A covariant model for the negative parity resonances of the nucleon

Journal of Physics: Conference Series PAPER OPEN ACCESS A covariant model for the negative parity resonances of the nucleon To cite this article: G. Ramalho 6 J. Phys.: Conf. Ser. 76 45 View the article online for updates and enhancements. Related content - A solution to the old puzzle of + resonances above the + Hoyle state in C A new analysis with complexscaled 3 OCM S Ohtsubo, Y Fukushima, M Kamimura et al. - Towards a covariant model for cosmic selfacceleration Alexey S. Koshelev and Theodore N. Tomaras - Electric Magnetic duality in (linearized) Hoava Lifshitz gravity Ignacio Cortese and J Antonio García This content was downloaded from IP address 46.3.93.6 on //7 at 5:4

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 A covariant model for the negative parity resonances of the nucleon G. Ramalho International Institute of Physics, Federal University of Rio Grande do Norte, Av. Odilon Gomes de Lima 7, Capim Macio, Natal-RN 5978-4, Brazil E-mail: gilberto.ramalho3@gmail.com Abstract. We present a model for the γ N N helicity amplitudes, where N is the nucleon and N is a negative parity nucleon excitation, member of the SU(6)-multiplet [7, ]. The model combines the results from the single quark transition model for the helicity amplitudes with the results of the covariant spectator quark model for the γ N N (535) and γ N N (5) transitions. With the knowledge of the amplitudes A / and A 3/ for those transitions we calculate three independent coefficients defined by the single quark transition model and make predictions for the helicity amplitudes associated with the γ N N (65), γ N N (7), γ N (6), and γ N (7) transitions. In order to facilitate the comparison with future experimental data at high Q, we provide also simple parametrizations for the amplitudes, compatible with the expected falloff at high Q.. Introduction One of the challenges in the modern physics is the description of the internal structure of the baryons and mesons. The electromagnetic structure of the nucleon N and the nucleon resonances N can be accessed through the γ N N reactions, which depend of the (photon) momentum transfer squared Q [,, 3, 4]. The data associated with those transitions are represented in terms of helicity amplitudes and have been collected in the recent years at Jefferson Lab, with increasing Q []. The new data demands the development of theoretical models based on the underlying structure of quarks and quark-antiquark states (mesons) [, ]. Those models may be used to guide future experiments as the ones planned for the Jlab GeV upgrade, particularly for resonances in the second and third resonance region [energy W =.4.8 GeV] (see figure ) []. In that region there are several resonances N from the multiplet [7, ] of SU(6) O(3), characterized by a negative parity [, 5, 6]. According with the single quark transition model (SQTM), when the electromagnetic interaction is the result of the photon coupling with just one quark, the helicity amplitudes of the [7, ] members depend only on three independent functions of Q : A,B and C [6, 7]. In this work we use the covariant spectator quark model [, 7, 8] developed for the γ N N (5) and γ N N (535) transitions, also members of [7, ], to calculate those functions [9, ]. Since the covariant spectator quark model breaks the SU()-flavor symmetry, we restrict our study to reactions with proton targets (average on the SQTM coefficients) [7]. Later on, with the knowledge of the functions A,B, and C we predict the helicity amplitudes for transitions associated with the remaining members of the multiplet [7, ] [7]. Content from this work may be used under the terms of the Creative Commons Attribution 3. licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Published under licence by Ltd

