REVIEW 3 major objections 7 minor 127 references
Faddeev equations for the $J/\psi\,NN$ and $\phi\,NN$ three-body systems in momentum space
T0 review · 3 major / 7 minor · reviewed 2026-08-15 · deepseek-v4-flash
Pith's one-line read Solving three-body Faddeev equations with lattice QCD two-body inputs, the paper finds phi-N-N bound states in three isospin-zero channels and no J/psi-N-N bound state.
desk verdict Solid momentum-space Faddeev calculation, but the phi NN bound states it advertises are inherited from earlier work and rest on the least reliable input in the model. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The engine is the Faddeev equations in momentum space, the exact coupled integral equations for three-body bound states. The two-body subsystem t-matrix comes from the Lippmann-Schwinger equation, solved by matrix inversion; the three-body equations are then discretized with cubic-spline interpolation and Gauss-Legendre quadrature, and the bound-state condition is recast as an auxiliary eigenvalue problem $K(z)|\varphi(z)\rangle = \lambda(z)|\varphi(z)\rangle$, with the physical binding energy found where $\lambda(E)=1$. Only S-wave two-body interactions are kept. The two controls are the constructed spin-1/2 phi-nucleon potentials: scheme I scales the spin-3/2 lattice potential by a factor fitted to measured phi-proton correlation functions, while scheme II assumes the spin-spin part of the phi-N and J/psi-N interactions is inversely proportional to the hadron masses.
What would settle it
Measure the near-threshold $\gamma d \to \phi d$ cross section; a bound phi-N-N state would appear as a sharp near-threshold enhancement whose energy sets the binding energy. Alternatively, a lattice QCD calculation of the spin-1/2 phi-N potential including the Lambda-K and Sigma-K coupled channels would determine whether the $0^-$ and $1^-$ bound states survive.
Extended reading notes
Core claim
The central numerical discovery is a sharp asymmetry between the charmonium and strange-meson three-body systems: with the two-body inputs adopted, the J/psi-N-N system has no three-body bound state, while the phi-N-N system supports bound states in the $(I)J^P=(0)0^-$, $(0)1^-$, and $(0)2^-$ channels in both schemes for the spin-1/2 phi-N force. The deepest state (about 50 MeV in scheme I) comes from the strongly attractive spin-1/2 phi-N interaction, which in that scheme even binds the two-body phi-N system; the shallowest (about 2.4 MeV) is the $2^-$ state, driven by the deuteron plus the spin-3/2 phi-N force and essentially identical in both schemes. In the isospin-one $1^-$ channel, where the nucleon pair is in the unbound $^1S_0$ channel, no bound state is found.
Load-bearing premise
The prediction rests on the strength of the spin-1/2 phi-nucleon interaction, a poorly known quantity for which lattice QCD provides no reliable potential because that channel is strongly coupled to open strange channels such as Lambda-K and Sigma-K, and both schemes are constructed guesses rather than measured inputs.
Editorial extensions
If this is right
- A phi-N-N bound state would appear near threshold in photon-induced phi production on the deuteron, such as $\gamma d \to \phi d$, with the final deuteron energy reflecting the binding energy.
- The $(0)2^-$ state is predicted in both schemes with essentially the same binding energy, making it the cleanest prediction to test.
- J/psi-N-N is predicted not to bind, so the charmonium-nucleon force remains too weak to form this kind of hadronic molecule.
- The spread between scheme I and scheme II in the $0^-$ and $1^-$ channels quantifies how much the unknown spin-spin part of the phi-N force controls the three-body spectrum.
Reading between the lines
- Because the $(0)2^-$ state is insensitive to the spin-1/2 ambiguity, an experimental search for a phi-N-N bound state should look first in that channel; not finding it would call the spin-3/2 phi-N input into question rather than the spin-1/2 schemes.
- The S-wave-only truncation probably underestimates the three-body attraction; adding higher partial waves and the open Lambda-K and Sigma-K channels could shift the binding energies and might even turn the isospin-one channel into a bound state.
- Using the Faddeev wave functions to compute the $\gamma d \to \phi d$ amplitude would convert the existence prediction into a quantitative cross-section prediction, giving experiment a sharper target.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This paper formulates momentum-space Faddeev equations for the J/psi NN and phi NN three-body systems with two identical nucleons. The two-body input consists of the Malfliet-Tjon NN potential, the HAL QCD J/psi N potentials in the 4S3/2 and 2S1/2 channels, the HAL QCD phi N potential in the 4S3/2 channel, and two constructed models for the phi N 2S1/2 channel: scheme I scales the HAL QCD 4S3/2 short-range part by beta=6.9 obtained from the ALICE phi p correlation function, and scheme II assumes that spin-spin interactions scale inversely with the hadron mass. The Lippmann-Schwinger equation is solved for the two-body t-matrix and the Faddeev equations are solved by discretization and diagonalization. The author reports no J/psi NN bound state and phi NN bound states in the (0)0-, (0)1-, and (0)2- channels in both schemes, with binding energies given in Tables V and VI.
