- Open Access
Hidden heavy flavor tetraquarks in the Born-Oppenheimer approximation
Phys. Rev. D 111, 114016 – Published 17 June, 2025
DOI: https://doi.org/10.1103/xnbg-wklj
Abstract
The Born-Oppenheimer approximation is one of the very successful tools for solving the hydrogen atom problem. The experimental discovery of hidden heavy flavor tetraquarks (, and , , ) provides great possibilities for the hydrogen-bond-like structure of the quantum chromodynamics version. In this work, considering that the colors of and are both 8, the tetraquark system is formed by color coupling . In order to study the mass splitting caused by the color-spin hyperfine interaction, the color-spin basis vectors of the -wave tetraquark states are appropriately constructed. Then, we use the Born-Oppenheimer approximation to calculate the mass spectra of the -wave hidden heavy flavor tetraquark states. The results show that some of the hidden heavy flavor exotic hadrons discovered experimentally can be well explained as this type of hydrogen-bond-like tetraquark structure. In addition, some candidates for tetraquark bound states are predicted and may be compact tetraquark states.
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References (65)
- S. Godfrey and N. Isgur, Phys. Rev. D 32, 189 (1985).
- E. Klempt and A. Zaitsev, Phys. Rep. 454, 1 (2007).
- R. F. Lebed, R. E. Mitchell, and E. S. Swanson, Prog. Part. Nucl. Phys. 93, 143 (2017).
- R. L. Jaffe, Phys. Rev. D 15, 267 (1977).
- R. L. Jaffe, Phys. Rev. D 15, 281 (1977).
- C. Lodha and A. K. Rai, Few Body Syst. 65, 99 (2024).
- A. Esposito, M. Papinutto, A. Pilloni, A. D. Polosa, and N. Tantalo, Phys. Rev. D 88, 054029 (2013).
- E. Braaten, C. Langmack, and D. H. Smith, Phys. Rev. D 90, 014044 (2014).
- L. Maiani, A. D. Polosa, and V. Riquer, Phys. Rev. D 100, 014002 (2019).
- L. Maiani, A. D. Polosa, and V. Riquer, Phys. Rev. D 100, 074002 (2019).
- H. Mutuk, Phys. Rev. D 110, 034025 (2024).
- M. Berwein, N. Brambilla, A. Mohapatra, and A. Vairo, Phys. Rev. D 110, 094040 (2024).
- D. Germani, B. Grinstein, and A. D. Polosa, J. High Energy Phys. 04 (2025) 004.
- S. K. Choi et al. (Belle Collaboration), Phys. Rev. Lett. 91, 262001 (2003).
- L. Maiani, F. Piccinini, A. D. Polosa, and V. Riquer, Phys. Rev. D 71, 014028 (2005).
- R. D. Matheus, S. Narison, M. Nielsen, and J. M. Richard, Phys. Rev. D 75, 014005 (2007).
- H.-X. Chen, W. Chen, X. Liu, and S.-L. Zhu, Phys. Rep. 639, 1 (2016).
- Z.-G. Wang, Phys. Rev. D 109, 014017 (2024).
- C.-Y. Wong, Phys. Rev. C 69, 055202 (2004).
- M. T. AlFiky, F. Gabbiani, and A. A. Petrov, Phys. Lett. B 640, 238 (2006).
- Y.-R. Liu, X. Liu, W.-Z. Deng, and S.-L. Zhu, Eur. Phys. J. C 56, 63 (2008).
- F.-K. Guo, C. Hidalgo-Duque, J. Nieves, and M. P. Valderrama, Phys. Rev. D 88, 054007 (2013).
- T. Barnes and S. Godfrey, Phys. Rev. D 69, 054008 (2004).
- G. Bali et al., Proc. Sci. LATTICE2011 (2011) 135 [arXiv:1108.6147].
- D. Mohler, S. Prelovsek, and R. M. Woloshyn, Phys. Rev. D 87, 034501 (2013).
- T. M. Aliev and M. Savc𝚤, Eur. Phys. J. C 75, 169 (2015).
- D. V. Bugg, Phys. Lett. B 598, 8 (2004).
- C. Hanhart, Y. S. Kalashnikova, A. E. Kudryavtsev, and A. V. Nefediev, Phys. Rev. D 76, 034007 (2007).
- F.-K. Guo, C. Hanhart, Q. Wang, and Q. Zhao, Phys. Rev. D 91, 051504 (2015).
