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arxiv: 1906.08553 · v2 · pith:GJI7Q5JWnew · submitted 2019-06-20 · ✦ hep-ph · hep-ex

Deciphering the X(3872) via its polarization in prompt production at the CERN LHC

Pith reviewed 2026-05-25 19:54 UTC · model grok-4.3

classification ✦ hep-ph hep-ex
keywords X(3872)polarizationprompt hadroproductionnonrelativistic QCDexotic hadronχ_c1(2P)LHC
0
0 comments X

The pith

The X(3872) is predicted to be largely longitudinally polarized in prompt production at the LHC while the J/ψ from its decay is largely transverse.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper calculates the polarization of the X(3872) in prompt hadroproduction at the CERN LHC to next-to-leading order in the strong coupling constant within nonrelativistic QCD factorization. It assumes the X(3872) is a mixture of states but that production occurs mainly through its χ_c1(2P) component, including both color-singlet and color-octet contributions. The resulting prediction is that the X(3872) is mostly longitudinally polarized while the J/ψ it decays into is mostly transversely polarized, for the acceptance cuts of ATLAS, CMS, and LHCb. A sympathetic reader would care because polarization is an observable that current LHC experiments can measure and because the result offers a concrete test of whether the X(3872) contains a dominant conventional charmonium piece.

Core claim

Based on the hypothesis that the X(3872) exotic hadron is a mixture of χ_c1(2P) and other states and that its prompt hadroproduction predominately proceeds via its χ_c1(2P) component, the prompt-X(3872) polarization at the CERN LHC is calculated through next-to-leading order in α_s within the factorization formalism of nonrelativistic QCD, including both the color-singlet 3P1[1] and color-octet 3S1[8] c c-bar Fock states. The prediction is that the X(3872) is largely longitudinally polarized, while the J/ψ produced by the subsequent X(3872) decay is largely transversely polarized under ATLAS, CMS, and LHCb experimental conditions.

What carries the argument

Next-to-leading-order nonrelativistic QCD factorization for the polarization of the χ_c1(2P) component, incorporating color-singlet 3P1[1] and color-octet 3S1[8] Fock states in hadroproduction.

If this is right

  • Polarization measurements at ATLAS, CMS, and LHCb can distinguish whether the χ_c1(2P) component dominates the X(3872) wave function.
  • The same framework can be applied to other exotic states with non-zero spin to test analogous production hypotheses.
  • The J/ψ from X(3872) decay will carry different polarization information than directly produced J/ψ.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Confirmation of the predicted polarizations would favor models in which the X(3872) retains substantial conventional charmonium content over pure molecular pictures.
  • The method supplies a template that could be tested in other collider environments or for additional exotic candidates.
  • If the assumption holds, prompt production at hadron colliders becomes a diagnostic tool for the internal composition of spin-carrying exotics.

Load-bearing premise

The prompt hadroproduction of the X(3872) predominately proceeds via its χ_c1(2P) component.

What would settle it

An LHC measurement showing the X(3872) to be transversely polarized or the J/ψ longitudinally polarized under the same experimental conditions would falsify the central prediction.

Figures

Figures reproduced from arXiv: 1906.08553 by Bernd A. Kniehl, Mathias Butenschoen, Zhi-Guo He.

Figure 1
Figure 1. Figure 1: FIG. 1: The [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2: The differential cross sections of prompt [PITH_FULL_IMAGE:figures/full_fig_p003_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3 [PITH_FULL_IMAGE:figures/full_fig_p004_3.png] view at source ↗
read the original abstract

Based on the hypothesis that the $X(3872)$ exotic hadron is a mixture of $\chi_{c1}(2P)$ and other states and that its prompt hadroproduction predominately proceeds via its $\chi_{c1}(2P)$ component, we calculate the prompt-$X(3872)$ polarization at the CERN LHC through next-to-leading order in $\alpha_s$ within the factorization formalism of nonrelativistic QCD, including both the color-singlet $^3\!P_1^{[1]}$ and color-octet $^3\!S_1^{[8]}$ $c\bar c$ Fock states. We also consider the polarization of the $J/\psi$ produced by the subsequent $X(3872)$ decay. We predict that, under ATLAS, CMS, and LHCb experimental conditions, the $X(3872)$ is largely longitudinally polarized, while the $J/\psi$ is largely transversely polarized. We propose that the LHC experiments perform such polarization measurements to pin down the nature of the $X(3872)$ and other $X$, $Y$, $Z$ exotic states with non-zero spin.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript calculates the prompt hadroproduction polarization of the X(3872) at NLO in NRQCD (color-singlet ³P₁[¹] plus color-octet ³S₁[⁸]) under the explicit hypothesis that production proceeds predominantly via the χ_c1(2P) component of a mixed state. It also computes the polarization of the J/ψ arising from the subsequent X(3872) decay and predicts that, for ATLAS/CMS/LHCb kinematics, the X(3872) is largely longitudinally polarized while the J/ψ is largely transversely polarized. The result is framed as a testable diagnostic for the internal structure of the X(3872) and similar exotics.