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 σ T 6 5 4 3 (3) P 33 γ p -> n π + N(44) P N(5) D 3 4 6 8 W (MeV) N(535) S (6) P 33 N(65) S N(7) P Q = GeV Figure. Representation of the γp nπ + cross section. The graph define the 3 resonance regions. The vertical lines represent resonant states described by the covariant spectator quark model. At red we indicate the states studded in this work. At blue are the states used as input.. Covariant Spectator Quark Model The covariant spectator quark model is based on the formalism of the covariant spectator theory []. In the covariant spectator quark model, baryons are treated as three-quark systems. The baryon wave functions are derived from the quark states according with the SU(6) O(3) symmetry group. A quark is off-mass-shell, and free to interact with the photon fields, and other two quarks are on-mass-shell [8,, 3, 4]. Integrating over the quark-pair degrees of freedom we reduce the baryon to a quark-diquark system, where the diquark can be represented as an on-mass-shell spectator particle with an effective mass of m D [8, 9,,, 4]. The electromagnetic interaction with the baryons is described by the photon coupling with the constituent quarks in the relativistic impulse approximation. The quark electromagnetic structure is represented in terms of the quark form factors parametrized by a vector meson dominance mechanism[8, 4, 5]. The parametrization of the quark current was calibrated in the studies of the nucleon form factors data [8], by the lattice QCD data for the decuplet baryon [4], and encodes effectively the gluon and quark-antiquark substructure of the constituent quarks. The quark current has the general form [8, 4] j µ q(q ) = j (Q )γ µ +j (Q ) iσµν q ν M, () where M is the nucleon mass and j i (i =,) are the Dirac and Pauli quark form factors. In the SU()-flavor sector the functions j i can also be decomposed into the isoscalar (f i+ ) and the isovector (f i ) components: j i = 6 f i+ + f i τ 3, where τ 3 acts on the isospin states of baryons (nucleon or resonance). The details can be found in [8, 3, 4]. When the nucleon wave function (Ψ N ) and the resonance wave function (Ψ R ) are both expressed in terms of the single quark and quark-pair states, the transition current in impulse approximation as can be written [8,, 4] J µ = 3 Ψ R (P +,k)j qψ µ N (P,k), () Γ k where P,P +, and k are the nucleon, the resonance, and the diquark momenta respectively. In the previous equation the index Γ labels the possible states of the intermediate diquark polarizations, the factor 3 takes account of the contributions from the other quark pairs by the symmetry, and the integration symbol represents the covariant integration over the diquark

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 on-mass-shell momentum. In the study of inelastic reactions we replace γ µ γ µ qqµ in q equation (). This procedure ensures the conservation of the transition current and it is equivalent to the use of the Landau prescription [7, 9, ]. Using equation (), we can express the transition current in terms of the quark electromagnetic form factor f i± (i =,) and the radial wave functions ψ N and ψ R [8, 9, ]. The radial wave functions are scalar functions that depend on the baryon (P) and diquark (k) momenta and parametrize the momentum distributions of the quark-diquark systems. From the transition current we can extract the form factors and the helicity transition amplitudes, defined in the rest frame of the resonance (final state), for the reaction under study [,, 9, ]. There are however some processes such as the meson exchanged between the different quarks inside the baryon, which cannot be reduced