b -like depicted ure of our s, through ent with Physics Letters B 581 (2004) 75–81 www.elsevier.com/locate/physlet Electromagnetic form factor of the pion in the space- and time regions within the front-form dynamics J.P.B.C. de Meloa, T. Fredericob, E. Pacec, G. Salmèd a Instituto de Física Teórica, Universidade Estadual Paulista, 01405-900 São Paulo, SP, Brazil b Departamento de Física, Instituto Tecnológico da Aeronáutica, Centro Técnico Aeroespacial, 12.228-900 São José dos Campos, São Paulo, Brazil c Dipartimento di Fisica, Università di Roma “Tor Vergata” and Istituto Nazionale di Fisica Nucleare, Sezione Tor Vergata, Via della Ricerca Scientifica 1, I-00133 Roma, Italy d Istituto Nazionale di Fisica Nucleare, Sezione Roma I, P.le A. Moro 2, I-00185 Roma, Italy Received 10 November 2003; accepted 28 November 2003 Editor: P.V. Landshoff Abstract The pion electromagnetic form factor is calculated in the space- and time-like regions from−10 (GeV/c)2 up to 10(GeV/c)2, within a front-form model. The dressed photon vertex where a photon decays in a quark–antiquark pair is generalizing the vector meson dominance ansatz, by means of the vector meson vertex functions. An important feat model is the description of the on-mass-shell vertex functions in the valence sector, for the pion and the vector meson the front-form wave functions obtained within a realistic quark model. The theoretical results show an excellent agreem the data in the space-like region, while in the time-like region the description is quite encouraging. 2003 Elsevier B.V. All rights reserved. PACS:12.39.Ki; 12.40.Vv; 13.40.Gp; 14.40.Aq Keywords:Relativistic quark model; Vector-meson dominance; Electromagnetic form factors; Pion ] ber lec- g l- e- a c- in art- le ate er- ce rtex In the framework of the front-form dynamics [1 (see, e.g., [2,3] for extensive reviews) a large num of papers has been devoted to the study of the e tromagnetic form factor of the pion, mostly dealin with the space-like (SL) region [4–10]. To our know edge, in the front-form quantization the elastic tim like (TL) form factor has only been calculated in E-mail address:salmeg@roma1.infn.it (G. Salmè). 0370-2693/$ – see front matter 2003 Elsevier B.V. All rights reserved doi:10.1016/j.physletb.2003.11.072 scalar field theory model forqQ̄ mesons with point- like vertices [11]. In this Letter, the pion electromagnetic form fa tor is evaluated within the front-form dynamics, both the SL and the TL regions, by using as a st ing point the Mandelstam formula [12] for the triang diagrams of Figs. 1 and 2. Our aim is to investig the possibility of describing the photon–hadron int action by applying the vector meson (VM) dominan ansatz (see, e.g., [13]) at the level of the photon ve function. . http://www.elsevier.com/locate/physletb 76 J.P.B.C. de Melo et al. / Physics Letters B 581 (2004) 75–81 n arks on the nt Fig. 1. Diagrammatic representation of the pion elastic form factor forq+ > 0 vs. the globalx+-time flow. Diagram (a) (0� −k+ � P+ π ) is the contribution of the valence component in the initial pion wave function. Diagram (b) (P+ π � −k+ � P ′+ π ) is the non-valence contributio to the pion form factor. Both processes contain the contribution from the dressed photon vertex. The crosses correspond to the qu k− shell (see text). Fig. 2. Diagrammatic representation of the photon decay (γ ∗ → ππ̄ ) vs. the globalx+-time flow. Diagrams (a) and (b) correspond to differe x+-time orderings. The crosses correspond to the quarks on thek− shell (see text). r ra- re- (b), ses r y a ul- g- pli- by te e., een nt ses ion k; to ta; 2 the ude ere ht it The virtual processes where a quark absorbs o diates a pion are present in both the SL and the TL gions (see the square blobs in Figs. 1(b) and 2(a), respectively) [10]. In a recent study of