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Light-Front Quark-Scalar-Diquark Model

Updated 9 July 2026
  • The light-front quark-scalar-diquark model is a two-body valence framework where a proton is described by an active quark and a spectator scalar diquark with dynamics encoded in LFWFs.
  • It utilizes both soft-wall AdS/QCD-inspired profiles and spectator formulations to compute key distributions such as PDFs, TMDs, GPDs, and GTMDs, ensuring consistency with experimental data.
  • The model enables analytic derivations of overlap representations, evolution equations, and spatial imaging of nucleon structure, while highlighting its validity as a low-scale, valence-focused framework.

Searching arXiv for recent and foundational papers on the light-front quark–scalar-diquark model. arXiv search query: "light-front quark scalar diquark model proton TMD GPD GTMD" The light-front quark-scalar-diquark model is a two-body valence description of the proton in which an active quark is accompanied by a spectator scalar diquark, and the nonperturbative dynamics are encoded in light-front wave functions (LFWFs). In the cited literature, this framework appears both in soft-wall AdS/QCD-inspired form and in spectator formulations with a point-like quark-diquark vertex, and it is used to compute PDFs, TMDs, GPDs, GTMDs, Wigner distributions, gravitational form factors, and higher-twist correlators (Maji et al., 2016, Maji et al., 2017, Kaur et al., 2018).

1. Effective degrees of freedom and model definition

In its minimal form, the model truncates the proton Fock expansion to a single active quark plus a scalar diquark spectator. For the scalar channel, the diquark has spin $0$ and helicity λS=0\lambda_S=0, while the proton retains helicity Jz=±12J^z=\pm \tfrac12 and the quark helicity takes λq=±12\lambda_q=\pm \tfrac12 (Maji et al., 2017, Kaur et al., 2018). The basic state content is therefore

qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,

with xx the quark light-cone momentum fraction and pp_\perp its transverse momentum (Sharma et al., 2023).

A broader spin-flavor decomposition often embeds the scalar channel into a quark-diquark basis containing both scalar and axial-vector spectators. In the SU(4) basis used for nucleon modeling,

P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,

with the scalar sector isolated by retaining only uS0±|u\,S^0\rangle^\pm or, in a pure scalar-diquark treatment, by setting the scalar weight CS=1C_S=1 (Maji et al., 2016, Sharma et al., 2023).

The model is also used in a spectator realization in which the proton is treated as a quark of mass λS=0\lambda_S=00 coupled to a scalar diquark of mass λS=0\lambda_S=01 through a point-like vertex of strength λS=0\lambda_S=02. In that formulation, no explicit Lagrangian is required for practical calculations because the dynamics are carried by the LFWFs themselves, although an effective Yukawa-type interaction λS=0\lambda_S=03 is a standard underlying picture (Kaur et al., 2018, Sharma et al., 2023).

2. Light-front state expansion and helicity structure

For the scalar-diquark sector, the proton state is expanded as

λS=0\lambda_S=04

with

λS=0\lambda_S=05

In the soft-wall AdS/QCD-based construction, the four nonzero helicity amplitudes are (Maji et al., 2017, Maji et al., 2016)

λS=0\lambda_S=06

λS=0\lambda_S=07

A different but closely related spectator parameterization writes the scalar-channel spinor components as (Kaur et al., 2018, Sharma et al., 2023)

λS=0\lambda_S=08

with λS=0\lambda_S=09. In both implementations, the spin dependence is carried by explicit transverse-momentum prefactors and the radial dependence is isolated in one or two scalar profile functions.

Normalization is imposed sector by sector. A typical condition is

Jz=±12J^z=\pm \tfrac120

or its equivalent with the light-front measure written explicitly (Maji et al., 2017, Maji et al., 2016). In the AdS/QCD-based nucleon model, the free two-body invariant mass is

Jz=±12J^z=\pm \tfrac121

with Jz=±12J^z=\pm \tfrac122 in the massless-quark version of the model (Maji et al., 2016).

3. Radial wave-function ansätze and parameterizations

The best-known implementation uses soft-wall AdS/QCD-inspired profile functions. In momentum space,

Jz=±12J^z=\pm \tfrac123

with Jz=±12J^z=\pm \tfrac124; the strict AdS/QCD limit corresponds to Jz=±12J^z=\pm \tfrac125 and Jz=±12J^z=\pm \tfrac126 (Maji et al., 2017, Maji et al., 2016). The parameters Jz=±12J^z=\pm \tfrac127 are fitted either to unpolarized PDFs or to nucleon form-factor data, depending on the analysis (Maji et al., 2017, Maji et al., 2016).

A spectator alternative employs a single scalar profile

Jz=±12J^z=\pm \tfrac128

together with constituent masses and couplings fitted to form factors (Kaur et al., 2018). Higher-twist analyses also use an AdS/QCD-motivated Gaussian form,

Jz=±12J^z=\pm \tfrac129

with λq=±12\lambda_q=\pm \tfrac120 fixed by λq=±12\lambda_q=\pm \tfrac121 (Sharma et al., 2023).