to simple diagrams with quark dressing. Those processes are regarded as arising from a meson exchanged between the different quarks inside the baryon and can be classified as meson cloud corrections to the hadronic reactions [, 3, 6]. The covariant spectator quark model was used already in the study of several nucleon excitations including isospin / systems N(4),N(5),N(535),N(7) [9,, 7] and the isospin 3/ systems [8, 9, ]. The model generalized to the SU(3)-flavor sector was also used to study the octet and decuplet baryons as well as transitions between baryons with strange quarks [6, ]. In figure the position of the nucleon excitations are represented and compared with the bumps of the cross sections. Based on the parametrization of the quark current () in term of the vector meson dominance mechanism, the model was extended to the lattice QCD regime (heavy pions and no meson cloud) [5, 8], to the nuclear medium [3] and to the timelike regime []. The model was also used to study the nucleon deep inelastic scattering [8, 3] and the axial structure of the octet baryon [4]. 3. Results for N(535) and N(5) For the study of the states N(535) ( ) and N(5) ( 3 ) it is necessary to specify the shape of the radial wave function of the nucleon and resonant states. The radial wave function can be represented using the dimensionless variable χ = (P k) (M B m D ) M B m D, where M B is the mass of the baryon B. We choose in particular [ N ψ N (P,k) = m D (β +χ)(β +χ), ψ N R(P,k) = m D (β +χ) β +χ λ ] R, (3) β j +χ where N,N are normalization constants, β,β and β j are momentum range parameters in units M B m D. We use β j = β 3 for N(535) and β j = β 4 for N(5). Those parameters are fixed by a fit to the the large Q data [7, ]. The coefficient λ R is determined by an orthogonality condition between the nucleon and the state R. In the following we will use also the spectroscopic notation to represent the states N(535) (or S) and N(535) (or D3). In addition we use M S and M D to represent the S and D3 masses, respectively. 3.. State N(535) From the study of [7, 9] we conclude that we can write the amplitude A / for the N(535) state in terms of the Dirac transition form factor (F ). The final result is then A / = 3 F S (f + +f τ 3 )I S cosθ S, I S (Q k z ) = k k ψ S(P +,k)ψ N (P,k), (4) where F S = e and I S is a covariant integral calculated on the S rest frame. (M S +M) +Q 8M(M S M ) The result (4) is valid for large Q since only valence quark effects are considered and it is the consequence of the observation that the Pauli transition form factor (F ) vanishes for Q.5 3

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 A / ( -3 GeV -/ ) - -4-6 -8 3 4 5 A 3/ ( -3 GeV -/ ) 8 5 9 6 3 Meson cloud 3 4 5 Figure. Results for the resonance N(5). The amplitude A 3/ the result of meson cloud effects. was no contributions from valence quarks. Data from CLAS [3]. GeV, which is interpreted as the consequence of the cancellation between valence quark and meson cloud effects [9]. In this work we updated the model from [9] using the radial wave function ψ R given by equation (3), in order to ensure the exact orthogonality between nucleon and N(535) states. In the process we introduce a new parameter (β 3 ) that is adjusted by the large Q data (no meson cloud) [7]. 