Significance. The paper is a technically clean application of standard Faddeev machinery, and the two-body sector is checked by reproducing the input scattering lengths and the deuteron binding energy with the MT potential, which is a genuine internal consistency test. The strongest and least model-dependent result is the (0)2- phi NN bound state, which is driven by the well-determined HAL QCD 4S3/2 channel and is stable across the two schemes; this is a concrete prediction that could be probed in reactions such as gamma d -> phi d. The absence of a J/psi NN bound state is also consistent with the weak J/psi N interactions used. However, the (0)0- and (0)1- states rest on the phi N 2S1/2 interaction, which the author explicitly identifies as the least reliable input; the paper is transparent about this and offers two independent constructions, but neither construction is validated by data or lattice QCD. The falsifiable character of the prediction and the transparency about the unreliable channel are strengths of the manuscript.
major comments (3)
- [Section III C, Eq. (38), Tables V and VI] The existence of the (0)0- and (0)1- phi NN bound states rests entirely on the phi N 2S1/2 potential, and that potential is the least secure input in the calculation. Ref. [90] states explicitly that in the 2S1/2 channel the phi N potential is strongly coupled to the S-wave Lambda K and Sigma K channels and that the lattice information in this channel is not reliable. Scheme I replaces this channel with Eq. (38), scaling the 4S3/2 short-range Gaussian terms by beta=6.9 without any uncertainty or sensitivity analysis, while scheme II replaces it with Eq. (41), an untested inverse-mass scaling hypothesis. Because no strength variation or coupled-channel estimate is reported, the paper does not establish that the (0)0- and (0)1- bound states survive a moderate reduction of this interaction. I request a scan in the strength of the 2S1/2 potential, for example varying beta around 6.9 or scaling the whole potential, that identifies the critical strength at which each of these states disappears, or an estimate of the coupled-channel uncertainty.
- [Section IV C, Tables V and VI] The central numerical results are quoted as single numbers to two decimals with no propagated uncertainties and no numerical convergence tests. The input potentials carry uncertainties (Tables II and III), the factor beta has an unknown fit error, and the discretization parameters such as the number of Gauss-Legendre points, momentum cutoffs, and spline knots are not stated. For the (0)2- state with B3=2.39 MeV and for the scheme-II states with B3 around 3 MeV, this level of numerical detail is not sufficient to establish that the bound states are significant. Please add a convergence study and propagate at least the potential parameter uncertainties through the Faddeev equations.
- [Section III C, Eq. (23)] In both schemes the phi N 2S1/2 t-matrix is computed as a single-channel S-wave t-matrix, yet the dominant issue identified by HAL QCD for this channel is not a parameter uncertainty but missing coupled-channel dynamics due to the S-wave Lambda K and Sigma K channels. A single-channel potential fitted to the elastic phi p correlation function can reproduce an effective scattering length, but it cannot reproduce the coupled-channel physics that, according to Ref. [90], makes the lattice potential unreliable in this channel. The manuscript should state this limitation explicitly and, if possible, estimate the effect using a coupled-channel two-body model or a coupled-channel Faddeev calculation, since the (0)0- and (0)1- phi NN states are directly carried by this channel.
minor comments (7)
- [Table III] The caption states that 'alpha3 m_pi^4 and beta3 are in units of fm', which is dimensionally confusing because alpha3 m_pi^4 multiplies a 1/r^2 term; please clarify the units of the reported combination.
- [Eq. (38)] The factor beta is introduced without stating its normalization; please state that it is a dimensionless scaling factor and give its uncertainty from the fit to the ALICE phi p correlation function.
- [Tables V and VI] The notation '(I=1, JP=1- - (-))' is unclear; replace it with 'no bound state' or a consistent dash.
- [Section IV B] The absence of a J/psi NN bound state is reported without showing the largest eigenvalue of the Faddeev kernel in the relevant channels; a short table or a statement about the convergence of lambda(E) would strengthen this negative result.
- [Conclusions] The statement that the predicted bound states agree with Refs. [96-98] is not quantified; please give the corresponding binding energies from those references and explain what the present momentum-space treatment adds beyond them.
- [Section IV C] The binding energies are defined relative to the three-body threshold, but the threshold is not defined in the text; please state it explicitly as m_phi + 2 m_N (or as appropriate for the HAL QCD masses).
- [Eq. (38)] The two-pion exchange tail is not scaled by beta in scheme I; since the text justifies the tail as spin-independent, it would be helpful to state explicitly why only the short-range Gaussian terms are rescaled.