decay proces within the front-form dynamics [14] the amplitude fo the pion emission from a quark was described b pseudoscalar coupling of quark and pion fields, m tiplied by a constant. Here, we just follow this su gestion, and use a constant to parametrize the am tudes for the radiative pion absorption or emission a quark. In order to simplify our calculations, we evalua the pion form factor for a vanishing pion mass, i. at the chiral limit. As a consequence, the gap betw the SL region and the TL one (i.e., betweenq2 � 0 and q2 � 4m2 π ) disappears. Our starting point is the Mandelstam covaria expression [12] of the amplitudes for the proces πγ ∗ → π ′, or γ ∗ → ππ ′, where the mesonπ ′ is a pion in the elastic case or an antipion in the product process. For the TL region one has (see Fig. 2) jµ = −ıe2m 2 f 2 π Nc × ∫ d4k (2π)4 Λ̄π ′(k− Pπ ,Pπ ′)Λ̄π (k,Pπ) (1) × Tr [ S(k −Pπ)γ 5S(k − q)Γ µ(k, q)S(k)γ 5], where Nc = 3 is the number of colors;S(p) = 1 /p−m+ıε , with m the mass of the constituent quar qµ is the virtual photon momentum;̄Λπ(k,Pπ ) the vertex function for the pion, which will be assumed be a symmetric function of the two quark momen P µ π and Pµ π ′ are the pion momenta. The factor stems from isospin algebra. The “bar” notation on vertex function means that the associated amplit is the solution of the Bethe–Salpeter equation wh the two-body irreducible kernel is placed on the rig of the amplitude, while in the conventional case J.P.B.C. de Melo et al. / Physics Letters B 581 (2004) 75–81 77 gation. Fig. 3. Dressed photon vertex. The double-wiggly lines represent the front-form Green function describing the vector-meson propa de y en i- er- ith ual ate by rm is it 7]. tor o- - c- t of f nt n- he n - rm ith e, - x i- is placed on the left of the Bethe–Salpeter amplitu [15]. For the SL regionPµπ should be replaced b −Pµπ , and then the initial pion vertex should be writt asΛπ(−k,Pπ)= Λ̄π (k,−Pπ). The central assumption of the Letter is our m croscopical description of the dressed photon v tex, Γ µ(k, q), in the processes where a photon w q+ > 0 decays in a quark–antiquark pair at eq light-front times. In these processes we approxim the plus component of the photon vertex, dressed the interaction between theqq̄ pair, as follows (see Fig. 3) Γ +(k, q)= √ 2 ∑ n,λ [ ελ · V̂n(k, k− q)]Λn(k,Pn) (2)× [ε+λ ]∗fV n [q2 −M2 n + ıMnΓn(q2)] , wherefV n is the decay constant of thenth vector me- son in a virtual photon (see below),Mn the corre- sponding mass,Pn the VM total momentum (Pµn ≡ {P− n = (|q⊥|2 +M2 n)/q +,Pn⊥ = q⊥,P+ n = q+}; note that at the production vertex, see Fig. 3, the front-fo three-momentum is conserved), andελ the VM polar- ization. The total decay width in the denominator assumed to be vanishing in the SL region, while is equal toΓn(q2) = Γnq 2/M2 n in the TL one [16]. For a detailed discussion of Eq. (2) see Ref. [1 In Eq. (2) the sum runs over all the possible vec mesons, and the quantity[ελ · V̂n(k, k − q)]Λn(k, q) is the VM vertex function. The momentum comp nent,Λn(k,Pn), of the VM vertex function, evalu ated on the quark mass shell (i.e., fork− = k−on = (|k⊥|2 +m2)/k+), will be related for 0< k+
0. Both in the SL and the TL regions, the integrati on k− in Eq. (1) is performed with the assumptio that: (i) Λπ(k,Pπ ) does not diverge in the comple plane k− for |k−| → ∞, and (ii) the contributions of the possible singularities ofΛπ(k,Pπ) can be neglected. Also the contributions of the poles ink− of the photon vertex function,Γ +(k, q), are supposed to be negligible. Then, in the SL case, wherePµ π ′ = P µ π + qµ, the current matrix elementjµ becomes the sum o two contributions, corresponding to the diagrams Fig. 1(a) and (b), respectively,jµSL = j (I)µ SL + j (II)µ SL [9]. The contributionj (I)µSL has the integration o k+ constrained by−P+ π � k+ � 0, and j (II)µSL has the integration onk+ in the interval 0< k+ < q+. The valence component of the pion contributes j (I)µ SL only, while j (II)µSL is the contribution of the pair-production mechanism from an incoming virtu photon withq+ > 0 [7–9,20,22,23]. In the SL cas we adopt a frame wherePπ⊥ = Pπ ′⊥ = 0, and we obtain P+ π = q+(−1 + √ 1− 4m2 π/q 2 )/2. Then, in the limit mπ → 0 the longitudinal momenta of th pions areP+ π = 0 andP+ π ′ = q+. Therefore only the contribution of the pair-production mechanism,j (II)µSL , survives (Fig. 1(b)). As shown in Ref. [9], in a fram whereq+ > 0, j (II)µSL (q2) dominates the form factor a high momentum transfer. Moreover, it turns out tha the model of Ref. [9] the momentum region, whe j (II)µ SL (q2) starts to dominate the form factor, ten toward zero if the pion mass is artificially decreas in agreement with our present discussion. In the TL case, one hasPµ π ′ ≡ Pµπ̄ , qµ = Pµπ +Pµπ̄ . The integration range onk+ for the matrix elemen of the current,jµ, can be decomposed in two inte vals, 0< k+ < P+ π andP+ π < k + < q+, and thenjµTL becomes the sum of two contributions, correspo ing to differentx+-time orderings (see diagrams Fig. 2(a) and (b), respectively). In the final state theππ̄ pair we make the purely longitudinal choic Pπ̄⊥ = −Pπ⊥ = 0. Then, one obtainsP+ π /q + = xπ = (1 ± √ 1− 4m2 π/q 2 )2. In the limitmπ → 0, one has xπ = 1 or 0. Analogously to the SL case, in wh follows we adopt the choicexπ = 0, which implies P+ π = 0 andP+ π̄ = q+. Therefore only the contribu tion corresponding to the diagram of Fig. 2(b) s vives. The form factor of the pion in the TL and in th SL regions can be obtained from the plus com nent of the proper current matrix elements:jµTL = 〈ππ̄ |q̄γ µq|0〉 = (P µ π − P µ π̄ )Fπ (q 2), and j µ SL = 〈π |q̄γ µq|π ′〉 = (Pµπ + Pµ π ′ )Fπ(q2) Since in the limit mπ → 0 the form factor receives contributions on from the diagrams of Figs. 1(b) and 2(b), where photon decays in aqq̄ pair, one can apply our appro imation for the plus component of the dressed pho vertex (2), both in the SL and in the TL regions. Th the matrix elementj+ can be written as a sum ov the vector mesons and consequently the form fa becomes (6)Fπ ( q2) = ∑ n fV n q2 −M2 n + ıMnΓn(q2) g+ V n ( q2), J.P.B.C. de Melo et al. / Physics Letters B 581 (2004) 75–81 79 nt it ding rent rm e ce o- rm n t m n- )), stant me orp- in - n nt n s . f a thin el nic nel. er- lo– e- ates l en in- tate st nt). be - is s ent or tal whereg+ V n(q 2), for q2 > 0, is the form factor for the VM decay in a pair of pions. Each VM contribution to the sum (6) is invaria under kinematical front-form boosts and therefore can be evaluated in the rest frame of the correspon resonance. In this frame one hasq+ =Mn andq− = q2/Mn for the photon andP+ n = P− n = Mn for the vector meson. This means that we choose a diffe frame for each resonance (always withq⊥ = 0), but all the frames are related by kinematical front-fo boosts along thez axis to each other, and to the fram where q+ = −q− = √−q2 (qz = √−q2 ), adopted in previous analyses of the SL region [9,21]. Sin in our reference frame one has ∑ λ[ε+λ (Pn)]∗ελ(Pn) · Γ̂n = [ε+z (Pn)]∗εz(Pn) · Γ̂n = −Γ̂nz, we obtain from Eqs. (1)–(3) g+ V n ( q2) = Nc 8π3 √ 2 P+ π̄ m fπ q+∫ 0 dk+ (k+)2(q+ − k+) × ∫ dk⊥ Tr [[ ΘzΛ̄π(k;Pπ) ] (k−=q−+(k−q)−on) ] ×ψ ∗̄ π ( k+,k⊥;P+ π̄ ,Pπ̄⊥ ) × [M2 n −M2 0(k +,k⊥;q+,q⊥)] [q2 −M2 0(k +,k⊥;q+,q⊥)+ iε] (7)×ψn ( k+,k⊥;q+,q⊥ ) , where Θz = Vnz(k, k − q)γ 5[/k − /Pπ + m]γ 5. To obtain Eq. (7) we have first performed thek− in- tegration, and then we have related[Λ̄π̄ (k − Pπ, Pπ̄ )](k−=q−+(k−q)−on) in the valence sector to the m mentum component of the corresponding front-fo pion wave function through the following equatio (see Eq. (3)) ψπ ( k+,k⊥;P+ π ,Pπ⊥ ) (8)= m fπ P+ π [Λπ(k,Pπ)][k−=k−on] [m2 π −M2 0(k +,k⊥;P+ π ,Pπ⊥)] . As for the VM vertex function, we do no distinguish between[Λπ(k,Pπ )][k−=k−on] and [Λπ(k, Pπ )][k−=P− π −(Pπ−k)−on], in the range 0< k+