3.. State N(5) The model for from [] can be used to calculate the electromagnetic transition form factors for the γ N N(5) transition, including the magnetic dipole G M and the electric quadrupole G E form factors, based in the effects of the valence quarks. One obtain then G E = G M, where G M = R(f + +f τ 3 )I D3 + M D +M M (f + +f τ 3 )I D3. (5) 3 M (MD M) +Q 3 M D M In the equations R = (M D, and I +M) +Q D3 (Q ) = k z k k ψ D3(P +,k)ψ N (P,k) is the new invariant integral defined at the resonance rest frame. The result G M + G E = is interesting, since with is consistent with the expected QCD behavior for large Q, but it is inconsistent with the data at low Q, that shows a significant magnitude for the amplitude A 3/ (G M + G E ), near Q = [, 7, ]. In general, quark models predict small contributions for A 3/ ( 4%) [7, ]. There are however indications that the effects of the meson cloud contribution dominate the amplitude, as supported by the calculation from EBAC at Jefferson Lab[5]. Based on that information we represent the helicity amplitudes as A / = F D G M + 4 F DG π 4, A 3/ = 3 4 F DG π 4, (6) where F D = e MD M (M D +M) +Q M M D +M M. In the equations (6), G π 4 is a function that is not determined by the covariant spectator quark model (that predicts G π 4 ) and parametrize the amplitude A 3/ assuming the dominance of the pion/meson cloud effects. The function G π 4 is fitted to the data with a model inspired on the pion and meson cloud contributions for the γ N transition [7,, ]. The results from the amplitudes A / (valence quark) and A 3/ (meson cloud) are presented on figure. 4. Single Quark Transition Model The combination of the wave functions of a baryon (three-quark system) given by SU(6) O(3) group and the description of electromagnetic interaction in impulse approximation leads to the so-called single quark transition model (SQTM) [6, 6]. In this context single means that only one quark couples with the photon. In these conditions the SQTM can be used to parametrize the transition current between two multiplets, in an operational form that includes only four independent terms, with coefficients exclusively dependent of Q. 4

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 State Amplitude N(535) A / 6 (A+B C)cosθ S N(5) A / 6 (A B C)cosθ D A 3/ 6 (A+C)cosθ D N(65) A / 6 (A+B C)sinθ S (6) A / 8 (3A B +C) N(7) A / 6 (A B C)sinθ D A 3/ 6 (A+C)sinθ D (7) A / 8 (3A+B +C) A 3/ 6 (3A C) 6 Table. Amplitudes A / and A 3/ estimated by SQTM for the proton targets (N = p) [6, 7]. The angle θ S is the mixing angle associated with the N states (θ S = 3 ). The angle θ D is the mixing angle associated with the N 3 states (θs = 6 ). A (Q ) 4 3 3 4 5 6 7 8 9 B (Q ) 5 5 5 3 4 5 6 7 8 9 C (Q ) 4 3-3 4 5 6 7 8 9 Figure 3. Results for the coefficients A,B and C for the model (dashed-line) and model (solid-line). In the model : C = A. In particular, the SQTM can be used to parametrize the γ N N transitions, where N is a N (isospin /) or a (isospin 3/) state from the [7, ] multiplet, in terms on three independent functions of Q : A,B, and C [6, 6]. The relations between the functions A,B, and C andtheamplitudesarepresentedinthetable. Usingtheresultsfortheγ N N(535)and γ N N(5) amplitudes, respectively A S /, AD3 /, and AD3 3/ in the spectroscopic notation, we can write A = AS / + A D3 / cosθ + 6A D3 3/, B = AS / A D3 S cosθ S C = AS / cosθ S A D3 / + 6A D3 3/. (7) Once the coefficients A,B, and C, are determined, we can predict the amplitudes for the the transitions γ N N(65), γ N N(7), γ N (6) and γ N (7). Based on the amplitudes used in the calibration we expect the estimates to be accurate for Q GeV [7]. From the relations (7) we can conclude in the limit where no meson cloud is considered (A D3 3/ = ) one has C = A. That case defines the our model, and only the parameters A and B are necessary (since C = A). When we have a (non-zero) parametrization for A D3 3/, we define the model. Using the parametrization discussed in the previous section we obtain the results for A,B and C presented in figure 3. /, 5