Circularity Check
No significant circularity: the phiNN binding energies are computed outputs of a fixed-input Faddeev calculation, with the only fitted parameter (beta in scheme I) entering the two-body input potential and never tuned to the three-body result.
full rationale
The paper's central claim is produced by solving the homogeneous Faddeev equation K(E)|psi> = |psi> (Eqs. 28-31), where the bound-state energy is fixed by the eigenvalue condition lambda(E)=1. All two-body inputs -- the Malfliet-Tjon NN potential, the HAL QCD J/psi N potentials, the HAL QCD phi N (4S3/2) potential, and the two constructed phi N (2S1/2) potentials -- are fixed before the three-body diagonalization. No parameter is adjusted to reproduce the reported B3 values. In particular, scheme I's beta=6.9 is determined by fitting the ALICE phi-p correlation function (Section III C, Eq. 38) and is an ingredient of the two-body phi N potential; the three-body output is not used to tune anything. This is a model-input uncertainty, not a fitted quantity renamed as a prediction. Scheme II's inverse-mass scaling assumption (Eqs. 39-41) is also an input hypothesis, not a recirculated output. The reproduction of HAL QCD scattering lengths in Table IV is a sanity check, not circularity. The agreement with Refs. [96-98] is an external cross-check by other groups using different methods; the author's only self-citation, Ref. [72], is peripheral to the three-body claim. The genuine weakness -- that the (0)0- and (0)1- phiNN states depend on the poorly constrained 2S1/2 phi N force, which HAL QCD itself flags as unreliable due to Lambda K / Sigma K coupling (Section III C) -- is a robustness concern, and the paper explicitly states the HAL QCD limitation. A strength scan would test stability, but the absence of one does not make the derivation circular. Therefore the derivation chain is self-contained: outputs are computed from stated inputs, with no equation reducing a prediction to its inputs by construction.
Assumptions & free parameters
free parameters (4)
- beta (scheme I phi N spin-1/2 scale) =
6.9
- MT potential strength parameters (1S0, 3S1) =
1S0: C1=-514 MeV fm, C2=1439 MeV fm; 3S1: C1=-627 MeV fm, C2=1439 MeV fm; mu1=1.55 fn^-1, mu2=3.11 fm^-1
- HAL QCD J/psi N potential parameters (Table II) =
See Table II, from Ref. [76]
- HAL QCD phi N spin-3/2 potential parameters (Table III) =
alpha1=-371(27) MeV, beta1=0.13(1) fm, alpha2=-119(39) MeV, beta2=0.30(5) fm, alpha3 m_pi^4=-97(14), beta3=0.63(4) fm
assumptions (6)
- standard math Faddeev decomposition and Lippmann-Schwinger equations are valid for these three-body systems
- domain assumption Only S-wave two-body interactions contribute; higher partial waves are neglected
- ad hoc to paper The phi N spin-1/2 interaction can be represented by a single-channel potential
- ad hoc to paper Spin-spin parts of phi N and J/psi N interactions are inversely proportional to hadron masses (scheme II)
- ad hoc to paper The spin-1/2 phi N potential in scheme I is obtained by scaling the spin-3/2 HAL QCD potential by beta=6.9 and adding the same two-pion tail
- domain assumption Non-relativistic kinematics with static potentials is adequate near threshold
Cite this review
Pith. "Pith review of Faddeev equations for the $J/\psi\,NN$ and $\phi\,NN$ three-body systems in momentum space." pith.science (2026). https://pith.science/paper/LBQBRBMX
@misc{pith2026260803162,
author = {Pith},
title = {Pith review of: Faddeev equations for the $J/\psi\,NN$ and $\phi\,NN$ three-body systems in momentum space},
year = {2026},
howpublished = {\url{https://pith.science/paper/LBQBRBMX}},
note = {Machine review of arXiv:2608.03162}
}
abstract
We construct Faddeev equations for the $J/\psi\,NN$ and $\phi\,NN$ three-body systems in momentum space. The two-body subsystem $t$-matrix is obtained by solving the Lippmann-Schwinger equations. The $NN$ interactions are constructed using the Malfliet-Tjon potential. The $J/\psi\,N$ interaction potentials in the ${}^4S_{3/2}$ and ${}^2S_{1/2}$ channels are taken from HAL QCD. The $\phi\,N$ interaction potential in the ${}^4S_{3/2}$ channel is also taken from HAL QCD. The ${}^2S_{1/2}$ $\phi N$ interaction is obtained from the combination of the $\phi p$ correlation function analysis and the HAL QCD results, as well as from the assumption that the spin-spin parts of the $\phi N$ and $J/\psi N$ interactions are inversely proportional to the respective hadron masses. The Faddeev equations are solved to find bound states in the $J/\psi\,NN$ and $\phi\,NN$ three-body systems. The numerical results suggest that there exist bound states in the $\phi\,NN$ three-body system, while there is no bound state in the $J/\psi\,NN$ system.
