:2006.09721 [hep-ex]

  • [17]

    J. Billard, L. Strigari, and E. Figueroa-Feliciano, Phys. Rev. D 89, 023524 (2014), arXiv:1307.5458 [hep-ph]

  • [18]

    J. W. Chen, H. C. Chi, C. P. Liu et al., Phys. Lett. B 774, 656 (2017), arXiv:1610.04177 [hep-ex]

  • [19]

    H. Ma et al. (CDEX), J. Phys. Conf. Ser. 1342, 012067 (2020), arXiv:1712.06046 [hep-ex]

  • [20]

    J. Li, X. Ji, W. Haxton et al., Phys. Procedia 61, 576 (2015), arXiv:1404.2651 [physics.ins-det]

  • [21]

    X. Yan et al. (PandaX), Phys. Rev. Lett. 132, 152502 (2024), arXiv:2312.15632 [nucl-ex]

  • [22]

    L. Si et al. (PandaX), Research 2022, 9798721 (2022), arXiv:2205.12809 [nucl-ex]

  • [23]

    D. Zhang et al., Phys. Rev. C 105, 014604 (2022), arXiv:2102.02490 [nucl-ex]

  • [24]

    M. Szydagis, N. Barry, K. Kazkaz et al., NEST: A Comprehensive Model for Scintillation Yield in Liquid Xenon, JINST 6 , P10002 (2011), arXiv:1106.1613[physics.ins-det]

  • [25]

    E. Aprile et al. (XENON), Eur. Phys. J. C 80, 785 (2020), arXiv:2003.03825 [physics.ins-det]

  • [26]

    S. J. Haselschwardt, J. Kostensalo, X. Mougeot et al., Phys. Rev. C 102, 065501 (2020), arXiv:2007.13686 [hep-ex]

  • [27]

    E. Aprile et al. (XENON), Phys. Rev. C 106, 024328 (2022), arXiv:2205.04158 [hep-ex]

  • [28]

    E. Aprile et al. (XENON), Nature 568, 532 (2019), arXiv:1904.11002 [nucl-ex]

  • [29]

    W. Verkerke and D. P. Kirkby, The RooFit toolkit for data modeling, eConf C0303241 , MOLT007 (2003), arXiv:physics/0306116

  • [30]

    X. Chen et al., BambooMC — A Geant4-based simulation program for the PandaX experiments, JINST 16 (09), T09004 (2021), arXiv:2107.05935 [physics.ins-det]

  • [31]

    S. Agostinelli et al. (GEANT4), Nucl. Instrum. Meth. A 506, 250 (2003)

  • [32]

    J. B. Albert et al. (EXO-200), Phys. Rev. C 89, 015502 (2014), arXiv:1306.6106 [nuclex]

  • [33]

    X. Cui et al., Design and commissioning of the PandaX-4T cryogenic distillation system for krypton and radon removal, JINST 16 (07), P07046 (2021), arXiv:2012.02436 [physics.ins-det]

  • [34]

    J. N. Abdurashitov et al. (SAGE), Phys. Rev. C 80, 015807 (2009), arXiv:0901.2200 [nucl-ex]