0 quark– antiquark pairs. Our calculation of the pion form factor contain a very small set of parameters: (i) the constitu quark mass, (ii) the oscillator strength,ω, and (iii) the VM widths, Γn, for Mn > 2.150 GeV. The up-down quark mass is fixed at 0.265 GeV [25]. F the first four vector mesons the known experimen 80 J.P.B.C. de Melo et al. / Physics Letters B 581 (2004) 75–81 28]. M us- or ne, ss re gle e- ta al- ns ay be he e, ve uare nd lue h ns- ized 4 om ntly he nc- nly l tum the ely. de- TL ons at tent ure atz l ive m st for the ta, r ate n ella masses and widths are used in the calculations [ However, the non-trivialq2 dependence ofg+ V n(q 2) in our microscopical model implies a shift of the V masses, with respect to the values obtained by ing Breit–Wigner functions with constant values f g+ V n. As a consequence, the value of theρ meson mass is moved in our model from the usual o 0.775 to 0.750 GeV. For the other VM, the ma values corresponding to the model of Ref. [25] a used, while for the unknown widths we use a sin valueΓn = 0.15 GeV, which presents the best agre ment with the compilation of the experimental da of Ref. [29]. We consider 20 resonances in our c culations to obtain stability of the results up toq2 = 10 (GeV/c)2. The oscillator strength is fixed atω= 1.39 GeV2 [27]. The values of the coupling constants,fV n, are evaluated from the model VM wave functio through Eq. (5). The corresponding partial dec width [19] Γe+e− = 8πα2f 2 V n/(3M 3 n), where α is the fine structure constant, can be considered to in agreement with the experimental data for theρ meson (Γ th e+e− = 6.37 keV,Γ exp e+e− = 6.77± 0.32 keV), and for ρ′ and ρ′′ (Γ th e+e− = 1.61 keV andΓ th e+e− = 1.23 keV, respectively) to be consistent with t experimental lower bounds (Γ exp e+e− > 2.30± 0.5 keV andΓ exp e+e− > 0.18± 0.1 keV, respectively) [28]. We perform two sets of calculations. In the first on we use the asymptotic form of the pion valence wa function, obtained withΛπ(k,Pπ ) = 1 in Eq. (8); in the second one, we use the eigenstate of the sq mass operator of Refs. [24,25]. The pion radius fou for the asymptotic wave function israsymp π = 0.65 fm and for the full model wave function isrmodel π = 0.67 fm, to be compared with the experimental va r exp π = 0.67± 0.02 fm [30]. The good agreement wit the experimental form factor at low momentum tra fers is expected, since we have built-in the general ρ-meson dominance. The calculated pion form factor is shown in Fig. in a wide region of square momentum transfers, fr −10 (GeV/c)2 up to 10(GeV/c)2. A general quali- tative agreement with the data is seen, independe of the detailed form of the pion wave function. T results obtained with the asymptotic pion wave fu tion and the full model, present some differences o above 3(GeV/c)2. The SL form factor is notably wel described, except near−10 (GeV/c)2. It has to be Fig. 4. Pion electromagnetic form factor vs. the square momen transfer q2. Dashed and solid lines are the results with asymptotic (see text) and the full pion wave function, respectiv Experimental data are from Ref. [29]. stressed that the heights of the TL bumps directly pend on the calculated values offV n andg+ V n. The introduction ofω-like [31] andφ-like mesons could improve the description of the data in the region. For instance, the introduction of these mes could smooth out the oscillations of the form factor high momentum transfer values. However, a consis dynamical description ofω-like andφ-like states is far beyond the present work, and we leave it for fut developments of the model. Our results show that a VM dominance ans for the (dressed