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 A / ( -3 GeV -/ ) 8 6 4 N(65) CLAS- CLAS- MAID 3 4 5 A / ( -3 GeV -/ ) -5 - -5 - -5-3 N(7) CLAS- -35 3 4 5 A 3/ ( -3 GeV -/ ) 3 - - N(7) CLAS- -3 3 4 5 Figure 4. Results for the resonances N(65) and N(7). Model (dashed-line) and Model (solid-line). Data from [3, 7, 8, 9]. A / ( -3 GeV -/ ) 8 6 4 (7) CLAS- CLAS- MAID 3 4 5 Q (GeV ) A 3/ ( -3 GeV -/ ) 4 8 6 4 (7) CLAS- MAID NSTAR 3 4 5 Figure 5. Results for the resonance (7). Model : dashed-line; Model : solid line. Data from [3, 7, 8, 9, 3]. 5. Results With the results of the functions A,B and C, represented in figure 3, for the model (dashedline) and model (solid-line), it is possible to calculate the amplitudes for the remaining transition of the multiplet [7, ] using the relations from table. The results are compared with data from CLAS (CLAS-) [3, 7], preliminary data from CLAS (CLAS-) [8], data from the MAID analysis [4], data presented in proceedings and workshops (NSTAR) [, 6] and data for Q = [9]. The results for the states N(65) and N(7) are on figure 4. In the graphs, we can see that the model gives a better description for the amplitude A 3/ (the model gives A 3/ ). Both models have the same result for N(65) which describe well the MAID data for Q GeV. The results for the states are presented in the figures 5 and 6, respectively for (7) and (65). For (7) we can see the models have very similar results for Q GeV. As for (65) only the model has a good description of the data for Q GeV. The model predicts negative values for the amplitude A /. We can conclude then, in general that only the model gives a good description of the data, particularly for Q GeV. Note that the model is the model that takes into account the meson cloud effects (A D3 3/ ). Based on the expected behavior for large Q given by A / /Q 3 and A / /Q 5 in accordance with perturbative QCD arguments [3], we parametrize the amplitudes as ( ) Λ A / (Q 3/ ) Λ ) = D Λ +Q, A 3/(Q 5/ ) = D( Λ +Q, (8) for Q 5 GeV. In the previous expression D and Λ are respectively coefficients and cutoffs dependent on the amplitude and on the resonance. The results of the parametrizations are in table. Those results may be useful to compare with future experiments at large Q as the ones predicted for the Jlab- GeV upgrade []. 6

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 A / ( -3 GeV -/ ) 8 6 4 (6) CLAS- CLAS- MAID - 3 4 5 Figure 6. Results for (6). Note that only the model (solid-line) has the correct sign. S / ( -3 GeV -/ ) - - S / data F(Q )x( A / data) -3 3 4 5 6 Figure 7. Relation between the amplitudes A / and S / for the γ N N(535) transition. F(Q ) = +τ M S M M S Q. State Amplitude D( 3 GeV / ) Λ (GeV ) N(65) A / 68.9 3.35 (6) A /...... N(7) A / 8.5.8 A 3/ 4.36 3.6 Table. Parameters from the high Q parametrization given by equations (8). (7) A / 39..69 A 3/ 4.5 8.4 For the amplitude A / associated with the (6) state it was not possible to find a parametrization consistent the power 3/ as in equation (8). This is because, for that particular amplitude, there is a partial cancellation between the leading terms (on /Q 3 ) of our A,B and C parametrization due to the difference of sign between the amplitudes A S / and AD3 / used in the determination of the SQTM coefficients (see dashed-line on figure 6). As consequence the amplitude A / for the state (6) is dominated by next leading terms (on /Q 5 ) or contributions due to meson cloud effects (A D3 3/ ). It is clear in figure 6 that when we neglect the contributions from A D3 3/ the result correspondent to the model (dashed-line), is almost zero. This result shows that in the γ N (6) transition, contrarily to what is usually expected, there is a strong suppression of the valence quark effects for Q = GeV. For a more detailed discussion see [7]. A simple parametrization of the amplitudes A / derived from our model is A / = 77. ( Λ Λ +Q ) 5/ in units 3 GeV /, with Λ = GeV. Note in particular the power 5/, instead of the expected 3/. Another interesting prediction relatively to the helicity amplitudes of baryon with negative parity is the correlation between the amplitudes A / and S / associated with the γ N N(535) transition. The consequence of the experimental result, F, observed for Q.5 +τ M S M GeV is that we can write in that regime S / = M S Q A /, where τ = The correlation between the amplitudes is shown on figure 7. Q (M S +M) [9]. 7