Reference graph
Works this paper leans on
-
[99]
L.-Z. Wen, Y. Ma, L. Meng, and S.-L. Zhu, Phys. Rev. D111, 114004 (2025), [Erratum: Phys.Rev.D 112, 039901 (2025)], arXiv:2503.11938 [hep-ph]
arXiv 2025
-
[90]
R. Mutoet al.(KEK-PS-E325), Phys. Rev. Lett.98, 042501 (2007), arXiv:nucl-ex/0511019
arXiv 2007
-
[1]
In this channel, the two-body subsystemNNis in the 3S1 channel, andϕNis in the 2S1/2 channel
SchemeI In scheme I, there exists a deep bound state in the (I)JP = (0)0− channel. In this channel, the two-body subsystemNNis in the 3S1 channel, andϕNis in the 2S1/2 channel. TheNNinteraction in the 3S1 channel is strong and forms the deuteron. TheϕNinteraction in the 2S1/2 channel is even stronger, and can form a bound state with binding energy around ...
-
[2]
The 2S1/2 ϕN interaction cannot form a two-body bound state
SchemeII In scheme II, the strength of the 2S1/2 ϕNinterac- tion is weaker compared to scheme I. The 2S1/2 ϕN interaction cannot form a two-body bound state. We found bound states in the three-bodyϕNNsystem in the (I)J P = (0)0−, (0)1−, and (0)2− channels. In the (I)JP = (0)0− channel, the binding energy of theϕNN three-body system is smaller compared wit...
-
[3]
F. Grosset al., Eur. Phys. J. C83, 1125 (2023), arXiv:2212.11107 [hep-ph]
arXiv 2023
-
[4]
D. J. Gross and F. Wilczek, Phys. Rev. Lett.30, 1343 (1973)
1973
-
[5]
H. D. Politzer, Phys. Rev. Lett.30, 1346 (1973)
1973
-
[6]
M. E. Peskin, Nucl. Phys. B156, 365 (1979)
1979
Show all 127 references
-
[7]
Kharzeev, Proc
D. Kharzeev, Proc. Int. Sch. Phys. Fermi130, 105 11 (1996), arXiv:nucl-th/9601029
1996 arXiv
-
[8]
Kharzeev, H
D. Kharzeev, H. Satz, A. Syamtomov, and G. Zinovjev, Eur. Phys. J. C9, 459 (1999), arXiv:hep-ph/9901375
1999 arXiv
-
[9]
Gottfried, Phys
K. Gottfried, Phys. Rev. Lett.40, 598 (1978)
1978
-
[10]
Bhanot and M
G. Bhanot and M. E. Peskin, Nucl. Phys. B156, 391 (1979)
1979
-
[11]
M. B. Voloshin, Nucl. Phys. B154, 365 (1979)
1979
-
[12]
We expand the combination as a Legendre series, δ(p−π 12) pl+2 δ(p′−π′ 12) p′l′+2 = X k 2π p ˆk(−1)kgkY 00 kk(ˆq′ ˆq),(A11) where the coefficientsg k are defined as gk = Z 1 −1 dxP k(x) δ p− r m2 2 m2 23 q2 +q′2 + 2m2 m23 qq′x pl+2 δ p′− r q2 + m2 1 m2 13 q′2 + 2m1 m13 qq′x p′...
-
[13]
Appelquist and W
T. Appelquist and W. Fischler, Phys. Lett. B77, 405 (1978)
1978
-
[14]
M. E. Luke, A. V. Manohar, and M. J. Savage, Phys. Lett. B288, 355 (1992), arXiv:hep-ph/9204219
1992 arXiv
-
[15]
Ji, Phys
X.-D. Ji, Phys. Rev. Lett.74, 1071 (1995), arXiv:hep- ph/9410274
1995
-
[16]
Hatta and D.-L
Y. Hatta and D.-L. Yang, Phys. Rev. D98, 074003 (2018), arXiv:1808.02163 [hep-ph]
2018 arXiv
- [17]
-
[18]
S. J. Brodsky, I. A. Schmidt, and G. F. de Teramond, Phys. Rev. Lett.64, 1011 (1990)
1990
-
[19]
Tarr´ us Castell` a and G
J. Tarr´ us Castell` a and G. Krein, Phys. Rev. D98, 014029 (2018), arXiv:1803.05412 [hep-ph]
2018 arXiv
-
[20]
Wu, X.-K
B. Wu, X.-K. Dong, M.-L. Du, F.-K. Guo, and B.-S. Zou, Fund. Res.5, 2530 (2025), arXiv:2410.19526 [hep- ph]
2025
-
[21]
Aaijet al.(LHCb), Phys
R. Aaijet al.(LHCb), Phys. Rev. Lett.115, 072001 (2015), arXiv:1507.03414 [hep-ex]
2015 arXiv
-
[22]