Significance. If the production hypothesis holds, the work supplies a concrete, falsifiable polarization observable that LHC experiments can measure to constrain the χ_c1(2P) admixture. The inclusion of NLO corrections and both color-singlet and color-octet channels is a methodological strength; the conditional framing avoids overclaiming.

major comments (2)
  1. [§3] §3 (or equivalent results section): the numerical polarization predictions rely on specific LDME values for the χ_c1(2P) component, yet the manuscript provides neither the explicit numerical inputs nor an error-propagation or sensitivity analysis; because the central claim is a quantitative prediction, this omission directly affects the reliability of the quoted polarization fractions.
  2. [§4] The polarization result is stated to be largely independent of the mixing angle once the dominance hypothesis is imposed, but no explicit scan or derivative with respect to the mixing fraction is shown; a brief quantification would strengthen the claim that the prediction is robust under the stated assumption.
minor comments (2)
  1. [Abstract] The abstract and introduction should explicitly state the numerical LDME set adopted (or cite the precise reference and values) so that readers can immediately reproduce the quoted polarization numbers.
  2. [Figures] Figure captions for the polarization plots should include the exact kinematic cuts (p_T, |y|) corresponding to each LHC experiment so that the comparison with data is unambiguous.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the careful review and the constructive comments. We address the major points below and will revise the manuscript accordingly to improve clarity and transparency.

read point-by-point responses
  1. Referee: [§3] §3 (or equivalent results section): the numerical polarization predictions rely on specific LDME values for the χ_c1(2P) component, yet the manuscript provides neither the explicit numerical inputs nor an error-propagation or sensitivity analysis; because the central claim is a quantitative prediction, this omission directly affects the reliability of the quoted polarization fractions.

    Authors: We agree that the explicit LDME values and a sensitivity analysis are important for the reliability of the quantitative predictions. In the revised manuscript we will add the specific numerical LDME inputs employed for the χ_c1(2P) component together with a brief sensitivity study showing the effect of reasonable variations on the predicted polarization fractions. revision: yes

  2. Referee: [§4] The polarization result is stated to be largely independent of the mixing angle once the dominance hypothesis is imposed, but no explicit scan or derivative with respect to the mixing fraction is shown; a brief quantification would strengthen the claim that the prediction is robust under the stated assumption.

    Authors: Under the explicit dominance hypothesis the non-χ_c1(2P) contribution is taken to be negligible, rendering the polarization independent of the mixing angle by construction. Nevertheless, to strengthen the presentation we will include a short quantification (e.g., a brief scan or derivative) of the residual dependence for small admixtures in the revised version. revision: yes

Circularity Check

0 steps flagged

No significant circularity identified

full rationale

The paper states its central result as conditional on the explicit hypothesis that prompt hadroproduction proceeds predominantly via the χ_c1(2P) component. It then performs a standard NLO NRQCD factorization calculation of the polarization observables (color-singlet ³P₁[¹] plus color-octet ³S₁[⁸] channels, followed by the X(3872) → J/ψ decay chain). The LDMEs are external inputs taken from the literature or determined from independent processes; the polarization fractions constitute a distinct, falsifiable observable rather than a re-expression of the fitted cross-section inputs. No self-definitional equations, fitted-input-renamed-as-prediction steps, or load-bearing self-citation chains appear in the derivation chain. The work is therefore self-contained against external benchmarks.

