Introduction. Fully charm tetraquarks provide a rare opportunity to study how QCD binds four quarks within a nonrelativistic framework. Their heavy constituents permit an expansion in the relative velocity, while the absence of valence light quarks limits the role of light-meson exchange [1 , 2 , 3 ] . These features make their spectrum a test of short-distance color interactions and nonperturbative four-quark binding.
The LHCb Collaboration first observed a pronounced structure near 6.9 GeV in the di-J / ψ J/\psi J / ψ spectrum [4 ] . ATLAS and CMS later confirmed the X ( 6900 ) X(6900) X ( 6900 ) and reported additional structures near 6.6 and 7.1 GeV [5 , 6 ] . An NRQCD study of hadroproduction had previously suggested spin 2 for the observed di-J / ψ J/\psi J / ψ resonances [7 ] . Recent CMS analyses favor a common J P C = 2 + + J^{PC}=2^{++} J P C = 2 ++ assignment for the X ( 6600 ) X(6600) X ( 6600 ) , X ( 6900 ) X(6900) X ( 6900 ) , and X ( 7100 ) X(7100) X ( 7100 ) [8 , 9 ] . This assignment supports their interpretation as radial excitations [10 , 11 ] , but leaves their microscopic origin unsettled. Compact tetraquarks, hadronic molecules, and threshold effects can produce similar spectra [12 , 13 , 14 , 15 , 16 , 17 , 18 , 19 ] . Discriminating among these possibilities requires complementary decay observables.
For the observed structures above the di-J / ψ J/\psi J / ψ threshold, radiative decays into a photon and charmonium offer complementary information on their nature. The radiative process proceeds through short-distance c c ˉ c\bar c c c ˉ annihilation and probes the quark contact density [20 , 21 ] , while the di-J / ψ J/\psi J / ψ spectrum can also be affected by threshold effects and rescattering [19 ] . In NRQCD, the contact densities appear as long-distance matrix elements (LDMEs) of definite color-spin configurations, factorized from perturbative short-distance coefficients [22 ] . Together with the di-J / ψ J/\psi J / ψ channel, radiative decays can also help constrain the spin and nature of the observed structures. Radiative width ratios have already been used to probe the nature of χ c 1 ( 3872 ) \chi_{c1}(3872) χ c 1 ( 3872 ) [21 , 23 , 24 ] . The radiative-to-di-J / ψ J/\psi J / ψ yield ratio provides a spin-sensitive constraint, while compatible pole positions extracted from both amplitudes would test a common resonance interpretation against a threshold enhancement [19 ] .
Radiative decays also provide search channels for states below their lowest double-charmonium strong-decay thresholds. Beyond the observed 2 + + 2^{++} 2 ++ states, the 0 + + 0^{++} 0 ++ and 1 + − 1^{+-} 1 +− sectors remain unestablished. A recent lattice calculation [25 ] puts the 0 + 0^+ 0 + and 1 + 1^+ 1 + levels 33.2(13) and 10.9(14) MeV below the η c η c \eta_c\eta_c η c η c and η c J / ψ \eta_cJ/\psi η c J / ψ thresholds, respectively. If these levels lie below their corresponding thresholds, the strong decays are kinematically closed. The 0 + 0^+ 0 + state could then decay only electromagnetically or weakly, with γ J / ψ \gamma J/\psi γ J / ψ expected to dominate over the diphoton channel by orders of magnitude [26 , 27 ] . The corresponding radiative search channel for the 1 + − 1^{+-} 1 +− state is η c \eta_c η c ; charge-conjugation parity forbids interchanging the two charmonia in these channels.
The γ J / ψ \gamma J/\psi γ J / ψ and γ η c \gamma\eta_c γ η c widths have so far been calculated only at LO [28 ] . A complete one-loop calculation tests NRQCD factorization and calibrates the relation between radiative widths and tetraquark LDMEs. This is important at the charm scale, where NLO corrections to quarkonium annihilation and fully heavy tetraquark electromagnetic decays can reach tens of percent or order unity [27 , 29 , 30 , 31 ] . The 0 + + 0^{++} 0 ++ channel involves two S S S -wave color-spin operators and their interference, so its NLO hard coefficient is a 2 × 2 2\times2 2 × 2 matrix, whereas the 2 + + 2^{++} 2 ++ and 1 + − 1^{+-} 1 +− channels each have a single leading-v v v operator. A common NLO normalization would preserve the LO color-spin hierarchy, whereas a nonuniform correction would change the relative weights and make the radiative width sensitive to the initial color-spin composition.
In this Letter, we present the first complete NLO QCD calculation of T 4 c ( 0 + + , 2 + + ) → γ J / ψ T_{4c}(0^{++},2^{++})\to\gamma J/\psi T 4 c ( 0 ++ , 2 ++ ) → γ J / ψ and T 4 c ( 1 + − ) → γ η c T_{4c}(1^{+-})\to\gamma\eta_c T 4 c ( 1 +− ) → γ η c at leading order in the relative velocity. We determine the short-distance coefficients for all relevant color-spin operators, including scalar interference, and predict the tensor J / ψ J/\psi J / ψ polarization and dilepton angular distribution without an overall LDME normalization. For a spin-resolved tensor state, we show how the ratio of its γ J / ψ \gamma J/\psi γ J / ψ and di-J / ψ J/\psi J / ψ yields, combined with an inclusive-production fit and the total width, can constrain its LDME without a potential-model input. This extraction requires compatible production and decay normalizations. If scalar and tensor signals are unresolved, the same yield ratio can instead constrain their relative contributions, provided their respective radiative-to-hadronic decay ratios are known. We discuss these inputs and assumptions below.
NRQCD factorization and matching
The decays T 4 c ( 0 + + , 2 + + ) → γ J / ψ T_{4c}(0^{++},2^{++}) \to\gamma J/\psi T 4 c ( 0 ++ , 2 ++ ) → γ J / ψ and T 4 c ( 1 + − ) → γ η c T_{4c}(1^{+-}) \to\gamma\eta_c T 4 c ( 1 +− ) → γ η c are treated in NRQCD at leading order in the heavy-quark relative velocity v v v [22 , 28 ] . The J / ψ J/\psi J / ψ and η c \eta_c η c are projected onto the color-singlet 3 S 1 {}^{3}S_{1} 3 S 1 and 1 S 0 {}^{1}S_{0} 1 S 0 states, respectively. Their decay widths can be written as
Γ J = 12 π 4 e c 2 α α s 4 ( μ R ) m c 11 ρ H [ R J ( 0 ) + 4 π α s ( μ R ) R J ( 1 ) ( μ R / m c ) ] , (1) \Gamma_J = \frac{12\pi^4 e_c^2 \alpha\alpha_s^4(\mu_R)}{m_c^{11}} \rho_H \left[R_J^{(0)} + 4\pi\alpha_s(\mu_R) R_J^{(1)}(\mu_R/m_c)\right], \tag*{(1)} Γ J = m c 11 12 π 4 e c 2 α α s 4 ( μ R ) ρ H [ R J ( 0 ) + 4 π α s ( μ R ) R J ( 1 ) ( μ R / m c ) ] , (1)
R J ( i ) = Tr [ h J ( i ) ρ T , J ] . R_J^{(i)} = \operatorname{Tr}\left[h_J^{(i)}\rho_{T,J}\right]. R J ( i ) = Tr [ h J ( i ) ρ T , J ] .
Here ρ H = ⟨ O 1 J / ψ ( 3 S 1 ) ⟩ \rho_H = \langle O_1^{J/\psi}({}^{3}S_1)\rangle ρ H = ⟨ O 1 J / ψ ( 3 S 1 )⟩ for J = 0 , 2 J=0,2 J = 0 , 2 and ρ H = ⟨ O 1 η c ( 1 S 0 ) ⟩ \rho_H = \langle O_1^{\eta_c}({}^{1}S_0)\rangle ρ H = ⟨ O 1 η c ( 1 S 0 )⟩ for J = 1 J=1 J = 1 . The matrices h J ( i ) h_J^{(i)} h J ( i ) and ρ T , J \rho_{T,J} ρ T , J are the hard coefficients and tetraquark LDMEs. The NLO matrices h J ( 1 ) h_J^{(1)} h J ( 1 ) follow from Born–one-loop interference in each color-spin channel.
For identical charm quarks, Pauli statistics restrict the allowed S S S -wave color-spin bases to
B 0 + + = { [ ( c c ) 3 ˉ ( 3 S 1 ) ( c ˉ c ˉ ) 3 ( 3 S 1 ) ] 0 , [ ( c c ) 6 ( 1 S 0 ) ( c ˉ c ˉ ) 6 ˉ ( 1 S 0 ) ] 0 } , \mathcal{B}_{0^{++}} = \left\{\left[(cc)_{\bar{3}}({}^{3}S_1)(\bar{c}\bar{c})_{3}({}^{3}S_1)\right]_0,\left[(cc)_{6}({}^{1}S_0)(\bar{c}\bar{c})_{\bar{6}}({}^{1}S_0)\right]_0\right\}, B 0 ++ = { [ ( cc ) 3 ˉ ( 3 S 1 ) ( c ˉ c ˉ ) 3 ( 3 S 1 ) ] 0 , [ ( cc ) 6 ( 1 S 0 ) ( c ˉ c ˉ ) 6 ˉ ( 1 S 0 ) ] 0 } ,
B 1 + − , 2 + + = { [ ( c c ) 3 ˉ ( 3 S 1 ) ( c ˉ c ˉ ) 3 ( 3 S 1 ) ] 1 , 2 } . (2) \mathcal{B}_{1^{+-},2^{++}} = \left\{\left[(cc)_{\bar{3}}({}^{3}S_1)(\bar{c}\bar{c})_{3}({}^{3}S_1)\right]_{1,2}\right\}. \tag*{(2)} B 1 +− , 2 ++ = { [ ( cc ) 3 ˉ ( 3 S 1 ) ( c ˉ c ˉ ) 3 ( 3 S 1 ) ] 1 , 2 } . (2)
For each operator Q n Q_n Q n , we define L n = ⟨ 0 ∣ Q n r e n ∣ T ⟩ L_n = \langle0|Q_n^{\mathrm{ren}}|T\rangle L n = ⟨ 0∣ Q n ren ∣ T ⟩ and ( ρ T ) n m = L n L m ∗ (\rho_T)_{nm} = L_n L_m^* ( ρ T ) nm = L n L m ∗ . The scalar hard coefficient and LDME are therefore 2 × 2 2 \times2 2 × 2 matrices. Their off-diagonal entries describe interference between the two color-spin amplitudes. The transpose in Eq. (1) follows from ∣ ∑ n F n L n ∣ 2 \left|\sum_n F_nL_n\right|^2 ∣ ∑ n F n L n ∣ 2 and is retained for complex LDMEs. The axial and tensor channels each contain one leading-v v v operator. The tensor amplitude nevertheless has three physical polarization components, whose spin-averaged contraction gives a single hard coefficient. Reduced nonrelativistic state normalization is used throughout. State-conversion factors and initial-spin averages are included once in Eq. (1) .
The hard coefficients are determined by matching renormalized QCD amplitudes onto NRQCD with on-shell partonic states. The matching is performed at P T = P H + k P_T=P_H+k P T = P H + k , with P T 2 = ( 4 m c ) 2 P_T^2=(4m_c)^2 P T 2 = ( 4 m c ) 2 , P H 2 = ( 2 m c ) 2 P_H^2=(2m_c)^2 P H 2 = ( 2 m c ) 2 , and k 2 = 0 k^2=0 k 2 = 0 . The potential-region contribution is isolated at finite relative velocity and subtracted before the zero-relative-momentum limit is taken [32 ] . Dimensional regularization with D = 4 − 2 ϵ D=4-2\epsilon D = 4 − 2 ϵ is used in both theories. The charm-quark mass and field are renormalized in the on-shell scheme, while α s \alpha_s α s is renormalized in the M S ‾ \overline{\mathrm{MS}} MS scheme with n f = 4 n_f=4 n f = 4 . The nonpotential NRQCD loop contribution vanishes in pure dimensional regularization. Since
T 4 c → γ H g T_{4c} \to\gamma H_g T 4 c → γ H g vanishes by color conservation, the NLO correction is purely virtual. The BMHV prescription is adopted for γ 5 \gamma_5 γ 5 in the axial channel [33 , 34 ] .
We calculate the on-shell partonic amplitude c c c ˉ c ˉ → c c ˉ + γ c c\bar{c}\bar{c} \to c\bar{c}+\gamma cc c ˉ c ˉ → c c ˉ + γ and project its external heavy-quark states onto the required color and spin configurations. Representative Born and one-loop diagrams are shown in Figure 1 . At Born level, our implementation also reproduces the short-distance coefficients for T 4 c → γ ψ T_{4c} \to\gamma\psi T 4 c → γ ψ using the same operator conventions [26 ] . The one-loop integrals reduce to 52 common master-integral classes. Their analytic finite combinations agree with independent numerical integral evaluations. The hard coefficients are finite after renormalization and matching. Photon Ward identities are verified before the transverse projection, and the D D D -dimensional spin factors are retained through the Laurent expansion. The logarithmic terms agree with the running of α s 4 \alpha_s^4 α s 4 . The Supplemental Material provides operator conventions, finite amplitudes, matching checks, and numerical prescriptions [35 ] .
Figure 1. Representative Feynman diagrams for c c c ˉ c ˉ → γ c c ˉ c c \bar{c}\bar{c} \to\gamma c\bar{c} cc c ˉ c ˉ → γ c c ˉ at (a) Born and (b) one-loop order.
NLO short-distance coefficients and radiative widths
For N c = 3 N_c=3 N c = 3 and n f = 4 n_f=4 n f = 4 , the hard coefficients are evaluated at the leading-order matching point M T = 4 m c M_T=4m_c M T = 4 m c and M H = 2 m c M_H=2m_c M H = 2 m c . The finite one-loop terms below correspond to μ R = m c \mu_R=m_c μ R = m c . In the ordered scalar basis { 3 ˉ ⊗ 3 , 6 ⊗ 6 ˉ } \{\bar{3}\otimes3,6\otimes\bar{6}\} { 3 ˉ ⊗ 3 , 6 ⊗ 6 ˉ } , the hard matrices are
h 0 ( 0 ) = ( 109.82991 − 13.03692 − 13.03692 1.54750 ) , h_0^{(0)} =
\begin{pmatrix}
109.82991 & -13.03692 \\
-13.03692 & 1.54750
\end{pmatrix}, h 0 ( 0 ) = ( 109.82991 − 13.03692 − 13.03692 1.54750 ) ,
h 0 ( 1 ) = ( 26.92184 4.32217 − 1.02746 i 4.32217 + 1.02746 i − 1.40542 ) . (3) h_0^{(1)} =
\begin{pmatrix}
26.92184 & 4.32217-1.02746i \\
4.32217+1.02746i & -1.40542
\end{pmatrix}. \tag*{(3)} h 0 ( 1 ) = ( 26.92184 4.32217 + 1.02746 i 4.32217 − 1.02746 i − 1.40542 ) . (3)
The off-diagonal elements should be retained because they would contribute through ρ 36 \rho_{36} ρ 36 . More importantly, h 0 ( 1 ) h_0^{(1)} h 0 ( 1 ) is not proportional to h 0 ( 0 ) h_0^{(0)} h 0 ( 0 ) . The NLO correction therefore modifies the relative weights of the two color-spin directions and their interference differently. The positive correction to the 3 ˉ ⊗ 3 \bar{3}\otimes3 3 ˉ ⊗ 3 diagonal coefficient and the negative correction to the 6 ⊗ 6 ˉ 6\otimes\bar{6} 6 ⊗ 6 ˉ coefficient make this color dependence explicit.
At μ R = 2 m c \mu_R=2m_c μ R = 2 m c , the pure-sextet correction is Δ Γ / Γ ( 0 ) = − 1.93 \Delta\Gamma/\Gamma^{(0)}=-1.93 ΔΓ/ Γ ( 0 ) = − 1.93 , giving a negative truncated width. The fixed-order expansion is therefore not uniformly controlled across scalar color configurations.