Aaijet al.(LHCb), Phys
R. Aaijet al.(LHCb), Phys. Rev. Lett.117, 082002 (2016), arXiv:1604.05708 [hep-ex]
2016 arXiv
-
[23]
Aaijet al.(LHCb), Phys
R. Aaijet al.(LHCb), Phys. Rev. Lett.122, 222001 (2019), arXiv:1904.03947 [hep-ex]
2019 arXiv
-
[24]
J.-J. Wu, R. Molina, E. Oset, and B. S. Zou, Phys. Rev. Lett.105, 232001 (2010), arXiv:1007.0573 [nucl-th]
2010 arXiv
-
[25]
Liu, Y.-W
M.-Z. Liu, Y.-W. Pan, F.-Z. Peng, M. S´ anchez S´ anchez, L.-S. Geng, A. Hosaka, and M. Pavon Valderrama, Phys. Rev. Lett.122, 242001 (2019), arXiv:1903.11560 [hep-ph]
2019 arXiv
-
[26]
Fern´ andez-Ram´ ırez, A
C. Fern´ andez-Ram´ ırez, A. Pilloni, M. Albaladejo, A. Jackura, V. Mathieu, M. Mikhasenko, J. A. Silva- Castro, and A. P. Szczepaniak (JPAC), Phys. Rev. Lett. 123, 092001 (2019), arXiv:1904.10021 [hep-ph]
2019 arXiv
-
[27]
M.-L. Du, V. Baru, F.-K. Guo, C. Hanhart, U.-G. Meißner, J. A. Oller, and Q. Wang, Phys. Rev. Lett. 124, 072001 (2020), arXiv:1910.11846 [hep-ph]
2020 arXiv
-
[28]
H.-X. Chen, W. Chen, and S.-L. Zhu, Phys. Rev. D 100, 051501 (2019), arXiv:1903.11001 [hep-ph]
2019 arXiv
-
[29]
Chen, Z.-F
R. Chen, Z.-F. Sun, X. Liu, and S.-L. Zhu, Phys. Rev. D100, 011502 (2019), arXiv:1903.11013 [hep-ph]
2019 arXiv
-
[30]
J. He, Eur. Phys. J. C79, 393 (2019), arXiv:1903.11872 [hep-ph]
2019 arXiv
-
[31]
Guo and J
Z.-H. Guo and J. A. Oller, Phys. Lett. B793, 144 (2019), arXiv:1904.00851 [hep-ph]
2019 arXiv
-
[32]
C.-J. Xiao, Y. Huang, Y.-B. Dong, L.-S. Geng, and D.-Y. Chen, Phys. Rev. D100, 014022 (2019), arXiv:1904.00872 [hep-ph]
2019 arXiv
-
[33]
B. Wang, L. Meng, and S.-L. Zhu, JHEP11, 108 (2019), arXiv:1909.13054 [hep-ph]
2019 arXiv
-
[34]
C. W. Xiao, J. Nieves, and E. Oset, Phys. Rev. D100, 014021 (2019), arXiv:1904.01296 [hep-ph]
2019 arXiv
-
[35]
L. Meng, B. Wang, G.-J. Wang, and S.-L. Zhu, Phys. Rev. D100, 014031 (2019), arXiv:1905.04113 [hep-ph]
2019 arXiv
-
[36]
M. B. Voloshin, Phys. Rev. D100, 034020 (2019), arXiv:1907.01476 [hep-ph]
2019 arXiv
-
[37]
Wang and X
Z.-G. Wang and X. Wang, Chin. Phys. C44, 103102 (2020), arXiv:1907.04582 [hep-ph]
2020 arXiv
-
[38]
Yamaguchi, H
Y. Yamaguchi, H. Garc´ ıa-Tecocoatzi, A. Giachino, A. Hosaka, E. Santopinto, S. Takeuchi, and M. Takizawa, Phys. Rev. D101, 091502 (2020), arXiv:1907.04684 [hep-ph]
2020 arXiv
-
[39]
Lin and B.-S
Y.-H. Lin and B.-S. Zou, Phys. Rev. D100, 056005 (2019), arXiv:1908.05309 [hep-ph]
2019 arXiv
-
[40]
Gutsche and V
T. Gutsche and V. E. Lyubovitskij, Phys. Rev. D100, 094031 (2019), arXiv:1910.03984 [hep-ph]
2019 arXiv
-
[41]
T. J. Burns and E. S. Swanson, Phys. Rev. D100, 114033 (2019), arXiv:1908.03528 [hep-ph]
2019 arXiv
-
[42]
R. Zhu, X. Liu, H. Huang, and C.-F. Qiao, Phys. Lett. B797, 134869 (2019), arXiv:1904.10285 [hep-ph]
2019 arXiv
-
[43]
Wang, L.-Y
G.-J. Wang, L.-Y. Xiao, R. Chen, X.-H. Liu, X. Liu, and S.-L. Zhu, Phys. Rev. D102, 036012 (2020), arXiv:1911.09613 [hep-ph]
2020 arXiv
-
[44]
M.-L. Du, V. Baru, F.-K. Guo, C. Hanhart, U.-G. Meißner, J. A. Oller, and Q. Wang, JHEP08, 157 (2021), arXiv:2102.07159 [hep-ph]
2021 arXiv
-
[45]
C.-W. Shen, D. R¨ onchen, U.-G. Meißner, B.-S. Zou, and Y.-F. Wang, Eur. Phys. J. C84, 764 (2024), arXiv:2405.02626 [hep-ph]