Axiom & Free-Parameter Ledger

2 free parameters · 2 axioms · 0 invented entities

The central claim rests on the NRQCD factorization formalism, the assumption that production proceeds via the χ_c1(2P) component, and the use of color-singlet and color-octet LDMEs whose values are determined outside the present calculation.

free parameters (2)
  • NRQCD long-distance matrix elements
    Color-singlet ^3P_1^[1] and color-octet ^3S_1^[8] matrix elements are required for the NLO calculation and are conventionally fitted to data.
  • mixing fraction or angle
    The hypothesis that X(3872) is a mixture implies at least one parameter controlling the χ_c1(2P) component weight, which is not numerically specified in the abstract.
axioms (2)
  • domain assumption NRQCD factorization applies to prompt production of the X(3872)
    Invoked to justify the perturbative calculation of the short-distance coefficients.
  • ad hoc to paper Prompt hadroproduction of X(3872) proceeds predominantly via its χ_c1(2P) component
    Explicitly stated as the working hypothesis that enables the polarization prediction.

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Reference graph

Works this paper leans on

52 extracted references · 52 canonical work pages

  1. [1]

    have established the J P C = 1 ++ quantum numbers of the X(3872), and the very precise world average of its mass is mX = 3871 . 69 ± 0. 17 MeV [9]. On the theory side, however, we are still far away from a con- vincing, overall picture to explain all the measurements. The popular models on the market include charmonium [10], D∗0 ¯D0/D 0 ¯D∗0 molecule [11]...

  2. [2]

    The definition of θ depends on the choice of co- ordinate frame

    takes the values 0 , ± 1 if the J/ψ is unpolarized and totally transversely or longitudinally polarized, respec- tively. The definition of θ depends on the choice of co- ordinate frame. The helicity (HX) frame, in which the polar axis is chosen to point along the J/ψ flight di- rection in the center-of-mass (c.m.) frame of the col- lision, and the Collins-S...

  3. [3]

    1491 GeV from Ref

    1396 GeV, and the total decay width Γ ρ = 0. 1491 GeV from Ref. [9], using the functional form BW ρ(p2 ρ) = (p2 ρ − m2 ρ +iΓρ √ p2 ρ − 4m2 π)− 1, and integrating out the π +π − phase space numerically, we find the X(3872) de- cay distribution, WX (θ), to have the same form as in Eq. (2), with θ now being the polar angle of the J/ψ flight direction in the X(...

  4. [4]

    12g2)/ (13. 7 + 30. 6g + 18. 2g2). Finally, we determine g by fitting to the distributions of the X(3872) → J/ψπ +π − partial decay width in the π +π − invariant mass mππ , normalized to unity, as measured by CMS

  5. [5]

    5<m ππ < 0

    in the range 0 . 5<m ππ < 0. 78 GeV and by ATLAS

  6. [6]

    28 < mππ < 0

    in the range 0 . 28 < mππ < 0. 79 GeV. We thus ob- tain g = − 0. 51 ± 0. 10 with χ 2/ d. o. f. = 35. 3/ 22 = 1. 60. The goodness of the fit can also be judged from Fig. 1, which also contains the predictions evaluated with ei- ther A1 µ or A2 µ alone. The latter results are somewhat worse, yielding χ 2/ d. o. f. values of 45 . 9/ 23 = 2 . 00 and

  7. [7]

    48, respectively

    0/ 23 = 3 . 48, respectively. Other realistic functional forms of BW ρ(p2 ρ) yield very similar results, albeit with slightly larger χ 2/ d. o. f. values. Inserting our fit result for g in Eq. (5) and setting in turn σ X 00 = 0 and σ X 11 = 0, we obtain the allowed corridor − 0. 066 ≤ λ X θ ≤ 0. 141, where the lower bound f/ (2− f ), upper bound −f , and 0...

  8. [8]

    The yellow bands indicate the theoretical uncertainties

    (right panel) are compared with our NLO NRQCD results based on the new fit (solid lines). The yellow bands indicate the theoretical uncertainties. NRQCD scales to be µ r = µ f = ξmT and µ Λ = ηmc, respectively, where mT = √ p2 T + 4m2 c is the transverse mass, and independently vary ξ and η by a factor of 2 up and down about their default values ξ = η = 1 ...