Implementation Radial input Representative parameters
Soft-wall AdS/QCD nucleon model Two profiles λq=±12\lambda_q=\pm \tfrac122 with Gaussian λq=±12\lambda_q=\pm \tfrac123-dependence and powers λq=±12\lambda_q=\pm \tfrac124 λq=±12\lambda_q=\pm \tfrac125; at λq=±12\lambda_q=\pm \tfrac126: for λq=±12\lambda_q=\pm \tfrac127, λq=±12\lambda_q=\pm \tfrac128, λq=±12\lambda_q=\pm \tfrac129, qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,0, qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,1, qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,2, qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,3 (Maji et al., 2016, Sharma et al., 2023)
TMD-focused AdS/QCD scalar sector Same functional form, fitted to PDFs at a different initial scale qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,4; at qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,5: qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,6, qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,7, qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,8, qλq(xP+,p),S((1x)P+,p),|q^{\lambda_q}(xP^+,p_\perp),\,S((1-x)P^+,-p_\perp)\rangle,9, xx0 (Maji et al., 2017)
Spectator scalar-diquark model Single propagator-like profile xx1 xx2, xx3, xx4 (Kaur et al., 2018)

A more dynamical realization arises in the light-front Faddeev-Bethe-Salpeter approach, where a contact two-quark interaction produces a scalar-diquark subamplitude xx5, the proton valence wave function is obtained by symmetrizing a bachelor-quark vertex xx6, and model parameters are tuned to reproduce the proton mass and Dirac form factor (Ydrefors et al., 2022). This suggests a route from phenomenological quark-diquark LFWFs to a bound-state construction in which the scalar diquark is not merely an external spectator parameter.

4. Overlap representations for PDFs and TMDs

The scalar-diquark model is particularly suited to overlap calculations. For collinear PDFs, the unpolarized, helicity, and transversity distributions are obtained by integrating LFWF overlaps over transverse momentum. In the scalar channel these take the form (Maji et al., 2018, Maji et al., 2016)

xx7

xx8

and xx9 from the corresponding chiral-odd overlap. In the nucleon model based on soft-wall AdS/QCD LFWFs, the helicity and transversity distributions were reported to agree with phenomenological fits, axial and tensor charges were reported to agree with experimental or phenomenological extractions, and the Soffer bound was verified numerically at all scales studied (Maji et al., 2016, Maji et al., 2018).

At leading twist and for T-even TMDs, the scalar sector yields explicit overlap expressions. Representative examples are (Maji et al., 2017)

pp_\perp0

pp_\perp1

pp_\perp2

The remaining leading-twist T-even functions pp_\perp3, pp_\perp4, pp_\perp5, and pp_\perp6 follow from off-diagonal helicity overlaps (Maji et al., 2017).

A notable numerical result is the approximate pp_\perp7-pp_\perp8 factorization,

pp_\perp9

with

P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,0

The AdS/QCD scalar-diquark model does not factorize analytically into a product of pure P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,1- and P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,2-functions, but the Gaussian ansatz was found to be realized to very good approximation (Maji et al., 2017).

5. Generalized distributions, spatial imaging, and orbital structure

The same overlap machinery extends to GPDs, GTMDs, and Wigner distributions. For chiral-odd GPDs, the scalar-diquark model provides overlap formulas for P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,3, P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,4, P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,5, and P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,6 at both zero and nonzero skewness, with active-quark momentum arguments shifted as

P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,7

and similarly for P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,8 and P;±=CSuS0±+CVuA0±+CVVdA1±,|P;\pm\rangle = C_S\,|u\,S^0\rangle^\pm + C_V\,|u\,A^0\rangle^\pm + C_{VV}\,|d\,A^1\rangle^\pm,9 (Chakrabarti et al., 2015). Their two-dimensional Fourier transforms define impact-parameter-space GPDs, and a one-dimensional Fourier transform in uS0±|u\,S^0\rangle^\pm0 introduces a longitudinal impact coordinate uS0±|u\,S^0\rangle^\pm1. In the scalar model, uS0±|u\,S^0\rangle^\pm2, uS0±|u\,S^0\rangle^\pm3, and uS0±|u\,S^0\rangle^\pm4 show diffraction-like patterns in uS0±|u\,S^0\rangle^\pm5-space, whereas uS0±|u\,S^0\rangle^\pm6 does not display a pronounced diffraction pattern because it is odd in uS0±|u\,S^0\rangle^\pm7 (Chakrabarti et al., 2015).

Phase-space imaging is developed further through Wigner distributions and GTMDs. The twist-2 Wigner operator is

uS0±|u\,S^0\rangle^\pm8

and its Fourier transform in uS0±|u\,S^0\rangle^\pm9 yields

CS=1C_S=10

Combining proton and quark polarizations generates 16 independent twist-2 Wigner distributions, while the GTMD decomposition contains 16 complex functions of

CS=1C_S=11

of which only 10 survive at CS=1C_S=12 (Kaur et al., 2018). In the scalar-diquark sector, CS=1C_S=13 and CS=1C_S=14 are circularly symmetric in both CS=1C_S=15 and CS=1C_S=16; CS=1C_S=17 and CS=1C_S=18 display dipolar patterns and a quadrupole in mixed space; and CS=1C_S=19 at λS=0\lambda_S=000 is directly related to quark orbital angular momentum (Kaur et al., 2018).