For the one-operator tensor and axial channels, the corresponding coefficients are
( h 2 ( 0 ) , h 2 ( 1 ) ( 1 ) ) = ( 10.30795 , 3.73544 ) , \left(h_2^{(0)},h_2^{(1)}(1)\right)=(10.30795,3.73544), ( h 2 ( 0 ) , h 2 ( 1 ) ( 1 ) ) = ( 10.30795 , 3.73544 ) ,
( h 1 ( 0 ) , h 1 ( 1 ) ( 1 ) ) = ( 132.42274 , 48.34858 ) , (4) \left(h_1^{(0)},h_1^{(1)}(1)\right)=(132.42274,48.34858), \tag*{(4)} ( h 1 ( 0 ) , h 1 ( 1 ) ( 1 ) ) = ( 132.42274 , 48.34858 ) , (4)
where no leading-v v v color mixing occurs. Their tetraquark LDMEs therefore set the overall widths but cancel in the NLO-to-LO ratios.
The hard coefficients at a general renormalization scale are obtained from
h J ( 1 ) ( r ) = h J ( 1 ) ( 1 ) + β 0 2 π 2 ln r h J ( 0 ) , r = μ R m c , (5) h_J^{(1)}(r)=h_J^{(1)}(1)+\frac{\beta_0}{2\pi^2}\ln r\,h_J^{(0)},\qquad r=\frac{\mu_R}{m_c}, \tag*{(5)} h J ( 1 ) ( r ) = h J ( 1 ) ( 1 ) + 2 π 2 β 0 ln r h J ( 0 ) , r = m c μ R , (5)
where β 0 = ( 11 N c − 2 n f ) / 3 = 25 / 3 \beta_0=(11N_c-2n_f)/3=25/3 β 0 = ( 11 N c − 2 n f ) /3 = 25/3 . The central widths are evaluated at μ R = 2 m c \mu_R=2m_c μ R = 2 m c using h J ( 1 ) ( 2 ) h_J^{(1)}(2) h J ( 1 ) ( 2 ) . For the numerical analysis, we take
m c = 1.5 G e V , e c = 2 3 , α = 1 137.065 , α s ( 2 m c ) = 0.249. (6) m_c=1.5\ \mathrm{GeV},\ e_c=\frac{2}{3},\ \alpha=\frac{1}{137.065},\ \alpha_s(2m_c)=0.249. \tag*{(6)} m c = 1.5 GeV , e c = 3 2 , α = 137.065 1 , α s ( 2 m c ) = 0.249. (6)
These inputs give M T = 6.0 G e V M_T=6.0\ \mathrm{GeV} M T = 6.0 GeV and M H = 3.0 G e V M_H=3.0\ \mathrm{GeV} M H = 3.0 GeV at the leading-v v v matching point. Physical hadron masses differ by binding and relative-velocity effects. The production-based illustration below uses a separate mass and scale prescription.
The charmonium LDMEs are ρ J / ψ = 1.32 G e V 3 \rho_{J/\psi}=1.32\ \mathrm{GeV}^3 ρ J / ψ = 1.32 GeV 3 and ρ η c = 0.44 G e V 3 \rho_{\eta_c}=0.44\ \mathrm{GeV}^3 ρ η c = 0.44 GeV 3 . The tetraquark LDMEs are taken from Refs. [2 , 28 ] and listed in Table I . Table II gives the widths from Eq. (1) , their scale variations and charm-mass sensitivities, and K J = Γ J N L O / Γ J L O K_J=\Gamma_J^{\mathrm{NLO}}/\Gamma_J^{\mathrm{LO}} K J = Γ J NLO / Γ J LO .
Table I. Tetraquark LDME inputs in G e V 9 \mathrm{GeV}^9 GeV 9 . The scalar entries are ordered as ( ρ 33 , ρ 36 , ρ 66 ) (\rho_{33},\rho_{36},\rho_{66}) ( ρ 33 , ρ 36 , ρ 66 ) .
Table II. Radiative widths in MeV with separate scale and mass scans over m c ≤ μ R ≤ 4 m c m_c\leq\mu_R\leq4m_c m c ≤ μ R ≤ 4 m c at the central mass and m c = 1.5 ± 0.1 G e V m_c=1.5\pm0.1\ \mathrm{GeV} m c = 1.5 ± 0.1 GeV at μ R = 2 m c \mu_R=2m_c μ R = 2 m c . Central widths and K K K factors at μ R = 2 m c \mu_R=2m_c μ R = 2 m c are rounded to two significant figures. Scan shifts are rounded sensitivities, not statistical errors.
At the central scale, the NLO widths in Table II are 2.3–3.1 times the LO widths. For scalar and axial levels predicted below their respective lowest dicharmonium thresholds [25 ] , radiative annihilation offers alternative search channels. We provide the corresponding NLO short-distance coefficients. Sensitivity to η c \eta_c η c remains limited by η c \eta_c η c reconstruction: the useful hadronic branching fractions are at the few-percent level and the broad 32 MeV η c \eta_c η c width degrades the mass resolution. A quantitative assessment requires production rates, total widths, reconstruction efficiencies, backgrounds, and mass resolution.
Table II also shows pronounced charm-mass and scale dependences, characteristic of slow perturbative convergence at the charm scale [29 , 30 , 31 , 36 ] . At m c = 1.4 ( 1.6 ) G e V m_c=1.4\ (1.6)\ \mathrm{GeV} m c = 1.4 ( 1.6 ) GeV , all NLO widths are approximately 2.41 (0.44) times their central values. The common m c − 11 m_c^{-11} m c − 11 factor and running of α s ( 2 m c ) \alpha_s(2m_c) α s ( 2 m c ) dominate the mass sensitivity, while α s 4 ( μ R ) \alpha_s^4(\mu_R) α s 4 ( μ R ) and the LO-proportional logarithm govern scale variation. These predominantly common normalization changes do not discriminate color-spin configurations.
Figure 2 shows that the widths decrease monotonically with μ R \mu_R μ R , with milder slopes at larger scales as the running of α s \alpha_s α s weakens. Over the scale scan, the ratio of the LO widths at the two endpoints is about 8.3 and decreases to 6.1–6.3 at NLO, or 4.7 for scalar Model II. The NLO correction therefore improves the scale stability, although substantial residual dependence remains. Further stabilization may be possible with the optimized NRQCD strategy for exclusive double-J / ψ J/\psi J / ψ production, which separates photon-fragmentation and nonfragmentation amplitudes and resums radiative and relativistic corrections with the measured J / ψ J/\psi J / ψ decay constant [37 ] .
Figure 2. Renormalization-scale dependence at m c = 1.5 G e V m_c=1.5\ \mathrm{GeV} m c = 1.5 GeV with fixed central LDMEs. (a–c) Scalar, tensor, and axial radiative widths. Navy and rose denote Models I and II, and dashed and solid lines denote LO and NLO. (d) K = Γ N L O / Γ L O K=\Gamma_{\mathrm{NLO}}/\Gamma_{\mathrm{LO}} K = Γ NLO / Γ LO . The tensor and axial K K K factors are model independent and nearly coincide. Dotted vertical lines mark μ R = 2 m c \mu_R=2m_c μ R = 2 m c .
The K K K factors in Table II and Figure 2 reveal a channel-dependent pattern. In the 2 + + 2^{++} 2 ++ and 1 + − 1^{+-} 1 +− channels, the Model I and Model II K K K factors coincide because the single leading-v v v LDME cancels in Γ N L O / Γ L O \Gamma_{\mathrm{NLO}}/\Gamma_{\mathrm{LO}} Γ NLO / Γ LO , whereas the scalar K K K factors remain distinct because the two color components and their interference receive different NLO corrections.
Tensor polarization. The tensor amplitude provides an observable independent of the overall LDME normalization: the longitudinal fraction f L = Γ L / Γ f_L = \Gamma_L/\Gamma f L = Γ L /Γ of the daughter J / ψ J/\psi J / ψ . In a physical three-component basis, the longitudinal and transverse polarization metrics are G L = diag ( 0 , 0 , 2 / 5 ) G_L = \operatorname{diag}(0,0,2/5) G L = diag ( 0 , 0 , 2/5 ) and G T = diag ( 4 / 5 , 2 / 5 , 0 ) G_T = \operatorname{diag}(4/5,2/5,0) G T = diag ( 4/5 , 2/5 , 0 ) . The common tetraquark and charmonium LDMEs, phase space, and m − 11 m^{-11} m − 11 factor cancel in the fraction. Writing Γ = Γ ( 0 ) + Δ Γ \Gamma= \Gamma^{(0)}+\Delta\Gamma Γ = Γ ( 0 ) + ΔΓ and similarly for Γ L \Gamma_L Γ L , the strictly expanded NLO result is
f L N L O = f L ( 0 ) + Δ Γ L − f L ( 0 ) Δ Γ Γ ( 0 ) , f L ( 0 ) = Γ L ( 0 ) Γ ( 0 ) . (7) f_L^{\mathrm{NLO}} = f_L^{(0)} + \frac{\Delta\Gamma_L - f_L^{(0)}\Delta\Gamma}{\Gamma^{(0)}}, \qquad f_L^{(0)} = \frac{\Gamma_L^{(0)}}{\Gamma^{(0)}}. \tag*{(7)} f L NLO = f L ( 0 ) + Γ ( 0 ) Δ Γ L − f L ( 0 ) ΔΓ , f L ( 0 ) = Γ ( 0 ) Γ L ( 0 ) . (7)
At μ R = 2 m c \mu_R = 2m_c μ R = 2 m c , we obtain f L ( 0 ) = 0.11 f_L^{(0)} = 0.11 f L ( 0 ) = 0.11 and f L N L O = 0.18 f_L^{\mathrm{NLO}} = 0.18 f L NLO = 0.18 . The unexpanded quotient ( Γ L ( 0 ) + Δ Γ L ) / ( Γ ( 0 ) + Δ Γ ) (\Gamma_L^{(0)}+\Delta\Gamma_L)/(\Gamma^{(0)}+\Delta\Gamma) ( Γ L ( 0 ) + Δ Γ L ) / ( Γ ( 0 ) + ΔΓ ) instead gives 0.14 0.14 0.14 . The two prescriptions agree through NLO, but differ by 0.047 0.047 0.047 at the central scale because Δ Γ / Γ ( 0 ) ≃ 2.05 \Delta\Gamma/\Gamma^{(0)} \simeq2.05 ΔΓ/ Γ ( 0 ) ≃ 2.05 . This difference diagnoses higher-order sensitivity. It does not bound the unknown higher-order terms.
In Figure 3 (a), the LO fraction is scale independent. The expanded NLO curve remains above the quotient throughout m c ≤ μ R ≤ 4 m c m_c \le\mu_R \le4m_c m c ≤ μ R ≤ 4 m c . Their central separation exceeds either curve’s change to a scale endpoint, so scale variation alone misses this higher-order sensitivity. The universal renormalization logarithm cancels in f L f_L f L , whose remaining NLO scale dependence enters through α s \alpha_s α s .
Figure 3. Polarization in T 4 c ( 2 + + ) → γ J / ψ T_{4c}(2^{++}) \to\gamma J/\psi T 4 c ( 2 ++ ) → γ J / ψ . (a) Longitudinal fraction versus renormalization scale. (b) Normalized dilepton distribution at μ R = 2 m c \mu_R = 2m_c μ R = 2 m c . The curves show tensor LO, strictly NLO (NLO exp.), and the quotient of NLO widths (quot.). The scalar reference appears only in (b). The two NLO prescriptions illustrate higher-order sensitivity.
The polarization fraction can be accessed through J / ψ → ℓ + ℓ − J/\psi\to\ell^+\ell^- J / ψ → ℓ + ℓ − . Let θ \theta θ be the angle of ℓ + \ell^+ ℓ + in the J / ψ J/\psi J / ψ rest frame relative to the J / ψ J/\psi J / ψ direction in the tetraquark rest frame. After integration over the lepton azimuth, the normalized distribution is [38 ]
W ( z ) ≡ 1 Γ ℓ ℓ d Γ ℓ ℓ d z = 3 8 [ ( 1 + f L ) + ( 1 − 3 f L ) z 2 ] , z = cos θ . (8) W(z) \equiv\frac{1}{\Gamma_{\ell\ell}}\frac{\mathrm{d}\Gamma_{\ell\ell}}{\mathrm{d}z} = \frac{3}{8}\left[(1+f_L)+(1-3f_L)z^2\right], \qquad z=\cos\theta. \tag*{(8)} W ( z ) ≡ Γ ℓℓ 1 d z d Γ ℓℓ = 8 3 [ ( 1 + f L ) + ( 1 − 3 f L ) z 2 ] , z = cos θ . (8)
Here Γ ℓ ℓ \Gamma_{\ell\ell} Γ ℓℓ denotes the cascade rate for T 4 c → γ J / ψ → γ ℓ + ℓ − T_{4c} \to\gamma J/\psi\to\gamma\ell^+\ell^- T 4 c → γ J / ψ → γ ℓ + ℓ − . For a scalar parent and a real photon, angular momentum conservation requires f L = 0 f_L = 0 f L = 0 , independently of the scalar color mixture.
Figure 3 (b) compares the resulting angular shapes at the central scale. The scalar reference, W ( z ) = 3 ( 1 + z 2 ) / 8 W(z) = 3(1+z^2)/8 W ( z ) = 3 ( 1 + z 2 ) /8 , has the strongest rise toward ∣ z ∣ = 1 |z|=1 ∣ z ∣ = 1 . A nonzero tensor f L f_L f L increases the distribution near z = 0 z=0 z = 0 and reduces it near ∣ z ∣ = 1 |z|=1 ∣ z ∣ = 1 , making the tensor shape flatter. The strictly expanded NLO result gives the largest flattening. The quotient prediction lies between it and the tensor LO curve. Thus the angular distribution supplies
spin information without strong-decay inputs, while the separation between the two NLO tensor curves shows the present perturbative limitation of a quantitative comparison. These shapes assume an unpolarized parent, or integration over its complete decay solid angle. A fiducial measurement must correct for polarization-dependent acceptance or fit the parent spin density matrix jointly with the decay angles.
Tensor LDME extraction. Assuming a pure-2 + + 2^{++} 2 ++ state X X X , the radiative width retains its LDME dependence. The radiative yield measures σ X B γ ψ = σ X Γ γ ψ / Γ t o t \sigma_X\mathcal{B}_{\gamma\psi} = \sigma_X\Gamma_{\gamma\psi}/\Gamma_{\mathrm{tot}} σ X B γ ψ = σ X Γ γ ψ / Γ tot . Comparing radiative and di-J / ψ J/\psi J / ψ decays cancels the production normalization,
R γ / ψ ≡ B ( X → γ J / ψ ) B ( X → J / ψ J / ψ ) = Γ ( X → γ J / ψ ) Γ ( X → J / ψ J / ψ ) . (9) R_{\gamma/\psi} \equiv\frac{\mathcal{B}(X\to\gamma J/\psi)}{\mathcal{B}(X\to J/\psi J/\psi)} = \frac{\Gamma(X\to\gamma J/\psi)}{\Gamma(X\to J/\psi J/\psi)}. \tag*{(9)} R γ / ψ ≡ B ( X → J / ψ J / ψ ) B ( X → γ J / ψ ) = Γ ( X → J / ψ J / ψ ) Γ ( X → γ J / ψ ) . (9)
The production cross section, luminosity, and total width cancel in this ratio, but the unknown di-J / ψ J/\psi J / ψ branching fraction prevents extracting ρ T , 2 f i x \rho_{T,2}^{\mathrm{fix}} ρ T , 2 fix from this ratio alone.