2024 arXiv
-
[46]
Gell-Mann and F
M. Gell-Mann and F. Zachariasen, Phys. Rev.124, 953 (1961)
1961
-
[47]
N. M. Kroll, T. D. Lee, and B. Zumino, Phys. Rev. 157, 1376 (1967)
1967
-
[48]
E. A. Kuraev, L. N. Lipatov, and V. S. Fadin, Sov. Phys. JETP45, 199 (1977)
1977
-
[49]
I. I. Balitsky and L. N. Lipatov, Sov. J. Nucl. Phys.28, 822 (1978)
1978
-
[50]
T. H. Bauer, R. D. Spital, D. R. Yennie, and F. M. Pipkin, Rev. Mod. Phys.50, 261 (1978), [Erratum: Rev.Mod.Phys. 51, 407 (1979)]
1978
-
[51]
Pumplin and W
J. Pumplin and W. Repko, Phys. Rev. D12, 1376 (1975)
1975
-
[52]
V. D. Barger and R. J. N. Phillips, Phys. Lett. B58, 433 (1975)
1975
-
[53]
Gittelman, K
B. Gittelman, K. M. Hanson, D. Larson, E. Loh, A. Sil- verman, and G. Theodosiou, Phys. Rev. Lett.35, 1616 (1975)
1975
-
[54]
Camerini, J
U. Camerini, J. G. Learned, R. Prepost, C. M. Spencer, D. E. Wiser, W. Ash, R. L. Anderson, D. Ritson, D. Sherden, and C. K. Sinclair, Phys. Rev. Lett.35, 483 (1975)
1975
-
[55]
Aliet al.(GlueX), Phys
A. Aliet al.(GlueX), Phys. Rev. Lett.123, 072001 (2019), arXiv:1905.10811 [nucl-ex]
2019 arXiv
-
[56]
Adhikariet al.(GlueX), Phys
S. Adhikariet al.(GlueX), Phys. Rev. C108, 025201 (2023), arXiv:2304.03845 [nucl-ex]
2023 arXiv
-
[57]
Duranet al., Nature615, 813 (2023), arXiv:2207.05212 [nucl-ex]
B. Duranet al., Nature615, 813 (2023), arXiv:2207.05212 [nucl-ex]
2023 arXiv
-
[58]
Joostenet al.(007), (2026), arXiv:2602.14416 [nucl- ex]
S. Joostenet al.(007), (2026), arXiv:2602.14416 [nucl- ex]
2026
-
[59]
Chatagnonet al.(CLAS), Phys
P. Chatagnonet al.(CLAS), Phys. Rev. C113, 065203 (2026), arXiv:2602.22128 [hep-ex]
2026 arXiv
-
[60]
Strakovsky, D
I. Strakovsky, D. Epifanov, and L. Pentchev, Phys. Rev. C101, 042201 (2020), arXiv:1911.12686 [hep-ph]
2020 arXiv
-
[61]
Winneyet al.(Joint Physics Analysis Center), Phys
D. Winneyet al.(Joint Physics Analysis Center), Phys. Rev. D108, 054018 (2023), arXiv:2305.01449 [hep-ph]
2023 arXiv
-
[62]
I. I. Strakovsky, W. J. Briscoe, J. K. Ahn, M. G. Ryskin, and A. Schmidt, Phys. Rev. D113, 114023 (2026), arXiv:2603.09622 [hep-ph]
2026 arXiv
-
[63]
Wang, X.-H
Q. Wang, X.-H. Liu, and Q. Zhao, Phys. Rev. D92, 034022 (2015), arXiv:1508.00339 [hep-ph]
2015 arXiv
-
[64]
Kubarovsky and M
V. Kubarovsky and M. B. Voloshin, Phys. Rev. D92, 12 031502 (2015), arXiv:1508.00888 [hep-ph]
2015 arXiv
-
[65]
Karliner and J
M. Karliner and J. L. Rosner, Phys. Lett. B752, 329 (2016), arXiv:1508.01496 [hep-ph]
2016 arXiv
-
[66]
A. N. Hiller Blin, C. Fern´ andez-Ram´ ırez, A. Jackura, V. Mathieu, V. I. Mokeev, A. Pilloni, and A. P. Szczepaniak, Phys. Rev. D94, 034002 (2016), arXiv:1606.08912 [hep-ph]
2016 arXiv
-
[67]
Winney, C
D. Winney, C. Fanelli, A. Pilloni, A. N. Hiller Blin, C. Fern´ andez-Ram´ ırez, M. Albaladejo, V. Mathieu, V. I. Mokeev, and A. P. Szczepaniak (JPAC), Phys. Rev. D 100, 034019 (2019), arXiv:1907.09393 [hep-ph]
2019 arXiv
-
[68]
Wang, X.-R
X.-Y. Wang, X.-R. Chen, and J. He, Phys. Rev. D99, 114007 (2019), arXiv:1904.11706 [hep-ph]
2019 arXiv
-
[69]
J.-J. Wu, T. S. H. Lee, and B.-S. Zou, Phys. Rev. C 100, 035206 (2019), arXiv:1906.05375 [nucl-th]
2019 arXiv