  9. [9]

    Choi et al

    S.-K. Choi et al. (Belle Collaboration), Phys. Rev. Lett. 91, 262001 (2003)

  10. [10]

    Acosta et al

    D. Acosta et al. (CDF II Collaboration), Phys. Rev. Lett. 93, 072001 (2004)

  11. [11]

    V. M. Abazov et al. (D0 Collaboration), Phys. Rev. Lett. 93, 162002 (2004)

  12. [12]

    Aubert et al

    B. Aubert et al. (BABAR Collaboration), Phys. Rev. D 71, 071103 (2005)

  13. [13]

    S. L. Olsen, T. Skwarnicki, and D. Zieminska, Rev. Mod. Phys. 90, 015003 (2018)

  14. [14]

    Esposito, A

    A. Esposito, A. Pilloni, and A. D. Polosa, Phys. Rept. 668, 1 (2017)

  15. [15]

    Abulencia et al

    A. Abulencia et al. (CDF Collaboration), Phys. Rev. Lett. 96, 102002 (2006)

  16. [16]

    Aaij et al

    R. Aaij et al. (LHCb Collaboration), Phys. Rev. Lett. 110, 222001 (2013)

  17. [17]

    Tanabashi et al

    M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, 030001 (2018)

  18. [18]

    Barnes and S

    T. Barnes and S. Godfrey, Phys. Rev. D 69, 054008 (2004); E. J. Eichten, K. Lane, and C. Quigg, ibid. 69, 094019 (2004); M. Suzuki, ibid. 72, 114013 (2005)

  19. [19]

    F. E. Close and P. R. Page, Phys. Lett. B 578, 119 (2004); E. Braaten and M. Kusunoki, Phys. Rev. D 69, 074005 (2004); E. S. Swanson, Phys. Lett. B 588, 189 (2004); N. A. T¨ ornqvist,ibid. 590, 209 (2004)

  20. [20]

    Maiani, F

    L. Maiani, F. Piccinini, A. D. Polosa, and V. Riquer, Phys. Rev. D 71, 014028 (2005)

  21. [21]

    B. A. Li, Phys. Lett. B 605, 306 (2005)

  22. [22]

    H.-X. Chen, W. Chen, X. Liu, and S.-L. Zhu, Phys. Rept. 639, 1 (2016); R. F. Lebed, R. E. Mitchell, and E. S. Swanson, Prog. Part. Nucl. Phys. 93, 143 (2017); F.-K. Guo, C. Hanhart, U.-G. Meißner, Q. Wang, Q. Zhao, and B.-S. Zou, Rev. Mod. Phys. 90, 015004 (2018); A. Ali, J. S. Lange, and S. Stone, Prog. Part. Nucl. Phys. 97, 123 (2017)

  23. [23]

    Bauer et al

    G. Bauer et al. (CDF II Collaboration), Int. J. Mod. Phys. A 20, 3765 (2005)

  24. [24]

    Aaij et al

    R. Aaij et al. (LHCb Collaboration), Eur. Phys. J. C 72, 1972 (2012)

  25. [25]

    Chatrchyan et al

    S. Chatrchyan et al. (CMS Collaboration), J. High En- ergy Phys. 04 (2013) 154

  26. [26]

    Aaboud et al

    M. Aaboud et al. (ATLAS Collaboration), J. High En- ergy Phys. 01 (2017) 117

  27. [27]

    Butenschoen, Z

    M. Butenschoen, Z. G. He, and B. A. Kniehl, Phys. Rev. 6 D 88, 011501(R) (2013)

  28. [28]

    G. T. Bodwin, E. Braaten, and G. P. Lepage, Phys. Rev. D 51, 1125 (1995); 55, 5853(E) (1997)

  29. [29]

    Meng, Y.-J

    C. Meng, Y.-J. Gao, and K.-T. Chao, Phys. Rev. D 87, 074035 (2013); C. Meng, H. Han, and K.-T. Chao, ibid. 96, 074014 (2017)

  30. [30]

    Artoisenet and E

    P. Artoisenet and E. Braaten, Phys. Rev. D 81, 114018 (2010)

  31. [31]

    Bignamini, B

    C. Bignamini, B. Grinstein, F. Piccinini, A. D. Polosa, and C. Sabelli, Phys. Rev. Lett. 103, 162001 (2009)

  32. [32]

    Albaladejo, F.-K

    M. Albaladejo, F.-K. Guo, C. Hanhart, U.-G. Meißner, J. Nieves, A. Nogga, and Z. Yang, Chin. Phys. C 41, 121001 (2017)

  33. [33]