The complementary input is provided by the NLO+NLL analysis of inclusive production, p p → T 4 c ( 2 + + ) + X i n c l pp \to T_{4c}(2^{++})+X_{\mathrm{incl}} pp → T 4 c ( 2 ++ ) + X incl [39 ] . The di-J / ψ J/\psi J / ψ data constrain
P 2 f i t = ρ T , 2 p r o d B ψ ψ = 5 ξ ρ T , 2 f i x B ψ ψ , (10) P_2^{\mathrm{fit}} = \rho_{T,2}^{\mathrm{prod}}\mathcal{B}_{\psi\psi} = 5\xi\rho_{T,2}^{\mathrm{fix}}\mathcal{B}_{\psi\psi}, \tag*{(10)} P 2 fit = ρ T , 2 prod B ψ ψ = 5 ξ ρ T , 2 fix B ψ ψ , (10)
P 2 f i t = ( 2.22 ± 0.8 0 − 0.57 + 1.29 − 0.00 + 0.62 ) × 10 − 4 G e V 9 . P_2^{\mathrm{fit}} = (2.22 \pm0.80^{+1.29}_{-0.57}{}^{+0.62}_{-0.00}) \times10^{-4}\ \mathrm{GeV}^{9}. P 2 fit = ( 2.22 ± 0.8 0 − 0.57 + 1.29 − 0.00 + 0.62 ) × 1 0 − 4 GeV 9 .
The three uncertainties arise from experiment, scale variation, and PDFs. Here ρ T , 2 p r o d \rho_{T,2}^{\mathrm{prod}} ρ T , 2 prod denotes the fitted production-convention LDME. At leading order in v v v and under vacuum saturation, 5 ξ 5\xi 5 ξ relates it to the fixed-polarization decay LDME—the factor 5 5 5 sums the 2 J + 1 = 5 2J+1=5 2 J + 1 = 5 tensor polarizations—including operator, state, and polarization conventions. Identical currents and states with a spin-summed production LDME give ξ = 1 \xi=1 ξ = 1 . This identification remains unverified for the external fit. The initial-spin average is already in the decay coefficient. Writing Γ γ ψ = H 2 N L O ρ T , 2 f i x \Gamma_{\gamma\psi}=H_2^{\mathrm{NLO}}\rho_{T,2}^{\mathrm{fix}} Γ γ ψ = H 2 NLO ρ T , 2 fix and Γ ψ ψ = B ψ ψ Γ t o t \Gamma_{\psi\psi}=\mathcal{B}_{\psi\psi}\Gamma_{\mathrm{tot}} Γ ψ ψ = B ψ ψ Γ tot , the two constraints give
ρ T , 2 f i x = P 2 f i t R γ / ψ ψ Γ t o t 5 ξ H 2 N L O . (11) \rho^{\mathrm{fix}}_{T,2}=\sqrt{\frac{P^{\mathrm{fit}}_{2}R_{\gamma/\psi\psi}\Gamma_{\mathrm{tot}}}{5\xi\mathcal{H}^{\mathrm{NLO}}_{2}}}. \tag*{(11)} ρ T , 2 fix = 5 ξ H 2 NLO P 2 fit R γ / ψ ψ Γ tot . (11)
This relation avoids a potential-model tetraquark LDME input. For illustration, match the production mass and central hard scale, M = 6.847 M=6.847 M = 6.847 GeV, m c = M / 4 m_c=M/4 m c = M /4 , and μ R = M \mu_R=M μ R = M (μ F = M \mu_F=M μ F = M for production) [39 ] , together with P 2 f i t = 2.22 × 10 − 4 P^{\mathrm{fit}}_{2}=2.22\times10^{-4} P 2 fit = 2.22 × 1 0 − 4 GeV9 ^9 9 and the CMS interference-fit width Γ t o t = 135 \Gamma_{\mathrm{tot}}=135 Γ tot = 135 MeV [9 ] . Then
ρ T , 2 f i x ≃ 0.099 R γ / ψ ψ / ξ G e V 9 . (12) \rho^{\mathrm{fix}}_{T,2}\simeq0.099\sqrt{R_{\gamma/\psi\psi}/\xi}\ {\rm GeV}^{9}. \tag*{(12)} ρ T , 2 fix ≃ 0.099 R γ / ψ ψ / ξ GeV 9 . (12)
This coefficient uses our stated decay inputs. Their compatibility with the production fit and ξ \xi ξ remain conditions. Without fixing ξ \xi ξ , only the scaled combination ξ ρ T , 2 f i x \sqrt{\xi}\rho^{\mathrm{fix}}_{T,2} ξ ρ T , 2 fix is determined; the quoted CMS width errors propagate to about 8% on ρ T , 2 f i x \rho^{\mathrm{fix}}_{T,2} ρ T , 2 fix through the square root [9 ] . A mixed sample requires spin-resolved yields and a compatible production fit. No complete correlated uncertainty is claimed.
Disentanglement of scalar and tensor contributions. For unresolved 0 + + 0^{++} 0 ++ and 2 + + 2^{++} 2 ++ signals in one mass window, the di-J / ψ J/\psi J / ψ spectrum gives their combined yield. The radiative channel constrains their fractions through distinct radiative-to-hadronic responses.
For the inputs of Table I at m c = 1.5 m_c=1.5 m c = 1.5 GeV and μ R = 2 m c \mu_R=2m_c μ R = 2 m c , γ γ \gamma\gamma γ γ is suppressed by order 10 2 10^2 1 0 2 or more relative to γ J / ψ → γ ℓ + ℓ − \gamma J/\psi\to\gamma\ell^+\ell^- γ J / ψ → γ ℓ + ℓ − , taking B ( J / ψ → ℓ + ℓ − ) ≃ 0.06 \mathcal{B}(J/\psi\to\ell^+\ell^-)\simeq0.06 B ( J / ψ → ℓ + ℓ − ) ≃ 0.06 for either charged lepton [26 , 27 ] . Tensor η c η c \eta_c\eta_c η c η c requires a D D D wave and lacks a reliable width [1 , 40 ] , limiting these alternatives for quantitative spin separation.
Assuming that the resonant yield in the selected mass window is saturated by 0 + + 0^{++} 0 ++ and 2 + + 2^{++} 2 ++ contributions, define the scalar fraction of the di-J / ψ J/\psi J / ψ signal by
f 0 ψ ψ = σ 0 B 0 ( ψ ψ ) σ 0 B 0 ( ψ ψ ) + σ 2 B 2 ( ψ ψ ) , f 2 ψ ψ = 1 − f 0 ψ ψ , (13) f^{\psi\psi}_{0}=\frac{\sigma_{0}\mathcal{B}_{0}(\psi\psi)}{\sigma_{0}\mathcal{B}_{0}(\psi\psi)+\sigma_{2}\mathcal{B}_{2}(\psi\psi)},\qquad f^{\psi\psi}_{2}=1-f^{\psi\psi}_{0}, \tag*{(13)} f 0 ψ ψ = σ 0 B 0 ( ψ ψ ) + σ 2 B 2 ( ψ ψ ) σ 0 B 0 ( ψ ψ ) , f 2 ψ ψ = 1 − f 0 ψ ψ , (13)
where σ J \sigma_J σ J denotes the production cross section in the same fiducial region. For the pure-spin responses r J γ ψ ≡ Γ J ( γ J / ψ ) / Γ J ( J / ψ J / ψ ) r^{\gamma\psi}_{J}\equiv\Gamma_J(\gamma J/\psi)/\Gamma_J(J/\psi J/\psi) r J γ ψ ≡ Γ J ( γ J / ψ ) / Γ J ( J / ψ J / ψ ) , one has B J ( γ J / ψ ) = r J γ ψ B J ( J / ψ J / ψ ) \mathcal{B}_J(\gamma J/\psi)=r^{\gamma\psi}_{J}\mathcal{B}_J(J/\psi J/\psi) B J ( γ J / ψ ) = r J γ ψ B J ( J / ψ J / ψ ) . For this unresolved sample, R γ / ψ ψ R_{\gamma/\psi\psi} R γ / ψ ψ denotes the combined yield ratio,
R γ / ψ ψ = σ 0 B 0 ( γ ψ ) + σ 2 B 2 ( γ ψ ) σ 0 B 0 ( ψ ψ ) + σ 2 B 2 ( ψ ψ ) = r 0 γ ψ f 0 ψ ψ + r 2 γ ψ f 2 ψ ψ = r 2 γ ψ + ( r 0 γ ψ − r 2 γ ψ ) f 0 ψ ψ . (14) \begin{aligned}
R_{\gamma/\psi\psi}
&=\frac{\sigma_{0}\mathcal{B}_{0}(\gamma\psi)+\sigma_{2}\mathcal{B}_{2}(\gamma\psi)}{\sigma_{0}\mathcal{B}_{0}(\psi\psi)+\sigma_{2}\mathcal{B}_{2}(\psi\psi)}\\
&=r^{\gamma\psi}_{0}f^{\psi\psi}_{0}+r^{\gamma\psi}_{2}f^{\psi\psi}_{2}\\
&=r^{\gamma\psi}_{2}+\left(r^{\gamma\psi}_{0}-r^{\gamma\psi}_{2}\right)f^{\psi\psi}_{0}. \tag*{(14)}
\end{aligned} R γ / ψ ψ = σ 0 B 0 ( ψ ψ ) + σ 2 B 2 ( ψ ψ ) σ 0 B 0 ( γ ψ ) + σ 2 B 2 ( γ ψ ) = r 0 γ ψ f 0 ψ ψ + r 2 γ ψ f 2 ψ ψ = r 2 γ ψ + ( r 0 γ ψ − r 2 γ ψ ) f 0 ψ ψ . (14)
If r 0 γ ψ ≠ r 2 γ ψ r^{\gamma\psi}_{0}\ne r^{\gamma\psi}_{2} r 0 γ ψ = r 2 γ ψ , this relation can be inverted directly:
f 0 ψ ψ = R γ / ψ ψ − r 2 γ ψ r 0 γ ψ − r 2 γ ψ , f 2 ψ ψ = 1 − f 0 ψ ψ . (15) f^{\psi\psi}_{0}=\frac{R_{\gamma/\psi\psi}-r^{\gamma\psi}_{2}}{r^{\gamma\psi}_{0}-r^{\gamma\psi}_{2}},\qquad f^{\psi\psi}_{2}=1-f^{\psi\psi}_{0}. \tag*{(15)} f 0 ψ ψ = r 0 γ ψ − r 2 γ ψ R γ / ψ ψ − r 2 γ ψ , f 2 ψ ψ = 1 − f 0 ψ ψ . (15)
The response coefficients require external input for the strong di-J / ψ J/\psi J / ψ widths. The inversion is therefore conditional on the strong-decay model and the state assignment, with the radiative and strong widths in each response describing the same state. Alternatively, let g 2 γ ψ g^{\gamma\psi}_{2} g 2 γ ψ denote the tensor fraction of the efficiency-corrected radiative yield in the same mass window and production region. Since the scalar has f L , 0 = 0 f_{L,0}=0 f L , 0 = 0 and Eq. (8) is linear in f L f_L f L , an incoherent two-spin sample satisfies
f L , m i x = g 2 γ ψ f L , 2 , g 2 γ ψ = f L , m i x f L , 2 . (16) f_{L,\mathrm{mix}}=g^{\gamma\psi}_{2}f_{L,2},\qquad g^{\gamma\psi}_{2}=\frac{f_{L,\mathrm{mix}}}{f_{L,2}}. \tag*{(16)} f L , mix = g 2 γ ψ f L , 2 , g 2 γ ψ = f L , 2 f L , mix . (16)
This determines the radiative tensor fraction without strong-decay inputs, subject to the tensor-polarization prediction and acceptance conditions above. It does not by itself determine the di-J / ψ J/\psi J / ψ spin fractions.
Eq. (14) treats the scalar and tensor components as incoherent yields. If the selected mass window contains overlapping spin amplitudes, additional partial waves, or an interfering continuum background, the corresponding interference terms must be included in a joint angular and lineshape analysis.
Conclusion. We have calculated the complete NLO QCD corrections to three fully charm tetraquark radiative transitions at leading v v v . The NLO scalar hard matrix is not proportional to its LO counterpart, changing the relative contributions of the color-spin components and their interference. For the chosen LDMEs at m c = 1.5 m_c=1.5 m c = 1.5 GeV and μ R = 2 m c \mu_R=2m_c μ R = 2 m c , the NLO widths are 2.3–3.1 times the LO widths.
The diphoton angular distribution probes the parent spin without an overall LDME normalization, and NLO corrections affect this spin-sensitive observable. At μ R = 2 m c \mu_R=2m_c μ R = 2 m c , the tensor longitudinal fraction f L f_L f L changes from 0.11 at LO to 0.18 at strictly expanded NLO, although the prediction remains sensitive to higher-order corrections. The NLO-corrected radiative widths provide updated inputs for constraining tensor LDMEs and scalar–tensor fractions in combination with compatible production and strong-decay information. Our results provide important theoretical input for constraining the properties of fully charm tetraquarks and for searches for states below their respective lowest dicharmonium thresholds.
Acknowledgments. The authors thank Long-Bin Chen, Qi-Ming Feng, and Hao Yang for useful discussions. This work is supported by the National Natural Science Foundation of China (NSFC) under Grants No. 12547114, 12325503, and 12547172, and by the High-Performance Computing Platform of Peking University. X. L. is also supported by the China Postdoctoral Science Foundation under Grant No. 8206301723.