-
[70]
Cao and J.-p
X. Cao and J.-p. Dai, Phys. Rev. D100, 054033 (2019), arXiv:1904.06015 [hep-ph]
2019 arXiv
-
[71]
E. Y. Paryev, Nucl. Phys. A1029, 122562 (2023), arXiv:2211.16037 [hep-ph]
2023 arXiv
-
[72]
Strakovsky, W
I. Strakovsky, W. J. Briscoe, E. Chudakov, I. Larin, L. Pentchev, A. Schmidt, and R. L. Workman, Phys. Rev. C108, 015202 (2023), arXiv:2304.04924 [hep-ph]
2023 arXiv
- [73]
-
[74]
M.-X. Duan, C. Gong, L. Qiu, and Q. Zhao, (2024), arXiv:2409.10364 [hep-ph]
2024 arXiv
- [75]
- [76]
-
[77]
Yokokawa, S
K. Yokokawa, S. Sasaki, T. Hatsuda, and A. Hayashigaki, Phys. Rev. D74, 034504 (2006), arXiv:hep-lat/0605009
2006 arXiv
-
[78]
Skerbis and S
U. Skerbis and S. Prelovsek, Phys. Rev. D99, 094505 (2019), arXiv:1811.02285 [hep-lat]
2019 arXiv
-
[79]
Y. Lyu, T. Doi, T. Hatsuda, and T. Sugiura, Phys. Lett. B860, 139178 (2025), arXiv:2410.22755 [hep-lat]
2025 arXiv
-
[80]
L. D. Faddeev, Sov. Phys. JETP12, 1014 (1961)
1961
-
[81]
L. D. Faddeev,Mathematical aspects of the three-body problem in the quantum scattering theory(Israel Pro- gram for Scientific Translations, Jerusalem, 1965)
1965
-
[82]
Gl¨ ockle,The Quantum Mechanical Few-Body Prob- lem(Springer, Berlin, Heidelberg, 1983)
W. Gl¨ ockle,The Quantum Mechanical Few-Body Prob- lem(Springer, Berlin, Heidelberg, 1983)
1983
-
[83]
H. Gao, T. S. H. Lee, and V. Marinov, Phys. Rev. C 63, 022201 (2001), arXiv:nucl-th/0010042
2001 arXiv
-
[84]
H. Gao, H. Huang, T. Liu, J. Ping, F. Wang, and Z. Zhao, Phys. Rev. C95, 055202 (2017), arXiv:1701.03210 [hep-ph]
2017 arXiv
-
[85]
Huang, Z
F. Huang, Z. Y. Zhang, and Y. W. Yu, Phys. Rev. C 73, 025207 (2006), arXiv:nucl-th/0512079
2006 arXiv
-
[86]
J. He, H. Huang, D.-Y. Chen, and X. Zhu, Phys. Rev. D98, 094019 (2018), arXiv:1804.09383 [hep-ph]
2018 arXiv
-
[87]
Ishikawaet al., Phys
T. Ishikawaet al., Phys. Lett. B608, 215 (2005), arXiv:nucl-ex/0411016
2005 arXiv
-
[88]
M. H. Woodet al.(CLAS), Phys. Rev. Lett.105, 112301 (2010), arXiv:1006.3361 [nucl-ex]
2010 arXiv
-
[89]
B. Dey, C. A. Meyer, M. Bellis, and M. Williams (CLAS), Phys. Rev. C89, 055208 (2014), [Addendum: Phys.Rev.C 90, 019901 (2014)], arXiv:1403.2110 [nucl- ex]
2014 arXiv
-
[91]
Polyanskiyet al., Phys
A. Polyanskiyet al., Phys. Lett. B695, 74 (2011), arXiv:1008.0232 [nucl-ex]
2011 arXiv
-
[92]
I. I. Strakovsky, L. Pentchev, and A. Titov, Phys. Rev. C101, 045201 (2020), arXiv:2001.08851 [hep-ph]
2020 arXiv
-
[93]
Y. Lyu, T. Doi, T. Hatsuda, Y. Ikeda, J. Meng, K. Sasaki, and T. Sugiura, Phys. Rev. D106, 074507 (2022), arXiv:2205.10544 [hep-lat]
2022 arXiv
-
[94]
V. B. Belyaev, W. Sandhas, and I. I. Shlyk, Few Body Syst.44, 347 (2008), arXiv:0707.4615 [nucl-th]
2008 arXiv
-
[95]
V. B. Belyaev, W. Sandhas, and I. I. Shlyk, (2009), arXiv:0903.1703 [nucl-th]
2009 arXiv
-
[96]
S. A. Sofianos, G. J. Rampho, M. Braun, and R. M. Adam, Journal of Physics G: Nuclear and Particle Physics37, 085109 (2010)
2010
-
[97]
Etminan and A
F. Etminan and A. Aalimi, Phys. Rev. C109, 054002 (2024), arXiv:2402.06914 [nucl-th]
2024 arXiv
-
[98]
Filikhin, R
I. Filikhin, R. Y. Kezerashvili, and B. Vlahovic, Phys. Rev. D110, L031502 (2024), arXiv:2407.12190 [nucl- th]
