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Scalar Meson Exchange and the Baryon Spectra*

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Scalar Meson Exchange and the Baryon Spectra* View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server Scalar meson exchange and the baryon sp ectra P. Stassart and Fl. Stancu Universitede Liege, Institut de Physique B.5, Sart Tilman, B-4000 Liege 1, Belgium J.-M. Richard Institut des Sciences Nucleaires, Universite Joseph Fourier IN2P3-CNRS, 53, Avenue des Martyrs F-38026 Grenoble Cedex, France (Octob er 9, 1998) Abstract We explore the role of a scalar meson exchange interaction between quarks in a semirelativistic constituent quark mo del where the quarks are sub ject to a linear con nement. We search for a variational solution and show that the gap between the N = 1 band and the ground state N = 0 band increases with the strength of the scalar meson exchange interaction p otential. This result has go o d implications on the description of the low-lying baryon masses, esp ecially on the Rop er vs. negative-parity resonances ordering. It has b een suggested [1,2] that b eyond the scale of sp ontaneous chiral sypmmetry break- ing, nonstrange and strange baryons can b e viewed as systems of three quarks interacting via to app ear in the Pro ceedings of the Third International Conference on Quark Con nement and the Hadron Spectrum III, Je erson Lab. (Newp ort News, USA) June 7-12, 1998 , World Scienti c (Singap ore) 1 exchange of Goldstone b osons (pseudoscalar mesons). It has also b een shown that a prop- erly parametrized interaction provides go o d baryon sp ectra with a correct order of p ositive and negative parity levels b oth in a nonrelativistic [3] or a semirelativistic [4] treatment. In b oth parametrizations the pseudoscalar meson exchange interaction has two distinct parts: a long-range Yukawa p otential tail and a short-range part having opp osite sign as compared to the Yukawa p otential tail. It is the latter which plays a ma jor role in describing the baryon sp ectra in the frame of Goldstone b oson exchange (GBE) mo dels. Although the mo dels [2{4] are thought to be a consequence of the sp ontaneous chiral symmetry breaking, the chiral partner of the pion, the sigma meson, is not considered explicitly. One can think of having mo cked up its contribution in the parameters of the Hamiltonian [3,4], e.g. in the regularization parameter of the short-range spin-spin term. 0 The price which could have b een paid is the large role played by the meson exchange 2 which comes into the interaction with a strength g =4 ab out equal [4] or larger [3] than 0 2 the strength g =4 asso ciated with the pseudoscalar o ctet (; K; ). 8 Here we study the explicit role of a sigma-exchange interaction by considering the fol- lowing Hamiltonian 2 X X X p 1=2 1 g exp [ j~r ~r j] i j 2 2 H = m + p + j~r ~r j (1) 0 i j i i 2 4 j~r ~r j i j i i<j i<j where the second term is the con nement p otential with a strength tension [5] p 1 =1 GeV fm (2) 2 =4 is the coupling constant sigma-quark, = 600 MeV is the sigma meson mass and g 2 taken as a variable parameter. From the pion-nucleon coupling constant g =4 ' 14, N N 2 one obtains a pion-quark coupling constant g =4 = 0.67 which has b een used in [3,4]. qq 2 2 Assuming a sigma-nucleon coupling g =4 ' 8 [6] one obtains, by scaling, g =4 ' 0.4. N N qq 2 In the following we study the role of the -meson exchange by considering values of g =4 qq up to 0.2. A qualitative argument that the -meson contributes attractively in (1) is that we view it as a two correlated pions, as in the nucleon-nucleon interaction. Moreover, one can 2 consider more sophisticated arguments related to the di erences app earing in the scalar and pseudoscalar propagators [7] in a Nambu-Jona-Lasinio mo del. From there one can argue that the Fourier transform would lead to a Yukawa + a contact term for a scalar and a Yukawa - a contact term, for a pseudoscalar exchange, as in Refs. [3,4]. Due to the addition of the long and short range contributions in the scalar case, here we consider a simpli ed form of the -exchange p otential, containing a single term as in (1). The variational