References
Supplemental Material
Operator conventions and matching
With D = 4 − 2 ϵ D = 4 - 2\epsilon D = 4 − 2 ϵ , d s = D − 1 d_s = D - 1 d s = D − 1 , and two-component heavy-quark fields ψ \psi ψ , χ \chi χ , define
C 3 ˉ a b , c d = δ a c δ b d − δ a d δ b c 2 3 , C 6 a b , c d = δ a c δ b d + δ a d δ b c 2 6 , C_{\bar{3}}^{ab,cd} = \frac{\delta^{ac}\delta^{bd} - \delta^{ad}\delta^{bc}}{2\sqrt{3}}, \qquad C_{6}^{ab,cd} = \frac{\delta^{ac}\delta^{bd} + \delta^{ad}\delta^{bc}}{2\sqrt{6}}, C 3 ˉ ab , c d = 2 3 δ a c δ b d − δ a d δ b c , C 6 ab , c d = 2 6 δ a c δ b d + δ a d δ b c ,
S 0 a b = ψ a T i σ 2 ψ b , S 1 a b , i = ψ a T i σ 2 σ i ψ b , S_{0}^{ab} = \psi_a^T i\sigma^2\psi_b, \qquad S_{1}^{ab,i} = \psi_a^T i\sigma^2\sigma^i\psi_b, S 0 ab = ψ a T i σ 2 ψ b , S 1 ab , i = ψ a T i σ 2 σ i ψ b ,
S ˉ 0 c d = χ c i σ 2 χ d ∗ , S ˉ 1 c d , j = χ c i σ 2 σ j χ d ∗ . (17) \bar{S}_{0}^{cd} = \chi_c i\sigma^2\chi_d^*, \qquad\bar{S}_{1}^{cd,j} = \chi_c i\sigma^2\sigma^j\chi_d^*. \tag*{(17)} S ˉ 0 c d = χ c i σ 2 χ d ∗ , S ˉ 1 c d , j = χ c i σ 2 σ j χ d ∗ . (17)
The physical scalar phases and axial current are fixed by
Q 3 ˉ = − δ i j d s S 1 a b , i S ˉ 1 c d , j C 3 ˉ a b , c d , Q 6 = S 0 a b S ˉ 0 c d C 6 a b , c d , Q 1 i = − i ϵ i j k 2 S 1 a b , j S ˉ 1 c d , k C 3 ˉ a b , c d . (18) Q_{\bar{3}} = -\frac{\delta_{ij}}{\sqrt{d_s}}S_{1}^{ab,i}\bar{S}_{1}^{cd,j}C_{\bar{3}}^{ab,cd}, \qquad Q_{6} = S_{0}^{ab}\bar{S}_{0}^{cd}C_{6}^{ab,cd}, \qquad Q_{1}^{i} = -\frac{i\epsilon^{ijk}}{\sqrt{2}}S_{1}^{ab,j}\bar{S}_{1}^{cd,k}C_{\bar{3}}^{ab,cd}. \tag*{(18)} Q 3 ˉ = − d s δ ij S 1 ab , i S ˉ 1 c d , j C 3 ˉ ab , c d , Q 6 = S 0 ab S ˉ 0 c d C 6 ab , c d , Q 1 i = − 2 i ϵ ij k S 1 ab , j S ˉ 1 c d , k C 3 ˉ ab , c d . (18)
For each normalized symmetric traceless tensor polarization ϵ i j ( λ ) \epsilon^{ij}(\lambda) ϵ ij ( λ ) , define
Q 2 ( λ ) = ϵ i j ∗ ( λ ) S 1 a b , i S ˉ 1 c d , j C 6 a b , c d , ϵ i j ∗ ( λ ) ϵ i j ( λ ′ ) = δ λ λ ′ . (19) Q_{2}(\lambda) = \epsilon_{ij}^{*}(\lambda)S_{1}^{ab,i}\bar{S}_{1}^{cd,j}C_{6}^{ab,cd}, \qquad\epsilon_{ij}^{*}(\lambda)\epsilon^{ij}(\lambda^{\prime}) = \delta_{\lambda\lambda^{\prime}}. \tag*{(19)} Q 2 ( λ ) = ϵ ij ∗ ( λ ) S 1 ab , i S ˉ 1 c d , j C 6 ab , c d , ϵ ij ∗ ( λ ) ϵ ij ( λ ′ ) = δ λ λ ′ . (19)
The spin-two projector is Π i j , k l = 1 2 ( δ i k δ j l + δ i l δ j k ) − δ i j δ k l / d s \Pi^{ij,kl} = \frac{1}{2}(\delta^{ik}\delta^{jl}+\delta^{il}\delta^{jk})-\delta^{ij}\delta^{kl}/d_s Π ij , k l = 2 1 ( δ ik δ j l + δ i l δ j k ) − δ ij δ k l / d s . Axial external polarizations remain four-dimensional in BMHV. Loop momenta and contracted QCD indices are D D D -dimensional [33 , 34 ] . We use L n = ⟨ 0 ∣ Q n r e n ∣ T r e l ⟩ / 2 M T L_n = \langle0|Q_n^{\mathrm{ren}}|T_{\mathrm{rel}}\rangle/\sqrt{2M_T} L n = ⟨ 0∣ Q n ren ∣ T rel ⟩ / 2 M T and ρ n m = L n L m ∗ \rho_{nm}=L_nL_m^* ρ nm = L n L m ∗ , with spinful tetraquark decay LDMEs defined for one polarization. The charmonium convention is ρ ψ = ρ J / ψ \rho_{\psi}=\rho_{J/\psi} ρ ψ = ρ J / ψ (spin summed) and ρ η = ρ η c \rho_{\eta}=\rho_{\eta_c} ρ η = ρ η c .
Matching uses the same labelled on-shell partonic amplitude and operator matrix elements Φ \Phi Φ , fixing identical-particle factors. With coupling factors included,
M ( 0 ) = C ( 0 ) Φ ( 0 ) , C ( 1 ) Φ ( 0 ) = M Q C D , r e n ( 1 ) − C ( 0 ) Φ E F T , r e n ( 1 ) . (20) \mathcal{M}^{(0)}=C^{(0)}\Phi^{(0)}, \qquad C^{(1)}\Phi^{(0)}=\mathcal{M}_{\mathrm{QCD,ren}}^{(1)}-C^{(0)}\Phi_{\mathrm{EFT,ren}}^{(1)}. \tag*{(20)} M ( 0 ) = C ( 0 ) Φ ( 0 ) , C ( 1 ) Φ ( 0 ) = M QCD , ren ( 1 ) − C ( 0 ) Φ EFT , ren ( 1 ) . (20)
The common Coulomb term is subtracted at finite relative velocity with kinetic propagators retained, before the zero-velocity hard limit [32 ] . Nonpotential integrals are scaleless, with ultraviolet and infrared poles tracked separately. The half-LSZ residues arise by differentiating the heavy-quark self-energy with respect to a residual energy before the on-shell limit. In Feynman gauge, a s = α s / ( 4 π ) a_s=\alpha_s/(4\pi) a s = α s / ( 4 π ) gives
Φ n ( 1 ) ∣ p a i r s = − 8 a s ( 1 ϵ U V − 1 ϵ I R ) Φ ( 0 ) = − Φ n ( 1 ) ∣ h a l f − L S Z . (21) \left.\Phi_{n}^{(1)}\right|_{\mathrm{pairs}}=-8a_s\left(\frac{1}{\epsilon_{\mathrm{UV}}}-\frac{1}{\epsilon_{\mathrm{IR}}}\right)\Phi^{(0)}=-\left.\Phi_{n}^{(1)}\right|_{\mathrm{half-LSZ}}. \tag*{(21)} Φ n ( 1 ) pairs = − 8 a s ( ϵ UV 1 − ϵ IR 1 ) Φ ( 0 ) = − Φ n ( 1 ) half − LSZ . (21)
Thus Z P P ( 1 ) = 0 Z_{PP}^{(1)}=0 Z P P ( 1 ) = 0 and the on-shell nonpotential matrix element vanishes. Leading density vertices preserve the Pauli tensor. Subleading terms supply no derivative-free v 0 v^0 v 0 conversion. Dimensional spin factors are retained through pole-finite products [30 ] . Different residual-energy or evanescent conventions require finite coefficient conversion.
The workflow uses FeynArts [41 ] , CalcLoop [42 ] , Kira [43 ] , and AMFlow [44 ] . With the renormalization schemes stated in the Letter, M c t = m c δ Z m M m , u n i t + ( 3 δ Z 2 + 4 δ Z g ) M ( 0 ) \mathcal{M}_{\mathrm{ct}}=m_c\delta Z_m\mathcal{M}_{m,\mathrm{unit}}+(3\delta Z_2+4\delta Z_g)\mathcal{M}^{(0)} M ct = m c δ Z m M m , unit + ( 3 δ Z 2 + 4 δ Z g ) M ( 0 ) , where M m , u n i t \mathcal{M}_{m,\mathrm{unit}} M m , unit sums unit internal mass insertions. Our diphoton LO short-distance coefficients agree with the corrected arXiv v3 results of Ref. [26 ] . The LO radiative amplitudes of Ref. [28 ] are twice ours, and its widths are four times ours at fixed LDMEs, consistent with the prerevision normalization of Ref. [26 ] ; its scalar numbers additionally apply mixing-angle weights to the density entries.
Explicit finite coefficients without coefficient tables
Using the functions and branches defined with Eqs. (35) –(37) , the six finite coefficients are given explicitly below. The axial factor s 1 = 135 / 140608 s_1=135/140608 s 1 = 135/140608 is absorbed in c 1 c_1 c 1 .
F α ( 1 ) ( r ) = F α ( 0 ) 4 π 2 [ c a + 25 3 ln r ] , r = μ R m c . (22) F_{\alpha}^{(1)}(r)=\frac{F_{\alpha}^{(0)}}{4\pi^2}\left[c_a+\frac{25}{3}\ln r\right],\qquad r=\frac{\mu_R}{m_c}. \tag*{(22)} F α ( 1 ) ( r ) = 4 π 2 F α ( 0 ) [ c a + 3 25 ln r ] , r = m c μ R . (22)
Scalar channel
Scalar antitriplet component. For F ( 0 , 3 ˉ ) ( 0 ) = − 4901 270 6 F_{(0,\bar{3})}^{(0)}=-\frac{4901}{270\sqrt{6}} F ( 0 , 3 ˉ ) ( 0 ) = − 270 6 4901 ,
c ( 0 , 3 ˉ ) = 19705408 4631445 − 57013854379 93636702432 π 2 + 403532057 466849656 ℓ 2 − 2001013 743148432 ℓ 2 ℓ 11 + 3414669857593 343334575584 ℓ 2 2 + 105325 75029409 ℓ 2 ℓ 23 + 318182959 389041380 ℓ 3 − 811954208665 82873863072 ℓ 2 ℓ 3 + 7275333997643 2403342029088 ℓ 3 2 − 84023 411684 ℓ 5 − 255868253393 400557004848 ℓ 2 ℓ 5 − 586335896801 1201671014544 ℓ 3 ℓ 5 + 8373206987 100139251212 ℓ 5 2 − 728363 743148432 ℓ 7 ℓ 11 + 45394720867 92436231888 ℓ 2 ℓ 7 + 190216051555 1201671014544 ℓ 3 ℓ 7 − 21065 75029409 ℓ 5 ℓ 7 − 134064519937 1201671014544 ℓ 7 2 + 145040 L 44109 3 − 9432925 4234464 L 2 + 125631767 111154680 A + 4901 9 ℓ 11 ( ℓ 11 − ℓ 3 ) − 636325 743148432 U − 21065 75029409 ℓ 23 ( ℓ 23 − ℓ 5 ) + 1771795 4234464 L ( ℓ 2 + 5 ℓ 3 ) + i π [ 128796943 875343105 + 385 88218 3 + 636325 371574216 ℓ 19 + 2882768459 6827676219 ℓ 2 + 17 1058616 ℓ 3 − 759412700 6827676219 ℓ 5 − 1077152 10718487 ℓ 7 − 880 132327 L ] − 989731 6243874 Ψ 1 − 525723811 8403293808 Ψ 2 + 265181 471613428 Ψ 3 + 97264719247 200278502424 Ψ 4 + 5535310622767 1201671014544 Ψ 5 − 464279 550215666 Ψ 6 + 418342686661 75104438409 Ψ 7 − 253432628 10729205487 Ψ 8 − 419107058 2589808221 Ψ 9 + 636325 743148432 Ψ 10 − 21065 75029409 Ψ 11 − 21065 75029409 Ψ 12 + 9 4901 Ψ 13 + 1771795 2117232 Ψ 14 + 485392 10729205487 Ψ 15 + 7555292 71324253 Ψ 16 − 465191 926289 Ψ 17 − 989731 3121937 Ψ 18 . (23) \begin{aligned}
c_{(0,\bar{3})}={}&\frac{19705408}{4631445}-\frac{57013854379}{93636702432}\pi^2+\frac{403532057}{466849656}\ell_2-\frac{2001013}{743148432}\ell_2\ell_{11}+\frac{3414669857593}{343334575584}\ell_2^2\\
&+\frac{105325}{75029409}\ell_2\ell_{23}+\frac{318182959}{389041380}\ell_3-\frac{811954208665}{82873863072}\ell_2\ell_3+\frac{7275333997643}{2403342029088}\ell_3^2-\frac{84023}{411684}\ell_5\\
&-\frac{255868253393}{400557004848}\ell_2\ell_5-\frac{586335896801}{1201671014544}\ell_3\ell_5+\frac{8373206987}{100139251212}\ell_5^2-\frac{728363}{743148432}\ell_7\ell_{11}\\
&+\frac{45394720867}{92436231888}\ell_2\ell_7+\frac{190216051555}{1201671014544}\ell_3\ell_7-\frac{21065}{75029409}\ell_5\ell_7-\frac{134064519937}{1201671014544}\ell_7^2+\frac{145040L}{44109\sqrt{3}}\\
&-\frac{9432925}{4234464}L^2+\frac{125631767}{111154680}A+\frac{4901}{9}\ell_{11}(\ell_{11}-\ell_3)-\frac{636325}{743148432}U-\frac{21065}{75029409}\ell_{23}(\ell_{23}-\ell_5)\\
&+\frac{1771795}{4234464}L(\ell_2+5\ell_3)\\
&+i\pi\left[\frac{128796943}{875343105}+\frac{385}{88218\sqrt{3}}+\frac{636325}{371574216}\ell_{19}+\frac{2882768459}{6827676219}\ell_2+\frac{17}{1058616}\ell_3-\frac{759412700}{6827676219}\ell_5\right.\\
&\left.\qquad-\frac{1077152}{10718487}\ell_7-\frac{880}{132327}L\right]\\
&-\frac{989731}{6243874}\Psi_1-\frac{525723811}{8403293808}\Psi_2+\frac{265181}{471613428}\Psi_3+\frac{97264719247}{200278502424}\Psi_4\\
&+\frac{5535310622767}{1201671014544}\Psi_5-\frac{464279}{550215666}\Psi_6+\frac{418342686661}{75104438409}\Psi_7-\frac{253432628}{10729205487}\Psi_8\\
&-\frac{419107058}{2589808221}\Psi_9+\frac{636325}{743148432}\Psi_{10}-\frac{21065}{75029409}\Psi_{11}-\frac{21065}{75029409}\Psi_{12}\\
&+\frac{9}{4901}\Psi_{13}+\frac{1771795}{2117232}\Psi_{14}+\frac{485392}{10729205487}\Psi_{15}+\frac{7555292}{71324253}\Psi_{16}\\
&-\frac{465191}{926289}\Psi_{17}-\frac{989731}{3121937}\Psi_{18}. \tag*{(23)}
\end{aligned} c ( 0 , 3 ˉ ) = 4631445 19705408 − 93636702432 57013854379 π 2 + 466849656 403532057 ℓ 2 − 743148432 2001013 ℓ 2 ℓ 11 + 343334575584 3414669857593 ℓ 2 2 + 75029409 105325 ℓ 2 ℓ 23 + 389041380 318182959 ℓ 3 − 82873863072 811954208665 ℓ 2 ℓ 3 + 2403342029088 7275333997643 ℓ 3 2 − 411684 84023 ℓ 5 − 400557004848 255868253393 ℓ 2 ℓ 5 − 1201671014544 586335896801 ℓ 3 ℓ 5 + 100139251212 8373206987 ℓ 5 2 − 743148432 728363 ℓ 7 ℓ 11 + 92436231888 45394720867 ℓ 2 ℓ 7 + 1201671014544 190216051555 ℓ 3 ℓ 7 − 75029409 21065 ℓ 5 ℓ 7 − 1201671014544 134064519937 ℓ 7 2 + 44109 3 145040 L − 4234464 9432925 L 2 + 111154680 125631767 A + 9 4901 ℓ 11 ( ℓ 11 − ℓ 3 ) − 743148432 636325 U − 75029409 21065 ℓ 23 ( ℓ 23 − ℓ 5 ) + 4234464 1771795 L ( ℓ 2 + 5 ℓ 3 ) + iπ [ 875343105 128796943 + 88218 3 385 + 371574216 636325 ℓ 19 + 6827676219 2882768459 ℓ 2 + 1058616 17 ℓ 3 − 6827676219 759412700 ℓ 5 − 10718487 1077152 ℓ 7 − 132327 880 L ] − 6243874 989731 Ψ 1 − 8403293808 525723811 Ψ 2 + 471613428 265181 Ψ 3 + 200278502424 97264719247 Ψ 4 + 1201671014544 5535310622767 Ψ 5 − 550215666 464279 Ψ 6 + 75104438409 418342686661 Ψ 7 − 10729205487 253432628 Ψ 8 − 2589808221 419107058 Ψ 9 + 743148432 636325 Ψ 10 − 75029409 21065 Ψ 11 − 75029409 21065 Ψ 12 + 4901 9 Ψ 13 + 2117232 1771795 Ψ 14 + 10729205487 485392 Ψ 15 + 71324253 7555292 Ψ 16 − 926289 465191 Ψ 17 − 3121937 989731 Ψ 18 . (23)
Scalar sextet component. For F ( 0 , 6 ) ( 0 ) = 95 108 F_{(0,6)}^{(0)}=\frac{95}{108} F ( 0 , 6 ) ( 0 ) = 108 95 ,