2024 arXiv
-
[100]
Lazauskas, R
R. Lazauskas, R. Y. Kezerashvili, and I. Filikhin, Phys. Rev. D113, 074024 (2026)
2026
-
[101]
Lazauskas, R
R. Lazauskas, R. Y. Kezerashvili, and I. Filikhin, Phys. Lett. B877, 140496 (2026), arXiv:2601.14572 [nucl-th]
2026 arXiv
-
[102]
Yokota, E
A. Yokota, E. Hiyama, and M. Oka, PTEP2013, 113D01 (2013), arXiv:1308.6102 [nucl-th]
2013 arXiv
-
[103]
Chizzali, Y
E. Chizzali, Y. Kamiya, R. Del Grande, T. Doi, L. Fab- bietti, T. Hatsuda, and Y. Lyu, Phys. Lett. B848, 138358 (2024), arXiv:2212.12690 [nucl-ex]
2024 arXiv
-
[104]
Laverne and C
A. Laverne and C. Gignoux, Nucl. Phys. A203, 597 (1973)
1973
-
[105]
G. L. Payne, J. L. Friar, B. F. Gibson, and I. R. Afnan, Phys. Rev. C22, 823 (1980)
1980
-
[106]
Payne, B
G. Payne, B. F. Gibson, and J. L. Friar, Phys. Rev. C 22, 832 (1980)
1980
-
[107]
J. M. Blatt and V. F. Weisskopf,Theoretical Nuclear Physics(John Wiley & Sons, New York, 1952)
1952
-
[108]
M. I. Haftel and F. Tabakin, Nucl. Phys. A158, 1 (1970)
1970
-
[109]
R. L. Burden, J. D. Faires, and A. M. Burden,Numer- ical Analysis, 10th ed. (Cengage Learning, 2016)
2016
-
[110]
W. H. Press, S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery,Numerical Recipes: The Art of Scientific Computing, 3rd ed. (Cambridge University Press, 2007)
2007
-
[111]
Stadler, W
A. Stadler, W. Glockle, and P. U. Sauer, Phys. Rev. C 44, 2319 (1991)
1991
-
[112]
Gloeckle, Nucl
W. Gloeckle, Nucl. Phys. A381, 343 (1982)
1982
-
[113]
C. R. Chen, G. L. Payne, J. L. Friar, and B. F. Gibson, Phys. Rev. C33, 1740 (1986)
1986
-
[114]
C. R. Chen, G. L. Payne, J. L. Friar, and B. F. Gibson, Phys. Rev. C44, 50 (1991)
1991
-
[115]
R. B. Wiringa, V. G. J. Stoks, and R. Schiavilla, Phys. Rev. C51, 38 (1995), arXiv:nucl-th/9408016
1995 arXiv
- [116]
-
[117]
V. G. J. Stoks, R. A. M. Klomp, C. P. F. Terheggen, and J. J. de Swart, Phys. Rev. C49, 2950 (1994), arXiv:nucl-th/9406039
1994 arXiv
-
[118]
Epelbaum, H
E. Epelbaum, H. Krebs, and U. G. Meißner, Eur. Phys. J. A51, 53 (2015), arXiv:1412.0142 [nucl-th]
2015 arXiv
-
[119]
R. A. Malfliet and J. A. Tjon, Nucl. Phys. A127, 161 (1969)
1969
-
[120]
J. L. Friaret al., Phys. Rev. C42, 1838 (1990)
1990
-
[121]
Gloeckle, H
W. Gloeckle, H. Witala, D. Huber, H. Kamada, and 13 J. Golak, Phys. Rept.274, 107 (1996)
1996
-
[122]
Navratil, G
P. Navratil, G. P. Kamuntavicius, and B. R. Barrett, Phys. Rev. C61, 044001 (2000), arXiv:nucl-th/9907054
2000 arXiv
-
[123]
Kievsky, S
A. Kievsky, S. Rosati, M. Viviani, L. E. Marcucci, and L. Girlanda, J. Phys. G35, 063101 (2008), arXiv:0805.4688 [nucl-th]
2008 arXiv
-
[124]
Leidemann and G
W. Leidemann and G. Orlandini, Prog. Part. Nucl. Phys.68, 158 (2013), arXiv:1204.4617 [nucl-th]
2013 arXiv
-
[125]
Abramowitz and I
M. Abramowitz and I. A. Stegun,Handbook of Mathe- matical Functions with Formulas, Graphs, and Mathe- matical Tables(Dover, New York, 1964)
1964
-
[126]
Balian and E
R. Balian and E. Brezin, Nuovo Cim. B61, 403 (1969)
1969
-
[127]
A. R. Edmonds,Angular Momentum in Quantum Me- chanics(Princeton University Press, Princeton, New Jersey, 1957)
1957
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