photon)-(qq̄) vertex, within a mode consistent with the meson spectrum, is able to g a unified description of the SL and TL pion for factor. Using the experimental widths for the fir four vector mesons and a single free parameter the unknown widths of the other vector mesons, model gives a qualitative agreement with the TL da while in the SL region it works surprisingly well. Ou VM dominance model can be also applied to evalu other observables, as theγ ∗ → πγ form factor or the nucleon TL form factor. Acknowledgements This work was partially supported by the Brazilia agencies CNPq and FAPESP and by Ministero d J.P.B.C. de Melo et al. / Physics Letters B 581 (2004) 75–81 81 .F. di of or . 98) 88) 357 ys- 59 1) hys. 1. 65) . ara- ucl. ucl. ; 50; 04; 2) 02) 02) 44 v. Ricerca Scientifica e Tecnologica. J.P.B.C.M. and T acknowledge the hospitality of the Dipartimento Fisica, Università di Roma “Tor Vergata” and Istituto Nazionale di Fisica Nucleare, Sezione T Vergata and Sezione Roma I. References [1] P.A.M. Dirac, Rev. Mod. Phys. 21 (1949) 392. [2] B.D. Keister, W.N. Polizou, Adv. Nucl. Phys. 20 (1991) 225 [3] S.J. Brodsky, H.C. Pauli, S.S. Pinsky, Phys. Rep. 301 (19 299. [4] P.L. Chung, F. Coester, W.N. Polizou, Phys. Lett. B 205 (19 545. [5] T. Frederico, G.A. Miller, Phys. Rev. D 45 (1992) 4207; T. Frederico, G.A. Miller, Phys. Rev. D 50 (1994) 210. [6] F. Cardarelli, E. Pace, G. Salmè, S. Simula, Phys. Lett. B (1995) 267; F. Cardarelli, et al., Phys. Rev. D 53 (1996) 6682. [7] H.W.L. Naus, J.P.C. de Melo, T. Frederico, Few-Body S tems 24 (1998) 99; J.P.C. de Melo, H.W.L. Naus, T. Frederico, Phys. Rev. C (1999) 2278. [8] B.L.G. Bakker, H.-M. Choi, C.-R. Ji, Phys. Rev. D 63 (200 074014. [9] J.P.B.C. de Melo, T. Frederico, E. Pace, G. Salmè, Nucl. P A 707 (2002) 399. [10] C.-W. Hwang, Phys. Rev. D 64 (2001) 034011. [11] H.-M. Choi, C.-R. Ji, Nucl. Phys. A 679 (2001) 735. [12] S. Mandelstan, Proc. R. Soc. (London) A 233 (1956) 248. [13] H.B. O’Connell, et al., Prog. Part. Nucl. Phys. 39 (1997) 20 [14] C.-R. Ji, H.-M. Choi, Phys. Lett. B 513 (2001) 330. [15] D. Lurié, A.J. Macfarlane, Y. Takahashi, Phys. Rev. 140 (19 1091. [16] C.J. Gounaris, J.J. Sakurai, Phys. Rev. Lett. 21 (1968) 244 [17] J.P.B.C. de Melo, T. Frederico, E. Pace, G. Salmè, in prep tion. [18] W. Jaus, Phys. Rev. D 41 (1990) 3394. [19] W. Jaus, Phys. Rev. D 44 (1991) 2851; W. Jaus, Phys. Rev. D 60 (1999) 054026; W. Jaus, Phys. Rev. D 63 (2001) 053009. [20] J.P.B.C. de Melo, J.H.O. Sales, T. Frederico, P.U. Sauer, N Phys. A 631 (1998) 574c; J.P.B.C. de Melo, T. Frederico, H.W.L. Naus, P.U. Sauer, N Phys. A 660 (1999) 219. [21] F.M. Lev, E. Pace, G. Salmè, Nucl. Phys. A 641 (1998) 229 F.M. Lev, E. Pace, G. Salmè, Phys. Rev. Lett. 83 (1999) 52 F.M. Lev, E. Pace, G. Salmè, Phys. Rev. C 62 (2000) 0640 E. Pace, G. Salmè, Nucl. Phys. A 689 (2001) 411. [22] M. Sawicki, Phys. Rev. D 44 (1991) 433; M. Sawicki, Phys. Rev. D 46 (1992) 474. [23] B.L.G. Bakker, H.-M. Choi, C.-R. Ji, Phys. Rev. D 65 (200 116001. [24] T. Frederico, H.-C. Pauli, Phys. Rev. D 64 (2001) 054007. [25] T. Frederico, H.-C. Pauli, S.-G. Zhou, Phys. Rev. D 66 (20 054007; T. Frederico, H.-C. Pauli, S.-G. Zhou, Phys. Rev. D 66 (20 116011. [26] F. Iachello, N.C. Mukhopadhyay, L. Zhang, Phys. Rev. D (1991) 898. [27] A.V. Anisovitch, V.V. Anisovich, A.V. Sarantsev, Phys. Re D 62 (2000) 051502(R). [28] K. Hagiwara, et al., Phys. Rev. D 66 (2002) 010001. [29] R. Baldini, et al., Eur. Phys. J. C 11 (1999) 709; R. Baldini, et al., Nucl. Phys. A 666–667 (2000) 3; R. Baldini, et al., private communication. [30] S.R. Amendolia, et al., Phys. Lett. B 178 (1986) 116. [31] S. Gardner, H.B. O’Connell, Phys. Rev. D 57 (1998) 2716. Electromagnetic form factor of the pion in the space- and time-like regions within the front-form dynamics Acknowledgements References