c ( 0 , 6 ) = 17350 3591 − 768763063 259290720 π 2 + 1016561263 45246600 ℓ 2 + 16464109 72025200 ℓ 2 ℓ 11 + 21494572709 1751349600 ℓ 2 2 − 105325 290871 ℓ 2 ℓ 23 + 15283949 1508220 ℓ 3 + 471411350261 232929496800 ℓ 2 ℓ 3 + 695019422029 232929496800 ℓ 3 2 + 5179 7980 ℓ 5 − 10675072799 1552863312 ℓ 2 ℓ 5 − 134336682923 23292949680 ℓ 3 ℓ 5 + 195658747 388215828 ℓ 5 2 + 15352141 72025200 ℓ 7 ℓ 11 − 22204271851 8958826800 ℓ 2 ℓ 7 + 53389496683 116464748400 ℓ 3 ℓ 7 + 21065 290871 ℓ 5 ℓ 7 + 84289501273 116464748400 ℓ 7 2 − 308 L 171 3 − 508903 82080 L 2 − 57680083 2154600 A − 1425 11 ℓ 11 ( ℓ 11 − ℓ 3 ) + 636325 2881008 U + 21065 290871 ℓ 23 ( ℓ 23 − ℓ 5 ) + 44863 49248 L ( ℓ 2 + 5 ℓ 3 ) + i π [ − 12636587 16967475 + 7 342 3 − 636325 1440504 ℓ 19 − 996504107 661731525 ℓ 2 − 17 4104 ℓ 3 + 154343341 132346305 ℓ 5 + 34144 207765 ℓ 7 − 513 207765 L ] + 1374461 3267810 Ψ 1 + 327464491 814438800 Ψ 2 − 265181 1828332 Ψ 3 + 24679098253 3882158280 Ψ 4 \begin{aligned}
c_{(0,6)}={}&\frac{17350}{3591}-\frac{768763063}{259290720}\pi^2+\frac{1016561263}{45246600}\ell_2+\frac{16464109}{72025200}\ell_2\ell_{11}+\frac{21494572709}{1751349600}\ell_2^2-\frac{105325}{290871}\ell_2\ell_{23}\\
&+\frac{15283949}{1508220}\ell_3+\frac{471411350261}{232929496800}\ell_2\ell_3+\frac{695019422029}{232929496800}\ell_3^2+\frac{5179}{7980}\ell_5-\frac{10675072799}{1552863312}\ell_2\ell_5\\
&-\frac{134336682923}{23292949680}\ell_3\ell_5+\frac{195658747}{388215828}\ell_5^2+\frac{15352141}{72025200}\ell_7\ell_{11}-\frac{22204271851}{8958826800}\ell_2\ell_7\\
&+\frac{53389496683}{116464748400}\ell_3\ell_7+\frac{21065}{290871}\ell_5\ell_7+\frac{84289501273}{116464748400}\ell_7^2-\frac{308L}{171\sqrt{3}}-\frac{508903}{82080}L^2-\frac{57680083}{2154600}A\\
&-\frac{1425}{11}\ell_{11}(\ell_{11}-\ell_3)+\frac{636325}{2881008}U+\frac{21065}{290871}\ell_{23}(\ell_{23}-\ell_5)+\frac{44863}{49248}L(\ell_2+5\ell_3)\\
&+i\pi\left[-\frac{12636587}{16967475}+\frac{7}{342\sqrt{3}}-\frac{636325}{1440504}\ell_{19}-\frac{996504107}{661731525}\ell_2-\frac{17}{4104}\ell_3+\frac{154343341}{132346305}\ell_5\right.\\
&\left.\qquad+\frac{34144}{207765}\ell_7-\frac{513}{207765}L\right]\\
&+\frac{1374461}{3267810}\Psi_1+\frac{327464491}{814438800}\Psi_2-\frac{265181}{1828332}\Psi_3+\frac{24679098253}{3882158280}\Psi_4
\end{aligned} c ( 0 , 6 ) = 3591 17350 − 259290720 768763063 π 2 + 45246600 1016561263 ℓ 2 + 72025200 16464109 ℓ 2 ℓ 11 + 1751349600 21494572709 ℓ 2 2 − 290871 105325 ℓ 2 ℓ 23 + 1508220 15283949 ℓ 3 + 232929496800 471411350261 ℓ 2 ℓ 3 + 232929496800 695019422029 ℓ 3 2 + 7980 5179 ℓ 5 − 1552863312 10675072799 ℓ 2 ℓ 5 − 23292949680 134336682923 ℓ 3 ℓ 5 + 388215828 195658747 ℓ 5 2 + 72025200 15352141 ℓ 7 ℓ 11 − 8958826800 22204271851 ℓ 2 ℓ 7 + 116464748400 53389496683 ℓ 3 ℓ 7 + 290871 21065 ℓ 5 ℓ 7 + 116464748400 84289501273 ℓ 7 2 − 171 3 308 L − 82080 508903 L 2 − 2154600 57680083 A − 11 1425 ℓ 11 ( ℓ 11 − ℓ 3 ) + 2881008 636325 U + 290871 21065 ℓ 23 ( ℓ 23 − ℓ 5 ) + 49248 44863 L ( ℓ 2 + 5 ℓ 3 ) + iπ [ − 16967475 12636587 + 342 3 7 − 1440504 636325 ℓ 19 − 661731525 996504107 ℓ 2 − 4104 17 ℓ 3 + 132346305 154343341 ℓ 5 + 207765 34144 ℓ 7 − 207765 513 L ] + 3267810 1374461 Ψ 1 + 814438800 327464491 Ψ 2 − 1828332 265181 Ψ 3 + 3882158280 24679098253 Ψ 4
− 179021864863 116464748400 Ψ 5 + 464279 2133054 Ψ 6 − 5549133496 7279046775 Ψ 7 + 360294892 207972765 Ψ 8 + 6585099646 7279046775 Ψ 9 − 636325 2881008 Ψ 10 + 21065 290871 Ψ 11 + 21065 290871 Ψ 12 − 11 1425 Ψ 13 + 44863 24624 Ψ 14 − 485392 41594553 Ψ 15 + 9592532 1382535 Ψ 16 − 2021 17955 Ψ 17 + 1374461 1633905 Ψ 18 . (24) -\frac{179021864863}{116464748400}\Psi_5+\frac{464279}{2133054}\Psi_6-\frac{5549133496}{7279046775}\Psi_7+\frac{360294892}{207972765}\Psi_8+\frac{6585099646}{7279046775}\Psi_9-\frac{636325}{2881008}\Psi_{10}+\frac{21065}{290871}\Psi_{11}+\frac{21065}{290871}\Psi_{12}-\frac{11}{1425}\Psi_{13}+\frac{44863}{24624}\Psi_{14}-\frac{485392}{41594553}\Psi_{15}+\frac{9592532}{1382535}\Psi_{16}-\frac{2021}{17955}\Psi_{17}+\frac{1374461}{1633905}\Psi_{18}. \tag*{(24)} − 116464748400 179021864863 Ψ 5 + 2133054 464279 Ψ 6 − 7279046775 5549133496 Ψ 7 + 207972765 360294892 Ψ 8 + 7279046775 6585099646 Ψ 9 − 2881008 636325 Ψ 10 + 290871 21065 Ψ 11 + 290871 21065 Ψ 12 − 1425 11 Ψ 13 + 24624 44863 Ψ 14 − 41594553 485392 Ψ 15 + 1382535 9592532 Ψ 16 − 17955 2021 Ψ 17 + 1633905 1374461 Ψ 18 . (24)
Axial channel
Axial component. For F 1 ( 0 ) = 2197 3 270 F_1^{(0)}=\frac{2197\sqrt{3}}{270} F 1 ( 0 ) = 270 2197 3 ,
c 1 = 16052327 4152330 + 7015934041 167900294016 π 2 + 419180443 418554864 ℓ 2 − 10754225 1332542016 ℓ 2 ℓ 11 + 1307398287323 205211470464 ℓ 2 2 + 612485 33633873 ℓ 2 ℓ 23 + 237545047 697591440 ℓ 3 − 21163435187693 4309440879744 ℓ 2 ℓ 3 + 1638184539913 1436480293248 ℓ 3 2 − 478853 1245699 ℓ 5 − 2276199242171 2154720439872 ℓ 2 ℓ 5 − 459443697563 718240146624 ℓ 3 ℓ 5 + 22378953607 119706691104 ℓ 5 2 + 10754225 1332542016 ℓ 7 ℓ 11 + 15574666615 165747726144 ℓ 2 ℓ 7 + 715071965 79804460736 ℓ 3 ℓ 7 − 16030 4804839 ℓ 5 ℓ 7 + 50186459311 718240146624 ℓ 7 2 + 677375 L 158184 3 − 18979613 7592832 L 2 + 66021763 99655920 A − 10754225 1332542016 U − 129355 33633873 ℓ 23 ( ℓ 23 − ℓ 5 ) + 9341809 22778496 L ( ℓ 2 + 5 ℓ 3 ) + 1270 1245699 ℓ 3 ℓ 23 + i π [ − 13540663 784790370 − 250 19773 3 + 10754225 666271008 ℓ 19 + 803337779 1360303308 ℓ 2 + 132229 4429152 ℓ 3 − 6012145 302289624 ℓ 5 − 73768 369603 ℓ 7 + 500 59319 L ] − 415867 37786203 Ψ 1 + 2685323713 15067975104 Ψ 2 + 5648047 563767776 Ψ 3 + 224445296147 359120073312 Ψ 4 + 1759443607091 718240146624 Ψ 5 − 14122861 845651664 Ψ 6 + 900295374523 538680109968 Ψ 7 − 2546110145 19238575356 Ψ 8 − 18170393677 538680109968 Ψ 9 + 10754225 1332542016 Ψ 10 − 129355 33633873 Ψ 11 − 16030 4804839 Ψ 12 + 9341809 11389248 Ψ 14 + 566656 687091977 Ψ 15 + 124451 126126 Ψ 16 − 103457 118638 Ψ 17 − 831734 37786203 Ψ 18 − 1245699 635 Ψ 19 . (25) \begin{aligned}
c_1={}&\frac{16052327}{4152330}+\frac{7015934041}{167900294016}\pi^2+\frac{419180443}{418554864}\ell_2-\frac{10754225}{1332542016}\ell_2\ell_{11}+\frac{1307398287323}{205211470464}\ell_2^2\\
&+\frac{612485}{33633873}\ell_2\ell_{23}+\frac{237545047}{697591440}\ell_3-\frac{21163435187693}{4309440879744}\ell_2\ell_3+\frac{1638184539913}{1436480293248}\ell_3^2-\frac{478853}{1245699}\ell_5\\
&-\frac{2276199242171}{2154720439872}\ell_2\ell_5-\frac{459443697563}{718240146624}\ell_3\ell_5+\frac{22378953607}{119706691104}\ell_5^2+\frac{10754225}{1332542016}\ell_7\ell_{11}\\
&+\frac{15574666615}{165747726144}\ell_2\ell_7+\frac{715071965}{79804460736}\ell_3\ell_7-\frac{16030}{4804839}\ell_5\ell_7+\frac{50186459311}{718240146624}\ell_7^2+\frac{677375L}{158184\sqrt{3}}\\
&-\frac{18979613}{7592832}L^2+\frac{66021763}{99655920}A-\frac{10754225}{1332542016}U-\frac{129355}{33633873}\ell_{23}(\ell_{23}-\ell_5)+\frac{9341809}{22778496}L(\ell_2+5\ell_3)\\
&+\frac{1270}{1245699}\ell_3\ell_{23}+i\pi\left[-\frac{13540663}{784790370}-\frac{250}{19773\sqrt{3}}+\frac{10754225}{666271008}\ell_{19}+\frac{803337779}{1360303308}\ell_2+\frac{132229}{4429152}\ell_3-\frac{6012145}{302289624}\ell_5\right.\\
&\left.\qquad-\frac{73768}{369603}\ell_7+\frac{500}{59319}L\right]-\frac{415867}{37786203}\Psi_1+\frac{2685323713}{15067975104}\Psi_2+\frac{5648047}{563767776}\Psi_3+\frac{224445296147}{359120073312}\Psi_4\\
&+\frac{1759443607091}{718240146624}\Psi_5-\frac{14122861}{845651664}\Psi_6+\frac{900295374523}{538680109968}\Psi_7-\frac{2546110145}{19238575356}\Psi_8\\
&-\frac{18170393677}{538680109968}\Psi_9+\frac{10754225}{1332542016}\Psi_{10}-\frac{129355}{33633873}\Psi_{11}-\frac{16030}{4804839}\Psi_{12}\\
&+\frac{9341809}{11389248}\Psi_{14}+\frac{566656}{687091977}\Psi_{15}+\frac{124451}{126126}\Psi_{16}-\frac{103457}{118638}\Psi_{17}\\
&-\frac{831734}{37786203}\Psi_{18}-\frac{1245699}{635}\Psi_{19}. \tag*{(25)}
\end{aligned} c 1 = 4152330 16052327 + 167900294016 7015934041 π 2 + 418554864 419180443 ℓ 2 − 1332542016 10754225 ℓ 2 ℓ 11 + 205211470464 1307398287323 ℓ 2 2 + 33633873 612485 ℓ 2 ℓ 23 + 697591440 237545047 ℓ 3 − 4309440879744 21163435187693 ℓ 2 ℓ 3 + 1436480293248 1638184539913 ℓ 3 2 − 1245699 478853 ℓ 5 − 2154720439872 2276199242171 ℓ 2 ℓ 5 − 718240146624 459443697563 ℓ 3 ℓ 5 + 119706691104 22378953607 ℓ 5 2 + 1332542016 10754225 ℓ 7 ℓ 11 + 165747726144 15574666615 ℓ 2 ℓ 7 + 79804460736 715071965 ℓ 3 ℓ 7 − 4804839 16030 ℓ 5 ℓ 7 + 718240146624 50186459311 ℓ 7 2 + 158184 3 677375 L − 7592832 18979613 L 2 + 99655920 66021763 A − 1332542016 10754225 U − 33633873 129355 ℓ 23 ( ℓ 23 − ℓ 5 ) + 22778496 9341809 L ( ℓ 2 + 5 ℓ 3 ) + 1245699 1270 ℓ 3 ℓ 23 + iπ [ − 784790370 13540663 − 19773 3 250 + 666271008 10754225 ℓ 19 + 1360303308 803337779 ℓ 2 + 4429152 132229 ℓ 3 − 302289624 6012145 ℓ 5 − 369603 73768 ℓ 7 + 59319 500 L ] − 37786203 415867 Ψ 1 + 15067975104 2685323713 Ψ 2 + 563767776 5648047 Ψ 3 + 359120073312 224445296147 Ψ 4 + 718240146624 1759443607091 Ψ 5 − 845651664 14122861 Ψ 6 + 538680109968 900295374523 Ψ 7 − 19238575356 2546110145 Ψ 8 − 538680109968 18170393677 Ψ 9 + 1332542016 10754225 Ψ 10 − 33633873 129355 Ψ 11 − 4804839 16030 Ψ 12 + 11389248 9341809 Ψ 14 + 687091977 566656 Ψ 15 + 126126 124451 Ψ 16 − 118638 103457 Ψ 17 − 37786203 831734 Ψ 18 − 635 1245699 Ψ 19 . (25)
Tensor channel
First tensor component. For F ( 2 , 1 ) ( 0 ) = 454 135 F_{(2,1)}^{(0)}=\frac{454}{135} F ( 2 , 1 ) ( 0 ) = 135 454 ,
c ( 2 , 1 ) = 3321163 1103220 + 360597722209 624524898816 π 2 + 151819933 111204576 ℓ 2 − 222780197 4956546816 ℓ 2 ℓ 11 + 1342472275387 208174966272 ℓ 2 2 + 5027275 62552574 ℓ 2 ℓ 23 − 11676467 11583810 ℓ 3 − 1161536130707 1457224763904 ℓ 2 ℓ 3 − 1508389675015 1457224763904 ℓ 3 2 − 11036957 18534096 ℓ 5 − 328402317563 242870793984 ℓ 2 ℓ 5 − 494740059371 728612381952 ℓ 3 ℓ 5 + 2080537483 40478465664 ℓ 5 2 + 61129253 4956546816 ℓ 7 ℓ 11 + 20791021297 56047106304 ℓ 2 ℓ 7 + 87987509569 728612381952 ℓ 3 ℓ 7 − 1005455 62552574 ℓ 5 ℓ 7 + 39701625641 728612381952 ℓ 7 2 + 1144415 L 196128 3 − 32919995 9414144 L 2 − 190510889 46335240 A + 1799 110322 ℓ 11 ( ℓ 11 − ℓ 3 ) − 141954725 4956546816 U − 1005455 62552574 ℓ 23 ( ℓ 23 − ℓ 5 ) + 12101095 28242432 L ( ℓ 2 + 5 ℓ 3 ) + i π [ 54522751 417017160 − 140 681 3 + 141954725 2478273408 ℓ 19 + 3428049208 2846142117 ℓ 2 + 21263 261504 ℓ 3 − 29791891925 91076547744 ℓ 5 ] . \begin{aligned}
c_{(2,1)}={}&\frac{3321163}{1103220}+\frac{360597722209}{624524898816}\pi^2+\frac{151819933}{111204576}\ell_2-\frac{222780197}{4956546816}\ell_2\ell_{11}+\frac{1342472275387}{208174966272}\ell_2^2\\
&+\frac{5027275}{62552574}\ell_2\ell_{23}-\frac{11676467}{11583810}\ell_3-\frac{1161536130707}{1457224763904}\ell_2\ell_3-\frac{1508389675015}{1457224763904}\ell_3^2-\frac{11036957}{18534096}\ell_5\\
&-\frac{328402317563}{242870793984}\ell_2\ell_5-\frac{494740059371}{728612381952}\ell_3\ell_5+\frac{2080537483}{40478465664}\ell_5^2+\frac{61129253}{4956546816}\ell_7\ell_{11}\\
&+\frac{20791021297}{56047106304}\ell_2\ell_7+\frac{87987509569}{728612381952}\ell_3\ell_7-\frac{1005455}{62552574}\ell_5\ell_7+\frac{39701625641}{728612381952}\ell_7^2+\frac{1144415L}{196128\sqrt{3}}\\
&-\frac{32919995}{9414144}L^2-\frac{190510889}{46335240}A+\frac{1799}{110322}\ell_{11}(\ell_{11}-\ell_3)-\frac{141954725}{4956546816}U-\frac{1005455}{62552574}\ell_{23}(\ell_{23}-\ell_5)\\
&+\frac{12101095}{28242432}L(\ell_2+5\ell_3)+i\pi\left[\frac{54522751}{417017160}-\frac{140}{681\sqrt{3}}+\frac{141954725}{2478273408}\ell_{19}+\frac{3428049208}{2846142117}\ell_2+\frac{21263}{261504}\ell_3-\frac{29791891925}{91076547744}\ell_5\right].