- T. Aaltonen et al. (CDF Collaboration), Phys. Rev. Lett. 102, 242002 (2009).
- M. Padmanath, C. B. Lang, and S. Prelovsek, Phys. Rev. D 92, 034501 (2015).
- S.-Q. Luo, K. Chen, X. Liu, Y.-R. Liu, and S.-L. Zhu, Eur. Phys. J. C 77, 709 (2017).
- K. Abe et al. (Belle Collaboration), Phys. Rev. Lett. 94, 182002 (2005).
- D. Ebert, R. N. Faustov, and V. O. Galkin, Phys. Lett. B 634, 214 (2006).
- R. F. Lebed and A. D. Polosa, Phys. Rev. D 93, 094024 (2016).
- A. Bondar et al. (Belle Collaboration), Phys. Rev. Lett. 108, 122001 (2012).
- T. Guo, L. Cao, M.-Z. Zhou, and H. Chen, arXiv:1106.2284.
- L. Leskovec, S. Meinel, M. Pflaumer, and M. Wagner, Phys. Rev. D 100, 014503 (2019).
- M. Karliner, J. L. Rosner, and T. Skwarnicki, Annu. Rev. Nucl. Part. Sci. 68, 17 (2018).
- F.-K. Guo, C. Hanhart, U.-G. Meißner, Q. Wang, Q. Zhao, and B.-S. Zou, Rev. Mod. Phys. 90, 015004 (2018); 94, 029901(E) (2022).
- N. Brambilla, S. Eidelman, C. Hanhart, A. Nefediev, C.-P. Shen, C. E. Thomas, A. Vairo, and C.-Z. Yuan, Phys. Rep. 873, 1 (2020).
- H.-X. Chen, W. Chen, X. Liu, Y.-R. Liu, and S.-L. Zhu, Rep. Prog. Phys. 86, 026201 (2023).
- M. Ablikim et al. (BESIII Collaboration), Phys. Rev. Lett. 126, 102001 (2021).
- L. Meng, B. Wang, and S.-L. Zhu, Phys. Rev. D 102, 111502 (2020).
- M. Karliner and J. L. Rosner, Phys. Rev. D 104, 034033 (2021).
- J. F. Giron, R. F. Lebed, and S. R. Martinez, Phys. Rev. D 104, 054001 (2021).
- T. Guo, J. Li, J. Zhao, and L. He, Chin. Phys. C 47, 063107 (2023).
- M.-Z. Liu, Y.-W. Pan, Z.-W. Liu, T.-W. Wu, J.-X. Lu, and L.-S. Geng, Phys. Rep. 1108, 1 (2025).
- R. Aaij et al. (LHCb Collaboration), Phys. Rev. Lett. 127, 082001 (2021).
- C. Mony A. and R. Dhir, J. Phys. G 51, 115004 (2024).
- C. A. Bokade and Bhaghyesh, Phys. Rev. D 111, 014030 (2025).
- S.-Y. Li, Y.-R. Liu, Z.-L. Man, Z.-G. Si, and J. Wu, Phys. Rev. D 110, 094044 (2024).
- R. Vogt, Phys. Rev. D 110, 074036 (2024).
- G.-L. Yu, Z.-Y. Li, Z.-G. Wang, B. WU, Z. Zhou, and J. Lu, Eur. Phys. J. C 84, 1130 (2024).
- Z. Yang, X. Cao, F.-K. Guo, J. Nieves, and M. P. Valderrama, Phys. Rev. D 103, 074029 (2021).
- K. Chen, Phys. Rev. D 109, 034010 (2024).
- M. Ablikim et al. (BESIII Collaboration), Chin. Phys. C 47, 033001 (2023).
- R. Aaij et al. (LHCb Collaboration), Phys. Rev. Lett. 131, 071901 (2023).
- A. M. Badalian and Y. A. Simonov, Eur. Phys. J. C 83, 410 (2023).
- J. Hoffer, G. Eichmann, and C. S. Fischer, Phys. Rev. D 109, 074025 (2024).
- X. Chen, Y. Tan, X. Liu, and J. Ping, Phys. Rev. D 111, 054018 (2025).
- R. Bruschini and P. González, Phys. Rev. D 102, 074002 (2020).
- O. Andreev, Phys. Rev. D 106, 066002 (2022).
- A. Deur, S. J. Brodsky, and G. F. de Teramond, Nucl. Phys. 90, 1 (2016).
- E. Braaten and M. Kusunoki, Phys. Rev. D 72, 054022 (2005).