Momentum-space densities also reveal transverse-shape information. In the scalar model,

λS=0\lambda_S=001

with λS=0\lambda_S=002. The transverse-shape relation

λS=0\lambda_S=003

shows non-spherical, “pretzel” distortions driven by λS=0\lambda_S=004 (Maji et al., 2017).

For energy-momentum structure, the scalar-diquark LFWFs generate gravitational form factors through overlaps with λS=0\lambda_S=005: λS=0\lambda_S=006 Their two-dimensional Fourier transforms define the longitudinal momentum density λS=0\lambda_S=007 and the angular momentum density λS=0\lambda_S=008 in the transverse plane (Kumar et al., 2017).

T-odd extensions require an explicit final-state interaction. In the holographic scalar-diquark model with one-gluon-exchange phase,

λS=0\lambda_S=009

the T-odd GTMDs λS=0\lambda_S=010 and λS=0\lambda_S=011 emerge from the imaginary part of λS=0\lambda_S=012, and in the forward limit λS=0\lambda_S=013 they reduce to the Sivers and Boer-Mulders functions (Chakrabarti et al., 2019).

6. Evolution, higher-twist sectors, and limitations

The scalar-diquark model is defined at a low hadronic scale and then evolved. For integrated PDFs, ordinary DGLAP evolution is applied, either directly or through a simulated DGLAP procedure in which the profile parameters λS=0\lambda_S=014, λS=0\lambda_S=015, and λS=0\lambda_S=016 acquire scale dependence (Maji et al., 2016, Maji et al., 2018). For TMDs, a Collins-Soper-Sterman-type evolution is written in λS=0\lambda_S=017-space: λS=0\lambda_S=018 with

λS=0\lambda_S=019

followed by the Fourier transform back to momentum space (Maji et al., 2017).

Beyond leading twist, the model remains analytically tractable. For T-even twist-3 TMDs, the scalar sector yields explicit formulas for λS=0\lambda_S=020, λS=0\lambda_S=021, λS=0\lambda_S=022, λS=0\lambda_S=023, λS=0\lambda_S=024, λS=0\lambda_S=025, λS=0\lambda_S=026, and λS=0\lambda_S=027. Because explicit quark-gluon interaction terms are absent and the gauge link is set to unity for T-even observables, Wandzura-Wilczek-type relations become exact in the model, including

λS=0\lambda_S=028

for the corresponding twist-3 functions (Sharma et al., 2023).

At twist 4, the scalar-diquark sector gives closed expressions for λS=0\lambda_S=029, λS=0\lambda_S=030, λS=0\lambda_S=031, λS=0\lambda_S=032, λS=0\lambda_S=033, and λS=0\lambda_S=034, with model relations tying them to leading-twist TMDs. The simplest is

λS=0\lambda_S=035

and analogous formulas relate λS=0\lambda_S=036, λS=0\lambda_S=037, λS=0\lambda_S=038, λS=0\lambda_S=039, and λS=0\lambda_S=040 to λS=0\lambda_S=041, λS=0\lambda_S=042, λS=0\lambda_S=043, λS=0\lambda_S=044, λS=0\lambda_S=045, and λS=0\lambda_S=046 (Sharma et al., 2023). For the twist-4 T-even function λS=0\lambda_S=047, the scalar channel gives

λS=0\lambda_S=048

with reported numerical averages

λS=0\lambda_S=049

(Sharma et al., 2023). Twist-4 GTMDs have also been parameterized in the scalar sector, and their TMD limit reproduces the previously derived twist-4 T-even TMDs (Sharma et al., 2023).

The main limitations are tied to the same simplifications that make the model analytic. Many calculations are valence-only and retain only the minimal quark-diquark Fock sector (Maji et al., 2016, Ydrefors et al., 2022). In the chiral-odd GPD construction, the analysis is restricted to the DGLAP region λS=0\lambda_S=050, and all valence GPDs vanish at λS=0\lambda_S=051 because no explicit ERBL contribution is included (Chakrabarti et al., 2015). T-odd observables are absent unless an explicit final-state interaction phase is introduced (Chakrabarti et al., 2019). In the light-front Faddeev-Bethe-Salpeter approach, the evolved non-polarized valence PDFs suggest that higher Fock components beyond the valence one are needed for comparison with NNPDF4.0 (Ydrefors et al., 2022). A plausible implication is that the light-front quark-scalar-diquark model is most reliable as a controlled low-scale valence framework and as a laboratory for analytic relations among light-front distributions, rather than as a complete description of proton structure at all λS=0\lambda_S=052 and all twists.

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