\end{aligned} c ( 2 , 1 ) = 1103220 3321163 + 624524898816 360597722209 π 2 + 111204576 151819933 ℓ 2 − 4956546816 222780197 ℓ 2 ℓ 11 + 208174966272 1342472275387 ℓ 2 2 + 62552574 5027275 ℓ 2 ℓ 23 − 11583810 11676467 ℓ 3 − 1457224763904 1161536130707 ℓ 2 ℓ 3 − 1457224763904 1508389675015 ℓ 3 2 − 18534096 11036957 ℓ 5 − 242870793984 328402317563 ℓ 2 ℓ 5 − 728612381952 494740059371 ℓ 3 ℓ 5 + 40478465664 2080537483 ℓ 5 2 + 4956546816 61129253 ℓ 7 ℓ 11 + 56047106304 20791021297 ℓ 2 ℓ 7 + 728612381952 87987509569 ℓ 3 ℓ 7 − 62552574 1005455 ℓ 5 ℓ 7 + 728612381952 39701625641 ℓ 7 2 + 196128 3 1144415 L − 9414144 32919995 L 2 − 46335240 190510889 A + 110322 1799 ℓ 11 ( ℓ 11 − ℓ 3 ) − 4956546816 141954725 U − 62552574 1005455 ℓ 23 ( ℓ 23 − ℓ 5 ) + 28242432 12101095 L ( ℓ 2 + 5 ℓ 3 ) + iπ [ 417017160 54522751 − 681 3 140 + 2478273408 141954725 ℓ 19 + 2846142117 3428049208 ℓ 2 + 261504 21263 ℓ 3 − 91076547744 29791891925 ℓ 5 ] .
− 30420025 7148856 ℓ 7 + 700 6129 L ] + 375889 7808346 Ψ 1 + 24028243093 56047106304 Ψ 2 + 1553483 17872164 Ψ 3 + 87278032669 121435396992 Ψ 4 + 1144961541037 728612381952 Ψ 5 − 1644821 10425429 Ψ 6 − 2377327749583 91076547744 Ψ 7 − 127391497 116169066 Ψ 8 − 1841323817 5692284234 Ψ 9 + 141954725 4956546816 Ψ 10 − 1005455 62552574 Ψ 11 − 1005455 62552574 Ψ 12 + 1799 110322 Ψ 13 + 12101095 14121216 Ψ 14 + 30308422 406591731 Ψ 15 + 22565987 8108667 Ψ 16 − 6479 42903 Ψ 17 + 375889 3904173 Ψ 18 . (26) -\frac{30420025}{7148856}\ell_{7}+\frac{700}{6129}L]
+\frac{375889}{7808346}\Psi_{1}+\frac{24028243093}{56047106304}\Psi_{2}+\frac{1553483}{17872164}\Psi_{3}+\frac{87278032669}{121435396992}\Psi_{4}
+\frac{1144961541037}{728612381952}\Psi_{5}-\frac{1644821}{10425429}\Psi_{6}-\frac{2377327749583}{91076547744}\Psi_{7}-\frac{127391497}{116169066}\Psi_{8}
-\frac{1841323817}{5692284234}\Psi_{9}+\frac{141954725}{4956546816}\Psi_{10}-\frac{1005455}{62552574}\Psi_{11}-\frac{1005455}{62552574}\Psi_{12}
+\frac{1799}{110322}\Psi_{13}+\frac{12101095}{14121216}\Psi_{14}+\frac{30308422}{406591731}\Psi_{15}+\frac{22565987}{8108667}\Psi_{16}
-\frac{6479}{42903}\Psi_{17}+\frac{375889}{3904173}\Psi_{18}. \tag*{(26)} − 7148856 30420025 ℓ 7 + 6129 700 L ] + 7808346 375889 Ψ 1 + 56047106304 24028243093 Ψ 2 + 17872164 1553483 Ψ 3 + 121435396992 87278032669 Ψ 4 + 728612381952 1144961541037 Ψ 5 − 10425429 1644821 Ψ 6 − 91076547744 2377327749583 Ψ 7 − 116169066 127391497 Ψ 8 − 5692284234 1841323817 Ψ 9 + 4956546816 141954725 Ψ 10 − 62552574 1005455 Ψ 11 − 62552574 1005455 Ψ 12 + 110322 1799 Ψ 13 + 14121216 12101095 Ψ 14 + 406591731 30308422 Ψ 15 + 8108667 22565987 Ψ 16 − 42903 6479 Ψ 17 + 3904173 375889 Ψ 18 . (26)
Second tensor component. For F ( 2 , 2 ) ( 0 ) = 233 270 3 F^{(0)}_{(2,2)}=\frac{233}{270\sqrt{3}} F ( 2 , 2 ) ( 0 ) = 270 3 233 ,
c ( 2 , 2 ) = 810182 660555 + 11694988651 6677418384 π 2 − 381162167 33291972 ℓ 2 − 1718267 52995384 ℓ 2 ℓ 11 − 37321050089 2225806128 ℓ 2 2 + 3427325 21401982 ℓ 2 ℓ 23 − 92832356 13871655 ℓ 3 + 166011001781 7790321448 ℓ 2 ℓ 3 − 161564465269 15580642896 ℓ 3 2 + 2668901 1585332 ℓ 5 + 1438024657 2596773816 ℓ 2 ℓ 5 − 9906289751 7790321448 ℓ 3 ℓ 5 − 337816123 288530424 ℓ 5 2 + 460283 52995384 ℓ 7 ℓ 11 − 388832957 599255496 ℓ 2 ℓ 7 − 933732461 7790321448 ℓ 3 ℓ 7 − 685465 21401982 ℓ 5 ℓ 7 + 369054289 3895160724 ℓ 7 2 + 122945 L 4194 3 − 140945 50328 L 2 − 3839771 7926660 A + 224 18873 ℓ 11 ( ℓ 11 − ℓ 3 ) − 4675 227448 U − 685465 21401982 ℓ 23 ( ℓ 23 − ℓ 5 ) + 56735 150984 L ( ℓ 2 + 5 ℓ 3 ) + i π [ 60539053 499379580 − 5320 2097 3 + 4675 113724 ℓ 19 − 1646246209 973790181 ℓ 2 + 1199 12582 ℓ 3 + 234818800 973790181 ℓ 5 + 351389 3057426 ℓ 7 + 7280 6291 L ] + 966113 2671578 Ψ 1 + 128404699 599255496 Ψ 2 + 1024763 12229704 Ψ 3 + 1663823293 1298386908 Ψ 4 − 9605731379 1947580362 Ψ 5 − 1934137 14267988 Ψ 6 − 21508133974 973790181 Ψ 7 − 50970845 39746538 Ψ 8 − 187445795 3895160724 Ψ 9 + 4675 227448 Ψ 10 − 685465 21401982 Ψ 11 − 685465 21401982 Ψ 12 + 224 18873 Ψ 13 + 56735 75492 Ψ 14 + 12965144 139112883 Ψ 15 + 36551761 2774331 Ψ 16 − 238898 44037 Ψ 17 + 966113 1335789 Ψ 18 . (27) \begin{aligned}
c_{(2,2)}={}&\frac{810182}{660555}+\frac{11694988651}{6677418384}\pi^{2}-\frac{381162167}{33291972}\ell_{2}-\frac{1718267}{52995384}\ell_{2}\ell_{11}-\frac{37321050089}{2225806128}\ell_{2}^{2}\\
&+\frac{3427325}{21401982}\ell_{2}\ell_{23}-\frac{92832356}{13871655}\ell_{3}+\frac{166011001781}{7790321448}\ell_{2}\ell_{3}-\frac{161564465269}{15580642896}\ell_{3}^{2}+\frac{2668901}{1585332}\ell_{5}\\
&+\frac{1438024657}{2596773816}\ell_{2}\ell_{5}-\frac{9906289751}{7790321448}\ell_{3}\ell_{5}-\frac{337816123}{288530424}\ell_{5}^{2}+\frac{460283}{52995384}\ell_{7}\ell_{11}-\frac{388832957}{599255496}\ell_{2}\ell_{7}\\
&-\frac{933732461}{7790321448}\ell_{3}\ell_{7}-\frac{685465}{21401982}\ell_{5}\ell_{7}+\frac{369054289}{3895160724}\ell_{7}^{2}+\frac{122945L}{4194\sqrt{3}}-\frac{140945}{50328}L^{2}-\frac{3839771}{7926660}A\\
&+\frac{224}{18873}\ell_{11}(\ell_{11}-\ell_{3})-\frac{4675}{227448}U-\frac{685465}{21401982}\ell_{23}(\ell_{23}-\ell_{5})+\frac{56735}{150984}L(\ell_{2}+5\ell_{3})\\
&+i\pi\left[\frac{60539053}{499379580}-\frac{5320}{2097\sqrt{3}}+\frac{4675}{113724}\ell_{19}-\frac{1646246209}{973790181}\ell_{2}+\frac{1199}{12582}\ell_{3}+\frac{234818800}{973790181}\ell_{5}\right.\\
&\left.\qquad+\frac{351389}{3057426}\ell_{7}+\frac{7280}{6291}L\right]\\
&+\frac{966113}{2671578}\Psi_{1}+\frac{128404699}{599255496}\Psi_{2}+\frac{1024763}{12229704}\Psi_{3}+\frac{1663823293}{1298386908}\Psi_{4}\\
&-\frac{9605731379}{1947580362}\Psi_{5}-\frac{1934137}{14267988}\Psi_{6}-\frac{21508133974}{973790181}\Psi_{7}-\frac{50970845}{39746538}\Psi_{8}\\
&-\frac{187445795}{3895160724}\Psi_{9}+\frac{4675}{227448}\Psi_{10}-\frac{685465}{21401982}\Psi_{11}-\frac{685465}{21401982}\Psi_{12}\\
&+\frac{224}{18873}\Psi_{13}+\frac{56735}{75492}\Psi_{14}+\frac{12965144}{139112883}\Psi_{15}+\frac{36551761}{2774331}\Psi_{16}\\
&-\frac{238898}{44037}\Psi_{17}+\frac{966113}{1335789}\Psi_{18}. \tag*{(27)}
\end{aligned} c ( 2 , 2 ) = 660555 810182 + 6677418384 11694988651 π 2 − 33291972 381162167 ℓ 2 − 52995384 1718267 ℓ 2 ℓ 11 − 2225806128 37321050089 ℓ 2 2 + 21401982 3427325 ℓ 2 ℓ 23 − 13871655 92832356 ℓ 3 + 7790321448 166011001781 ℓ 2 ℓ 3 − 15580642896 161564465269 ℓ 3 2 + 1585332 2668901 ℓ 5 + 2596773816 1438024657 ℓ 2 ℓ 5 − 7790321448 9906289751 ℓ 3 ℓ 5 − 288530424 337816123 ℓ 5 2 + 52995384 460283 ℓ 7 ℓ 11 − 599255496 388832957 ℓ 2 ℓ 7 − 7790321448 933732461 ℓ 3 ℓ 7 − 21401982 685465 ℓ 5 ℓ 7 + 3895160724 369054289 ℓ 7 2 + 4194 3 122945 L − 50328 140945 L 2 − 7926660 3839771 A + 18873 224 ℓ 11 ( ℓ 11 − ℓ 3 ) − 227448 4675 U − 21401982 685465 ℓ 23 ( ℓ 23 − ℓ 5 ) + 150984 56735 L ( ℓ 2 + 5 ℓ 3 ) + iπ [ 499379580 60539053 − 2097 3 5320 + 113724 4675 ℓ 19 − 973790181 1646246209 ℓ 2 + 12582 1199 ℓ 3 + 973790181 234818800 ℓ 5 + 3057426 351389 ℓ 7 + 6291 7280 L ] + 2671578 966113 Ψ 1 + 599255496 128404699 Ψ 2 + 12229704 1024763 Ψ 3 + 1298386908 1663823293 Ψ 4 − 1947580362 9605731379 Ψ 5 − 14267988 1934137 Ψ 6 − 973790181 21508133974 Ψ 7 − 39746538 50970845 Ψ 8 − 3895160724 187445795 Ψ 9 + 227448 4675 Ψ 10 − 21401982 685465 Ψ 11 − 21401982 685465 Ψ 12 + 18873 224 Ψ 13 + 75492 56735 Ψ 14 + 139112883 12965144 Ψ 15 + 2774331 36551761 Ψ 16 − 44037 238898 Ψ 17 + 1335789 966113 Ψ 18 . (27)
Longitudinal tensor component. For F ( 2 , 3 ) ( 0 ) = − 46 27 F^{(0)}_{(2,3)}=-\frac{46}{27} F ( 2 , 3 ) ( 0 ) = − 27 46 ,
c ( 2 , 3 ) = 84379 39123 + 63129626233 45198466560 π 2 − 215690593 78871968 ℓ 2 − 60104669 2511025920 ℓ 2 ℓ 11 − 6579777773 105463088640 ℓ 2 2 + 1419715 12675852 ℓ 2 ℓ 23 − 79368337 32863320 ℓ 3 + 5076646284817 738241620480 ℓ 2 ℓ 3 − 3468300386959 738241620480 ℓ 3 2 + 942637 938952 ℓ 5 + 5061503627 5349576960 ℓ 2 ℓ 5 + 3349154077 369120810240 ℓ 3 ℓ 5 − 152119441 253169280 ℓ 5 2 + 145647581 2511025920 ℓ 7 ℓ 11 + 5378427043 5678781696 ℓ 2 ℓ 7 − 158781363239 369120810240 ℓ 3 ℓ 7 − 283943 12675852 ℓ 5 ℓ 7 − 6442551725 73824162048 ℓ 7 2 + 222817 L 19872 3 − 2960203 953856 L 2 − 45455099 9389520 A − 476 27945 ℓ 11 ( ℓ 11 − ℓ 3 ) − 894575 21835008 U − 283943 12675852 ℓ 23 ( ℓ 23 − ℓ 5 ) + 1304135 2861568 L ( ℓ 2 + 5 ℓ 3 ) + i π [ − 44489323 73942470 + 7 207 3 + 894575 10917504 ℓ 19 − 26477184683 23070050640 ℓ 2 + 12595 79488 ℓ 3 − 8983376405 18456040512 ℓ 5 + 7417979 9054180 ℓ 7 + 7 414 L ] + 3117851 7911540 Ψ 1 − 12752699843 28393908480 Ψ 2 + 3431165 57946752 Ψ 3 − 4968290597 61520135040 Ψ 4 − 225633278099 369120810240 Ψ 5 − 6491689 67604544 Ψ 6 − 856548988223 92280202560 Ψ 7 − 326596289 470817360 Ψ 8 + 28625338739 92280202560 Ψ 9 + 894575 21835008 Ψ 10 − 283943 12675852 Ψ 11 − 283943 12675852 Ψ 12 − 476 27945 Ψ 13 + 1304135 1430784 Ψ 14 − 2355344 205982595 Ψ 15 + 24758084 4107915 Ψ 16 − 974 945 Ψ 17 + 3117851 3955770 Ψ 18 . (28) \begin{aligned}
c_{(2,3)}={}&\frac{84379}{39123}+\frac{63129626233}{45198466560}\pi^{2}-\frac{215690593}{78871968}\ell_{2}-\frac{60104669}{2511025920}\ell_{2}\ell_{11}-\frac{6579777773}{105463088640}\ell_{2}^{2}\\
&+\frac{1419715}{12675852}\ell_{2}\ell_{23}-\frac{79368337}{32863320}\ell_{3}+\frac{5076646284817}{738241620480}\ell_{2}\ell_{3}-\frac{3468300386959}{738241620480}\ell_{3}^{2}+\frac{942637}{938952}\ell_{5}\\