Journal of Physics: Conference Series 76 (6) 45 doi:.88/74-6596/76/4/45 6. Summary and conclusions We combine the frameworks of the covariant spectator quark model and the single quark transition model in order to make predictions for the helicity amplitudes associated with negative parity resonances in the region of masses W =.5.8 GeV. The predictions are expected to be valid for Q GeV. Simple parametrizations for the amplitudes are calculated to facilitate the comparison with future experiments for Q 5 GeV. Contrarily to what it was expected, in some transitions, like for the resonances N(535) and (6), the valence quark effects are not dominant in the region Q = GeV. Acknowledgments The author thanks Kumar Gupta for comments and suggestions. The author was supported by the Brazilian Ministry of Science, Technology and Innovation (MCTI-Brazil). References [] Aznauryan I G, Bashir A, Braun V, Brodsky S J, Burkert V D, Chang L, Chen C, El-Bennich B et al. 3 Int. J. Mod. Phys. E, 335. [] Aznauryan I G and Burkert V D Prog. Part. Nucl. Phys. 67,. [3] Aznauryan I G et al. [CLAS Collaboration] 9 Phys. Rev. C 8, 553. [4] Drechsel D, Kamalov S S, Tiator L 7 Eur. Phys. J. A 34, 69; Tiator T, Drechsel D, Kamalov S S, Vanderhaeghen M Eur. Phys. J. ST 98, 4. [5] Capstick S, Roberts W Prog. Part. Nucl. Phys. 45, S4. [6] Burkert V D, De Vita R, Battaglieri M, Ripani M and Mokeev V 3 Phys. Rev. C 67, 354. [7] Ramalho G 4 Phys. Rev. D 9, 33. [8] Gross F, Ramalho G and Peña M T 8 Phys. Rev. C 77, 5. [9] Ramalho G and Peña M T Phys. Rev. D 84, 337; Ramalho G and Tsushima K Phys. Rev. D 84, 53. [] Ramalho G and Peña M T 4 Phys. Rev. D 89, 946. [] Gross F 969 Phys. Rev. 86, 448; Stadler A, Gross F and Frank M 997 Phys. Rev. C 56, 396. [] Gross F, Ramalho G and Peña M T Phys. Rev. D 85, 935. [3] Ramalho G and Tsushima K Phys. Rev. D 84, 544; Ramalho G, Tsushima K and Thomas A W 3 J. Phys. G 4, 5. Phys. Rev. D 84, 544 (); [4] Ramalho G, Tsushima K and Gross F 9 Phys. Rev. D 8, 334. [5] Ramalho G and Peña M T 9 J. Phys. G 36, 5. [6] Ramalho G and Tsushima K 3 Phys. Rev. D 87, 93; Phys. Rev. D 88, 53. [7] Ramalho G and Tsushima K Phys. Rev. D 8, 74; Ramalho G and Tsushima K 4 Phys. Rev. D 89, 73. [8] Ramalho G and Peña M T 9 Phys. Rev. D 8, 38. [9] Ramalho G, Peña M T and Gross F 8 Eur. Phys. J. A 36, 39; Phys. Rev. D 78, 47; Ramalho G, Peña M T and Gross F Phys. Rev. D 8, 3; Ramalho G, Peña M T and Stadler A Phys. Rev. D 86, 93. [] Ramalho G and Tsushima K Phys. Rev. D 8, 737. [] Ramalho G and Tsushima K Phys. Rev. D 86, 43; Ramalho G and Peña M T Phys. Rev. D 83, 54; Ramalho G, Jido D and Tsushima K Phys. Rev. D 85, 934. [] Ramalho G and Peña M T Phys. Rev. D 85, 34. [3] Gross F, Ramalho G, Peña M T Phys. Rev. D 85, 936. [4] Ramalho G and Tsushima K, to be submitted. [5] Sato T, Lee T-S L 9 J. Phys. G 36, 73. [6] Hey A J G and Weyers 974 Phys. Lett. B 48, 69; Cottingham W N and Dunbar I H 979 Z. Phys. C, 4. [7] Dugger M et al. [CLAS Collaboration] 9 Phys. Rev. C 79, 656. [8] Mokeev V I et al. [CLAS Collaboration] Phys. Rev. C 86, 353. [9] Beringer J et al. [Particle Data Group Collaboration] Phys. Rev. D 86,. [3] Electromagnetic N-N* Transition Form Factors Workshop, Jlab, Newport News, 8 (unpublished) [3] Carlson C E and Poor J L 998 Phys. Rev. D 38, 758. 8