    Wang, Chin

    W. Wang, Chin. Phys. C 42, 043103 (2018); A. Espos- ito, B. Grinstein, L. Maiani, F. Piccinini, A. Pilloni, A. D. Polosa, and V. Riquer, ibid. 42, 114107 (2018)

  34. [34]

    Braaten, L.-P

    E. Braaten, L.-P. He, and K. Ingles, arXiv:1811.08876 [hep-ph]

  35. [35]

    Butenschoen and B

    M. Butenschoen and B. A. Kniehl, Phys. Rev. Lett. 108, 172002 (2012)

  36. [36]

    Gong, L.-P

    B. Gong, L.-P. Wan, J.-X. Wang, and H.-F. Zhang, Phys. Rev. Lett. 110, 042002 (2013); J. X. Wang and H. F. Zhang, J. Phys. G 42, 025004 (2015); H.-F. Zhang, L. Yu, S.-X. Zhang, and L. Jia, Phys. Rev. D 93, 054033 (2016); 93, 079901(E) (2016); Y. Feng, B. Gong, C.- H. Chang, and J.-X. Wang, ibid. 99, 014044 (2019)

  37. [37]

    Butenschoen, Z.-G

    M. Butenschoen, Z.-G. He, and B. A. Kniehl, Phys. Rev. Lett. 114, 092004 (2015)

  38. [38]

    Ma, J.-W

    Y.-Q. Ma, J.-W. Qiu, G. Sterman, and H. Zhang, Phys. Rev. Lett. 113, 142002 (2014)

  39. [39]

    Butensch¨ on and B

    M. Butensch¨ on and B. A. Kniehl, Phys. Rev. Lett. 106, 022003 (2011)

  40. [40]

    Chao, Y.-Q

    K.-T. Chao, Y.-Q. Ma, H.-S. Shao, K. Wang, and Y.- J. Zhang, Phys. Rev. Lett. 108, 242004 (2012); H.- S. Shao, H. Han, Y.-Q. Ma, C. Meng, Y.-J. Zhang, and K.-T. Chao, J. High Energy Phys. HEP 05 (2015) 103

  41. [41]

    G. T. Bodwin, H. S. Chung, U-R. Kim, and J. Lee, Phys. Rev. Lett. 113, 022001 (2014); G. T. Bodwin, K.- T. Chao, H. S. Chung, U-R. Kim, J. Lee, and Y.-Q. Ma, Phys. Rev. D 93, 034041 (2016)

  42. [42]

    He and B

    Z.-G. He and B. A. Kniehl, Phys. Rev. D 92, 014009 (2015)

  43. [43]

    Shao, Y.-Q

    H.-S. Shao, Y.-Q. Ma, K. Wang, and K.-T. Chao, Phys. Rev. Lett. 112, 182003 (2014)

  44. [44]

    C. S. Lam and W.-K. Tung, Phys. Rev. D 18, 2447 (1978)

  45. [45]

    J. C. Collins and D. E. Soper, Phys. Rev. D 16, 2219 (1977)

  46. [46]

    Braaten and M

    E. Braaten and M. Kusunoki, Phys. Rev. D 72, 054022 (2005)

  47. [47]

    Pumplin, D

    J. Pumplin, D. R. Stump, J. Huston, H.-L. Lai, P. Nadol- sky, and W.-K. Tung, J. High Energy Phys. 07 (2002) 012

  48. [48]

    Y.-Q. Ma, K. Wang, and K.-T. Chao, Phys. Rev. D 83, 111503(R) (2011)

  49. [49]

    Albrecht et al

    H. Albrecht et al. (ARGUS Collaboration), Phys. Rept. 276, 224 (1996)

  50. [50]

    Chatrchyan et al

    S. Chatrchyan et al. (CMS Collaboration), Phys. Lett. B 727, 381 (2013)

  51. [51]

    Steerenberg, URL: https://home.cern/news/news/ physics/lhc-report-protons-mission-accomplished

    R. Steerenberg, URL: https://home.cern/news/news/ physics/lhc-report-protons-mission-accomplished

  52. [52]

    Aaij et al

    R. Aaij et al. (LHCb Collaboration), Eur. Phys. J. C 72, 2100 (2012); 74, 2872 (2014)