&+\frac{5061503627}{5349576960}\ell_{2}\ell_{5}+\frac{3349154077}{369120810240}\ell_{3}\ell_{5}-\frac{152119441}{253169280}\ell_{5}^{2}+\frac{145647581}{2511025920}\ell_{7}\ell_{11}\\
&+\frac{5378427043}{5678781696}\ell_{2}\ell_{7}-\frac{158781363239}{369120810240}\ell_{3}\ell_{7}-\frac{283943}{12675852}\ell_{5}\ell_{7}-\frac{6442551725}{73824162048}\ell_{7}^{2}+\frac{222817L}{19872\sqrt{3}}\\
&-\frac{2960203}{953856}L^{2}-\frac{45455099}{9389520}A-\frac{476}{27945}\ell_{11}(\ell_{11}-\ell_{3})-\frac{894575}{21835008}U-\frac{283943}{12675852}\ell_{23}(\ell_{23}-\ell_{5})\\
&+\frac{1304135}{2861568}L(\ell_{2}+5\ell_{3})\\
&+i\pi\left[-\frac{44489323}{73942470}+\frac{7}{207\sqrt{3}}+\frac{894575}{10917504}\ell_{19}-\frac{26477184683}{23070050640}\ell_{2}+\frac{12595}{79488}\ell_{3}-\frac{8983376405}{18456040512}\ell_{5}\right.\\
&\left.\qquad+\frac{7417979}{9054180}\ell_{7}+\frac{7}{414}L\right] \\
&+\frac{3117851}{7911540}\Psi_{1}-\frac{12752699843}{28393908480}\Psi_{2}+\frac{3431165}{57946752}\Psi_{3}-\frac{4968290597}{61520135040}\Psi_{4}
-\frac{225633278099}{369120810240}\Psi_{5}-\frac{6491689}{67604544}\Psi_{6}-\frac{856548988223}{92280202560}\Psi_{7}-\frac{326596289}{470817360}\Psi_{8}
+\frac{28625338739}{92280202560}\Psi_{9}+\frac{894575}{21835008}\Psi_{10}-\frac{283943}{12675852}\Psi_{11}-\frac{283943}{12675852}\Psi_{12}
-\frac{476}{27945}\Psi_{13}+\frac{1304135}{1430784}\Psi_{14}-\frac{2355344}{205982595}\Psi_{15}+\frac{24758084}{4107915}\Psi_{16}-\frac{974}{945}\Psi_{17}
+\frac{3117851}{3955770}\Psi_{18}. \tag*{(28)}
\end{aligned} c ( 2 , 3 ) = 39123 84379 + 45198466560 63129626233 π 2 − 78871968 215690593 ℓ 2 − 2511025920 60104669 ℓ 2 ℓ 11 − 105463088640 6579777773 ℓ 2 2 + 12675852 1419715 ℓ 2 ℓ 23 − 32863320 79368337 ℓ 3 + 738241620480 5076646284817 ℓ 2 ℓ 3 − 738241620480 3468300386959 ℓ 3 2 + 938952 942637 ℓ 5 + 5349576960 5061503627 ℓ 2 ℓ 5 + 369120810240 3349154077 ℓ 3 ℓ 5 − 253169280 152119441 ℓ 5 2 + 2511025920 145647581 ℓ 7 ℓ 11 + 5678781696 5378427043 ℓ 2 ℓ 7 − 369120810240 158781363239 ℓ 3 ℓ 7 − 12675852 283943 ℓ 5 ℓ 7 − 73824162048 6442551725 ℓ 7 2 + 19872 3 222817 L − 953856 2960203 L 2 − 9389520 45455099 A − 27945 476 ℓ 11 ( ℓ 11 − ℓ 3 ) − 21835008 894575 U − 12675852 283943 ℓ 23 ( ℓ 23 − ℓ 5 ) + 2861568 1304135 L ( ℓ 2 + 5 ℓ 3 ) + iπ [ − 73942470 44489323 + 207 3 7 + 10917504 894575 ℓ 19 − 23070050640 26477184683 ℓ 2 + 79488 12595 ℓ 3 − 18456040512 8983376405 ℓ 5 + 9054180 7417979 ℓ 7 + 414 7 L ] + 7911540 3117851 Ψ 1 − 28393908480 12752699843 Ψ 2 + 57946752 3431165 Ψ 3 − 61520135040 4968290597 Ψ 4 − 369120810240 225633278099 Ψ 5 − 67604544 6491689 Ψ 6 − 92280202560 856548988223 Ψ 7 − 470817360 326596289 Ψ 8 + 92280202560 28625338739 Ψ 9 + 21835008 894575 Ψ 10 − 12675852 283943 Ψ 11 − 12675852 283943 Ψ 12 − 27945 476 Ψ 13 + 1430784 1304135 Ψ 14 − 205982595 2355344 Ψ 15 + 4107915 24758084 Ψ 16 − 945 974 Ψ 17 + 3955770 3117851 Ψ 18 . (28)
Numerical prescriptions and production interface
The coupling follows two-loop running with β 0 = 25 / 3 \beta_{0}=25/3 β 0 = 25/3 , β 1 = 154 / 3 \beta_{1}=154/3 β 1 = 154/3 , and α s ( 3 G e V ) = 0.249 \alpha_{s}(3\ \mathrm{GeV})=0.249 α s ( 3 GeV ) = 0.249 , using fixed n f = 4 n_{f}=4 n f = 4 without threshold switching. Mass scans keep the absolute coupling anchor, LDMEs, and matching ratios fixed while setting μ R = 2 m c \mu_{R}=2m_{c} μ R = 2 m c . No model-LDME mass dependence or binding corrections are included. Models I and II retain the labels of Ref. [2 ] , based on Refs. [45 , 46 ] . Spin-summed axial and tensor inputs are divided by three and five. The scalar LDME matrices in Table I are rank one up to rounding. The rounded entries are used directly, without a positive-semidefinite projection. The second tensor LDME is rounded from 0.01256 to 0.0126 GeV9 ^{9} 9 [28 ] . The relation ρ η = ρ ψ / 3 \rho_{\eta}=\rho_{\psi}/3 ρ η = ρ ψ /3 uses leading spin symmetry with unquantified velocity corrections.
For M = 6.847 G e V M=6.847\ \mathrm{GeV} M = 6.847 GeV , m c = M / 4 m_{c}=M/4 m c = M /4 , μ R = M \mu_{R}=M μ R = M , and the spin-summed ρ ψ = 1.32 G e V 3 \rho_{\psi}=1.32\ \mathrm{GeV}^{3} ρ ψ = 1.32 GeV 3 ,
α s ( M ) = 0.19131 , H 2 N L O = 6.125 × 10 − 4 G e V − 8 , Γ γ ψ = H 2 N L O ρ T , 2 f i x . (29) \alpha_{s}(M)=0.19131,\qquad H_{2}^{\mathrm{NLO}}=6.125\times10^{-4}\ \mathrm{GeV}^{-8},\qquad\Gamma_{\gamma\psi}=H_{2}^{\mathrm{NLO}}\rho_{T,2}^{\mathrm{fix}}. \tag*{(29)} α s ( M ) = 0.19131 , H 2 NLO = 6.125 × 1 0 − 4 GeV − 8 , Γ γ ψ = H 2 NLO ρ T , 2 fix . (29)
For ρ T , 2 f i x = 0.0144 G e V 9 \rho_{T,2}^{\mathrm{fix}}=0.0144\ \mathrm{GeV}^{9} ρ T , 2 fix = 0.0144 GeV 9 this gives Γ γ ψ = 8.8 × 10 − 3 M e V \Gamma_{\gamma\psi}=8.8\times10^{-3}\ \mathrm{MeV} Γ γ ψ = 8.8 × 1 0 − 3 MeV , an order of magnitude below the m c = 1.5 G e V m_{c}=1.5\ \mathrm{GeV} m c = 1.5 GeV benchmark width in Table II . The partonic prescription m c = M / 4 m_{c}=M/4 m c = M /4 does not reproduce both physical hadron masses. The production fit retains its published coupling and PDF inputs [39 ] . Sharing M M M and a central scale does not establish full compatibility. The tensor production current printed in Ref. [39 ] [cf. Eq. (6) therein] includes the symmetric projection, but the full symmetric traceless projector obeys ϵ i j Π i j , k l = ϵ k l ∗ \epsilon_{ij}\Pi^{ij,kl}=\epsilon^{*}_{kl} ϵ ij Π ij , k l = ϵ k l ∗ . Its factors of 1 / 2 1/2 1/2 therefore do not imply an overall current rescaling. The paired production coefficient and state convention still require verification. We therefore retain the unverified conversion ρ T , 2 p r o d = 5 ξ ρ T , 2 f i x \rho_{T,2}^{\mathrm{prod}}=5\xi\rho_{T,2}^{\mathrm{fix}} ρ T , 2 prod = 5 ξ ρ T , 2 fix , with ξ > 0 \xi>0 ξ > 0 , and count the decay spin average once. The conversion covers operator, state, and polarization conventions. Changing production inputs requires a compatible response and refit. The fit and radiative ratio must describe the same resolved state. Unknown production/decay correlations preclude a complete combined uncertainty.
Finite amplitudes and tensor polarization
At M T = 4 m c M_{T}=4m_{c} M T = 4 m c , M H = 2 m c M_{H}=2m_{c} M H = 2 m c , the physical amplitude and hard contractions are
M = e e c g s 4 m c 5 ρ H ∑ n , a [ F n a ( 0 ) + g s 2 F n a ( 1 ) ] L n B a , g s 2 = 4 π α s , \mathcal{M}=\frac{e e_{c}g_{s}^{4}}{m_{c}^{5}}\sqrt{\rho_{H}}\sum_{n,a}\left[F_{na}^{(0)}+g_{s}^{2}F_{na}^{(1)}\right]L_{n}B_{a},\qquad g_{s}^{2}=4\pi\alpha_{s}, M = m c 5 e e c g s 4 ρ H n , a ∑ [ F na ( 0 ) + g s 2 F na ( 1 ) ] L n B a , g s 2 = 4 π α s ,
h m n ( 0 ) = ∑ a b F n a ( 0 ) G a b F m b ( 0 ) ∗ , h m n ( 1 ) = ∑ a b ( F n a ( 1 ) G a b F m b ( 0 ) ∗ + F n a ( 0 ) G a b F m b ( 1 ) ∗ ) . (30) h_{mn}^{(0)}=\sum_{ab}F_{na}^{(0)}G_{ab}F_{mb}^{(0)*},\qquad h_{mn}^{(1)}=\sum_{ab}\left(F_{na}^{(1)}G_{ab}F_{mb}^{(0)*}+F_{na}^{(0)}G_{ab}F_{mb}^{(1)*}\right). \tag*{(30)} h mn ( 0 ) = ab ∑ F na ( 0 ) G ab F mb ( 0 ) ∗ , h mn ( 1 ) = ab ∑ ( F na ( 1 ) G ab F mb ( 0 ) ∗ + F na ( 0 ) G ab F mb ( 1 ) ∗ ) . (30)
The scalar structure is B 0 = ( g μ ν − P H μ k ν / ( P H ⋅ k ) ) ϵ γ μ ∗ ϵ H ν ∗ B_{0}=(g^{\mu\nu}-P_{H}^{\mu}k^{\nu}/(P_{H}\cdot k))\epsilon_{\gamma\mu}^{*}\epsilon_{H\nu}^{*} B 0 = ( g μν − P H μ k ν / ( P H ⋅ k )) ϵ γ μ ∗ ϵ H ν ∗ , and the axial structure is B 1 = − ϵ T ⋅ ϵ γ ∗ + ( ϵ T ⋅ k ) ( P T ⋅ ϵ γ ∗ ) / ( P T ⋅ k ) B_{1}=-\epsilon_{T}\cdot\epsilon_{\gamma}^{*}+(\epsilon_{T}\cdot k)(P_{T}\cdot\epsilon_{\gamma}^{*})/(P_{T}\cdot k) B 1 = − ϵ T ⋅ ϵ γ ∗ + ( ϵ T ⋅ k ) ( P T ⋅ ϵ γ ∗ ) / ( P T ⋅ k ) . Their metrics are G 0 = 2 G_{0}=2 G 0 = 2 and G 1 = 2 / 3 G_{1}=2/3 G 1 = 2/3 . The tensor has G 2 = diag ( 4 / 5 , 2 / 5 , 2 / 5 ) G_{2}=\operatorname{diag}(4/5,2/5,2/5) G 2 = diag ( 4/5 , 2/5 , 2/5 ) . These include the initial-spin average. Together with the two-body factor 3 / ( 256 π m c ) 3/(256\pi m_{c}) 3/ ( 256 π m c ) and the state conversion, they yield Eq. (1) of the Letter. The loop factor is included in F ( 1 ) F^{(1)} F ( 1 ) . The two scalar color components, the axial amplitude, and the three tensor polarization components are ordered as a = ( ( 0 , 3 ‾ ) , ( 0 , 6 ) , 1 , ( 2 , 1 ) , ( 2 , 2 ) , ( 2 , 3 ) ) a=((0,\overline{3}),(0,6),1,(2,1),(2,2),(2,3)) a = (( 0 , 3 ) , ( 0 , 6 ) , 1 , ( 2 , 1 ) , ( 2 , 2 ) , ( 2 , 3 )) ,
F a ( 1 ) ( r ) = F a ( 0 ) 4 π 2 [ c a + 25 3 ln r ] , F_{a}^{(1)}(r)=\frac{F_{a}^{(0)}}{4\pi^{2}}\left[c_{a}+\frac{25}{3}\ln r\right], F a ( 1 ) ( r ) = 4 π 2 F a ( 0 ) [ c a + 3 25 ln r ] ,
c a = s a [ P a + i π R a + 1 N a ∑ k = 1 19 b k a Ψ k ] , s a = ( 1 , 1 , 135 / 140608 , 1 , 1 , 1 ) . (31) c_{a}=s_{a}\left[P_{a}+i\pi R_{a}+\frac{1}{N_{a}}\sum_{k=1}^{19}b_{ka}\Psi_{k}\right],\qquad s_{a}=(1,1,135/140608,1,1,1). \tag*{(31)} c a = s a [ P a + iπ R a + N a 1 k = 1 ∑ 19 b k a Ψ k ] , s a = ( 1 , 1 , 135/140608 , 1 , 1 , 1 ) . (31)
The exact Born coefficients and rounded one-loop checkpoints at r = μ R / m c = 1 r=\mu_R/m_c=1 r = μ R / m c = 1 are
Table S16.