wave function has the form 2 3 Y 4 5 f (r ) (~r ;~r ;~r ) : (3) (~r ;~r ;~r )= F ij n 12 13 13 n 12 13 23 123 i<j where f and F are two- and three-b o dy parts of the ground state wave function and 123 n with n 6= 0 contain orbital excitations [8]. The function f is parametrized as o n 1:5 ; f (r )= r exp W (r ) r [1 W (r )] r 1 1:5 1+exp ( r =a) (4) 0 W (r )= 1+exp [(r r ) =a] 0 The three-b o dy part is chosen as 13 0 2 X X p 1 A5 @ 4 r : (5) r F = 1 ij i4 123 2 i<j i The quantities , , a, r , and are variational parameters. In the minimization 1 1:5 0 pro cedure we found that the ground state exp ectation value of (1) varies smo othly with all these parameters but . It is quite natural b ecause cares for the b ehaviour of the wave function near the origin, typical for the solution of a relativistic equation with a 2 =4 the more dicult in reaching singular p otential. The larger the coupling constant g the minimum. The exp ectation value for the rst two excited states are obtained with the optimal values of the ground state parameters. The result is exhibited in the table b elow. 3 2 g =4 ground st. neg.parity radial excit. 0.00 940 1287 1446 0.05 940 1309 1444 0.10 940 1333 1444 0.15 940 1380 1445 0.20 940 1431 1446 One can see that the mass di erence between the rst radially excited state and the negative parity state is p ositive up to the coupling constant value of 0.20 but tends to vanish. Note also that the di erence b etween the radially excited state and the ground state remains practically constant as a function of the coupling constant, while the mass di erence 2 between the orbitally excited state and the ground state increases with g =4 . The reason for this is that at g 6= 0 all s states are lowered with resp ect to the p states. The wave function of the latter is small around the origin, so that it reduces some of the attraction in the exp ectation value. Preliminary results indicate that the mass di erence between the rst radially excited 2 state and the negative parity state b ecomes negative for g =4>0:20. This is precisely the desired b ehaviour for repro ducing the correct order of the exp erimental sp ectrum, as in Ref. [3]. These calculations indicate that a mo del incorp orating a p otential, whose Laplacian is negative in a region around the origin, can yield the right ordering of the lowest p ositive and negative parity states. For the p otential of Eq. (1) such a situation is achieved for 2 suitable values of the coupling constant g =4 . The Laplacian is related to the concavityof the two-body p otential as discussed in Ref. [9]. The conclusion is that Goldstone b oson exchange mo dels should include explicitly the chiral partner of the pseudoscalar mesons. It might be misleading to mo ck up its e ect in some nontrivial parameters of the mo del. We are presently studying the case of a p otential with b oth scalar and pseudoscalar terms. However the question still remains ab out the role 4 of the chromomagnetic interaction. Finally, the scalar exchange term, which we have shown to be imp ortant for the level ordering, might also genearate a new spin-orbit contribution. It would b e interesting to see whether or not that contribution could signi cantly improve our present knowledge of the spin-orbit problem in baryons [10]. 5 REFERENCES [1] A. Manohar and H. Georgi, Nucl.Phys. B234 (1984) 189 [2] L.Ya. Glozman and D.O. Riska, Phys. Rep. 268 (1996) 263 [3] L.Ya. Glozman, Z. Papp and W. Plessas, Phys. Lett. B381 (1996) 311; L.Ya. Glozman, Z. Papp, W. Plessas, K. Varga and R.F. Wagenbrunn, Nucl.Phys. A623 (1997) 90c [4] L.Ya. Glozman, W. Plessas, K. Varga and R.F. Wagenbrunn, Phys. Rev. D58 in print, e-print hep-ph/9706507 [5] J. Carlson, J. Kogut and V.R. Pandharipande, Phys.Rev. D28 (1983) 2808 [6] R. Machleidt, K. Holinde and Ch. Elster, Phys.Rep. 149 (1987) 1 [7] M. Jaminon, G. Ripka and P. Stassart, Nucl.Phys. A504 (1989) 733 [8] R. Sartor and Fl. Stancu, Phys. Rev. D31 (1985) 128 [9] A. Martin, J.-M. Richard and P. Taxil, Nucl. Phys. B329 (1990) 327 [10] See e.g., W. Lucha, F. Schob erl and D. Gromes, Phys. Rep. 203 (1991) 127, and refer- ences therein. 6.
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