Tensor polarization basis. Choose the photon along + z +z + z in the tetraquark rest frame. In units of m c m_c m c , k = ( 3 / 2 , 0 , 0 , 3 / 2 ) k=(3/2,0,0,3/2) k = ( 3/2 , 0 , 0 , 3/2 ) and P ψ = ( 5 / 2 , 0 , 0 , − 3 / 2 ) P_\psi=(5/2,0,0,-3/2) P ψ = ( 5/2 , 0 , 0 , − 3/2 ) . With g = diag ( 1 , − 1 , − 1 , − 1 ) g=\operatorname{diag}(1,-1,-1,-1) g = diag ( 1 , − 1 , − 1 , − 1 ) , the vector polarizations are V x = ( 0 , 1 , 0 , 0 ) V_x=(0,1,0,0) V x = ( 0 , 1 , 0 , 0 ) , V y = ( 0 , 0 , 1 , 0 ) V_y=(0,0,1,0) V y = ( 0 , 0 , 1 , 0 ) , and V L = ( 3 / 4 , 0 , 0 , − 5 / 4 ) V_L=(3/4,0,0,-5/4) V L = ( 3/4 , 0 , 0 , − 5/4 ) . The photon uses V x , V y V_x,V_y V x , V y . For spatial unit vectors x , y , z x,y,z x , y , z , the normalized tensor basis is
S 1 = x x − y y 2 , S 2 = x x + y y − 2 z z 6 , S 3 = x y + y x 2 , S 4 = x z + z x 2 , S 5 = y z + z y 2 . (32) S_1=\frac{xx-yy}{\sqrt{2}},\quad S_2=\frac{xx+yy-2zz}{\sqrt{6}},\quad S_3=\frac{xy+yx}{\sqrt{2}},\quad S_4=\frac{xz+zx}{\sqrt{2}},\quad S_5=\frac{yz+zy}{\sqrt{2}}. \tag*{(32)} S 1 = 2 xx − y y , S 2 = 6 xx + y y − 2 z z , S 3 = 2 x y + y x , S 4 = 2 x z + z x , S 5 = 2 y z + z y . (32)
with outer products understood and zero temporal components. The three tensor entries of Eq. (S16) are the amplitudes ( a , b , c ) (a,b,c) ( a , b , c ) for ( S 1 , V x , γ x ) (S_1,V_x,\gamma_x) ( S 1 , V x , γ x ) , ( S 2 , V x , γ x ) (S_2,V_x,\gamma_x) ( S 2 , V x , γ x ) , and ( S 4 , V L , γ x ) (S_4,V_L,\gamma_x) ( S 4 , V L , γ x ) . All nonzero rows are
Table S18.
1 5 ∑ ∣ A ∣ 2 = 4 5 ∣ a ∣ 2 + 2 5 ∣ b ∣ 2 + 2 5 ∣ c ∣ 2 . (33) \frac{1}{5}\sum|\mathcal{A}|^2=\frac{4}{5}|a|^2+\frac{2}{5}|b|^2+\frac{2}{5}|c|^2. \tag*{(33)} 5 1 ∑ ∣ A ∣ 2 = 5 4 ∣ a ∣ 2 + 5 2 ∣ b ∣ 2 + 5 2 ∣ c ∣ 2 . (33)
The longitudinal part is 2 ∣ c ∣ 2 / 5 2|c|^2/5 2∣ c ∣ 2 /5 , giving the metrics in the Letter. At NLO each squared amplitude retains only Born–one-loop interference. The angular and mixed-sample relations then follow from Eqs. (7) , (8) , and (16) .
All exact elementary terms are specified compactly by
P a = 1 D a ∑ j = 1 26 p j a X j , R a = 1 E a ∑ j = 1 8 r j a Y j . (34) P_a=\frac{1}{D_a}\sum_{j=1}^{26}p_{ja}X_j,\qquad R_a=\frac{1}{E_a}\sum_{j=1}^{8}r_{ja}Y_j. \tag*{(34)} P a = D a 1 j = 1 ∑ 26 p j a X j , R a = E a 1 j = 1 ∑ 8 r j a Y j . (34)
with integer coefficients in Table SI. Let ℓ n = ln n \ell_n=\ln n ℓ n = ln n , L = ln ( 2 + 3 ) L=\ln(2+\sqrt{3}) L = ln ( 2 + 3 ) , A = ( π − arctan 15 ) / 15 A=(\pi-\arctan\sqrt{15})/\sqrt{15} A = ( π − arctan 15 ) / 15 , and U = ( ℓ 19 − ℓ 5 ) ( ℓ 19 + ℓ 11 ) + 4 ℓ 19 ( ℓ 2 − ℓ 3 ) U=(\ell_{19}-\ell_5)(\ell_{19}+\ell_{11})+4\ell_{19}(\ell_2-\ell_3) U = ( ℓ 19 − ℓ 5 ) ( ℓ 19 + ℓ 11 ) + 4 ℓ 19 ( ℓ 2 − ℓ 3 ) . The ordered bases are
( X 1 , … , X 9 ) = ( 1 , π 2 , ℓ 2 , ℓ 2 ℓ 11 , ℓ 2 2 , ℓ 2 ℓ 23 , ℓ 3 , ℓ 2 ℓ 3 , ℓ 3 2 ) , ( X 10 , … , X 18 ) = ( ℓ 5 , ℓ 2 ℓ 5 , ℓ 3 ℓ 5 , ℓ 5 2 , ℓ 7 ℓ 11 , ℓ 2 ℓ 7 , ℓ 3 ℓ 7 , ℓ 5 ℓ 7 , ℓ 7 2 ) , ( X 19 , … , X 26 ) = ( L / 3 , L 2 , A , ℓ 11 ( ℓ 11 − ℓ 3 ) , U , ℓ 23 ( ℓ 23 − ℓ 5 ) , L ( ℓ 2 + 5 ℓ 3 ) , ℓ 3 ℓ 23 ) , ( Y 1 , … , Y 8 ) = ( 1 , 1 / 3 , ℓ 19 , ℓ 2 , ℓ 3 , ℓ 5 , ℓ 7 , L ) . (35) \begin{aligned}
(X_1,\ldots,X_9)&=(1,\pi^2,\ell_2,\ell_2\ell_{11},\ell_2^2,\ell_2\ell_{23},\ell_3,\ell_2\ell_3,\ell_3^2),\\
(X_{10},\ldots,X_{18})&=(\ell_5,\ell_2\ell_5,\ell_3\ell_5,\ell_5^2,\ell_7\ell_{11},\ell_2\ell_7,\ell_3\ell_7,\ell_5\ell_7,\ell_7^2),\\
(X_{19},\ldots,X_{26})&=(L/\sqrt{3},L^2,A,\ell_{11}(\ell_{11}-\ell_3),U,\ell_{23}(\ell_{23}-\ell_5),L(\ell_2+5\ell_3),\ell_3\ell_{23}),\\
(Y_1,\ldots,Y_8)&=(1,1/\sqrt{3},\ell_{19},\ell_2,\ell_3,\ell_5,\ell_7,L). \tag*{(35)}
\end{aligned} ( X 1 , … , X 9 ) ( X 10 , … , X 18 ) ( X 19 , … , X 26 ) ( Y 1 , … , Y 8 ) = ( 1 , π 2 , ℓ 2 , ℓ 2 ℓ 11 , ℓ 2 2 , ℓ 2 ℓ 23 , ℓ 3 , ℓ 2 ℓ 3 , ℓ 3 2 ) , = ( ℓ 5 , ℓ 2 ℓ 5 , ℓ 3 ℓ 5 , ℓ 5 2 , ℓ 7 ℓ 11 , ℓ 2 ℓ 7 , ℓ 3 ℓ 7 , ℓ 5 ℓ 7 , ℓ 7 2 ) , = ( L / 3 , L 2 , A , ℓ 11 ( ℓ 11 − ℓ 3 ) , U , ℓ 23 ( ℓ 23 − ℓ 5 ) , L ( ℓ 2 + 5 ℓ 3 ) , ℓ 3 ℓ 23 ) , = ( 1 , 1/ 3 , ℓ 19 , ℓ 2 , ℓ 3 , ℓ 5 , ℓ 7 , L ) . (35)
Φ j = Re Li 2 ( z j ) (principal branch, Feynman + i 0 ) , \Phi_j=\operatorname{Re}\operatorname{Li}_2(z_j)\qquad\text{(principal branch, Feynman $+i0$)}, Φ j = Re Li 2 ( z j ) (principal branch, Feynman + i 0) ,
( z 1 , … , z 9 ) = ( 1 5 , 3 23 , 3 22 , 1 7 , 4 27 , 4 25 , 1 6 , 5 27 , 9 44 ) , (z_1,\ldots,z_9)=\left(\frac{1}{5},\frac{3}{23},\frac{3}{22},\frac{1}{7},\frac{4}{27},\frac{4}{25},\frac{1}{6},\frac{5}{27},\frac{9}{44}\right), ( z 1 , … , z 9 ) = ( 5 1 , 23 3 , 22 3 , 7 1 , 27 4 , 25 4 , 6 1 , 27 5 , 44 9 ) ,
( z 10 , … , z 18 ) = ( 5 24 , 3 14 , 3 23 , 5 4 , 1 11 , 3 32 , 9 10 , 19 63 , 1 3 ) , (z_{10},\ldots,z_{18})=\left(\frac{5}{24},\frac{3}{14},\frac{3}{23},\frac{5}{4},\frac{1}{11},\frac{3}{32},\frac{9}{10},\frac{19}{63},\frac{1}{3}\right), ( z 10 , … , z 18 ) = ( 24 5 , 14 3 , 23 3 , 4 5 , 11 1 , 32 3 , 10 9 , 63 19 , 3 1 ) ,
( z 19 , … , z 25 ) = ( 11 32 , 19 54 , 23 63 , 9 23 , 2 5 , 3 7 , 9 19 ) , (z_{19},\ldots,z_{25})=\left(\frac{11}{32},\frac{19}{54},\frac{23}{63},\frac{9}{23},\frac{2}{5},\frac{3}{7},\frac{9}{19}\right), ( z 19 , … , z 25 ) = ( 32 11 , 54 19 , 63 23 , 23 9 , 5 2 , 7 3 , 19 9 ) ,
( z 26 , … , z 29 ) = ( 7 3 − 4 3 , 2 3 − 1 3 , 21 − 12 3 , 3 3 − 5 ) , (z_{26},\ldots,z_{29})=\left(\frac{7}{3}-\frac{4}{\sqrt{3}},\frac{2}{3}-\frac{1}{\sqrt{3}},21-12\sqrt{3},3\sqrt{3}-5\right), ( z 26 , … , z 29 ) = ( 3 7 − 3 4 , 3 2 − 3 1 , 21 − 12 3 , 3 3 − 5 ) ,
( z 30 , … , z 36 ) = ( 50 95 + 9 i 15 , 140 95 + 9 i 15 , 20 5 + 3 i 15 , 10 5 + i 15 , 20 25 + i 15 , 30 25 + i 15 , − 10 5 + 3 i 15 ) . (36) (z_{30},\ldots,z_{36})=\left(\frac{50}{95+9i\sqrt{15}},\frac{140}{95+9i\sqrt{15}},\frac{20}{5+3i\sqrt{15}},\frac{10}{5+i\sqrt{15}},\frac{20}{25+i\sqrt{15}},\frac{30}{25+i\sqrt{15}},\frac{-10}{5+3i\sqrt{15}}\right). \tag*{(36)} ( z 30 , … , z 36 ) = ( 95 + 9 i 15 50 , 95 + 9 i 15 140 , 5 + 3 i 15 20 , 5 + i 15 10 , 25 + i 15 20 , 25 + i 15 30 , 5 + 3 i 15 − 10 ) . (36)
The combinations entering Table SII are
( Ψ 1 , … , Ψ 9 ) = ( Φ 1 , Φ 4 , Φ 6 , Φ 7 , Φ 13 , Φ 16 , Φ 18 , Φ 23 , Φ 24 ) , (\Psi_1,\ldots,\Psi_9)=(\Phi_1,\Phi_4,\Phi_6,\Phi_7,\Phi_{13},\Phi_{16},\Phi_{18},\Phi_{23},\Phi_{24}), ( Ψ 1 , … , Ψ 9 ) = ( Φ 1 , Φ 4 , Φ 6 , Φ 7 , Φ 13 , Φ 16 , Φ 18 , Φ 23 , Φ 24 ) ,
Ψ 10 = Φ 3 + Φ 8 − Φ 9 + Φ 10 − Φ 17 − Φ 20 − 2 Φ 25 , \Psi_{10}=\Phi_3+\Phi_8-\Phi_9+\Phi_{10}-\Phi_{17}-\Phi_{20}-2\Phi_{25}, Ψ 10 = Φ 3 + Φ 8 − Φ 9 + Φ 10 − Φ 17 − Φ 20 − 2 Φ 25 ,
Ψ 11 = Φ 12 + Φ 15 , Ψ 12 = − Φ 21 + Φ 22 , Ψ 13 = Φ 11 + 2 Φ 14 − Φ 19 , \Psi_{11}=\Phi_{12}+\Phi_{15},\qquad\Psi_{12}=-\Phi_{21}+\Phi_{22},\qquad\Psi_{13}=\Phi_{11}+2\Phi_{14}-\Phi_{19}, Ψ 11 = Φ 12 + Φ 15 , Ψ 12 = − Φ 21 + Φ 22 , Ψ 13 = Φ 11 + 2 Φ 14 − Φ 19 ,
Ψ 14 = Φ 26 − Φ 27 − Φ 28 − Φ 29 , Ψ 15 = − Φ 30 + Φ 31 , Ψ 16 = Φ 32 − Φ 36 , \Psi_{14}=\Phi_{26}-\Phi_{27}-\Phi_{28}-\Phi_{29},\qquad\Psi_{15}=-\Phi_{30}+\Phi_{31},\qquad\Psi_{16}=\Phi_{32}-\Phi_{36}, Ψ 14 = Φ 26 − Φ 27 − Φ 28 − Φ 29 , Ψ 15 = − Φ 30 + Φ 31 , Ψ 16 = Φ 32 − Φ 36 ,
Ψ 17 = Φ 33 , Ψ 18 = Φ 34 − Φ 35 , Ψ 19 = Φ 2 + Φ 5 . (37) \Psi_{17}=\Phi_{33},\qquad\Psi_{18}=\Phi_{34}-\Phi_{35},\qquad\Psi_{19}=\Phi_2+\Phi_5. \tag*{(37)} Ψ 17 = Φ 33 , Ψ 18 = Φ 34 − Φ 35 , Ψ 19 = Φ 2 + Φ 5 . (37)
TABLE SI. Exact integer coefficients for the elementary terms in Eq. (34) . The upper and lower blocks specify P a P_a P a and R a R_a R a , respectively.
Table SI.
Table SII. Exact integer weights of the dilogarithm combinations in Eq. (31) , in the same component order as Table SI.