Bled Workshops in Physics Vol. 10, No. 1 p. 39 Quadrupole polarizabilities of the pion in the Nambu-Jona-Lasinio model* Brigitte Hillera, Wojciech Broniowskib,c, Alexander A. Osipova,d, Alex H. Blina a Centro de Física Computacional, Departamento de Física da Universidade de Coimbra, 3004-516 Coimbra, Portugal b The H. Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, PL-31342 Cracow, Poland c Institute of Physics, Jan Kochanowski University, PL-25406 Kielce, Poland d Dzhelepov Laboratory of Nuclear Problems, JINR, 141980 Dubna, Russia Abstract. We present the results for the pion electromagnetic quadrupole polarizabilities, calculated within the Nambu-Jona-Lasinio model. We obtain the sign and magnitude in agreement with the respective experimental analysis based on the Dispersion Sum Rules. At the same time the dipole polarizabilities are well reproduced. Comparison is also made with the results from the Chiral Perturbation Theory. The neutral and charged pion dipole and quadrupole polarizabilities have been recently analyzed using the Dispersion Relations (DR) and the Dispersion Sum Rules (DSR) [1,2], as displayed in Tables 2 and 3, together with the results of the Chiral Perturbation Theory (xPT) [3-5]. The first row shows our results based on the Nambu-Jona-Lasinio model (NJL) [6] model; for that purpose we have extended [7] the study of Ref. [8], where the dipole polarizabilities have been calculated, to the quadrupole case. We refer to these papers for details. Our leading-Nc calculations are done according to the Feynman diagrams of Fig. 1. The amplitude is a function of the Mandelstam variables related to the Y(pi, ) + y(P2, e2) —> na(p3) + nb(p4) reaction for the on-shell pions and photons, T (pi,p2,p3) = e2efeW, V = A(s,t,u)£^v + B(s,t,u)£^, with the Lorentz tensors ¿T =P2MP7 - = - +tlP£PJ +ulP£Pi + . Terms that vanish upon the conditions e1 • p1 = e2 • p2 = 0 are omitted and the notation £ = £ — m^, £ = s,t,u is used. The scalar quantities A and B enter the amplitudes H++ = —(A + m^B) and H+_ = (u1t1/s — m^)B for the equal-helicity and helicity-flipped photons. The dipole, a}, p1, and quadrupole, * Talk delivered by Brigitte Hiller a2> P2, polarizabilities are obtained in the t-channel and extracted from the first two coefficients of the Taylor expansion of the amplitudes aAl(s,t,u)/(2mn) and -amnBl(s,t,u) around s = 0 with u = t = m^ [9], (AMO.m^m2) +sAAi(0,m2,m^ = p} + Apt, -am« ^BMO.m^m^+s^BMO.m^m2)^ = (ai + Pi )l + ^j(n± are totally determined by the gauge-invariant quark box or the box + pion exchange contribution. This is a key result of the presented calculation. The sign is stable when the model parameters are changed. The magnitude depends on the value chosen for the constituent quark mass, but the best overall fit to the other empirical data, typically yielding M ~ 300 MeV, also yields the optimum values for the polarizabilities [7]. Moreover, the main part of the box contribution comes from the first non-vanishing p8-order term in the chiral expansion. Based on this fact we expect that the contact term of the p8 3-loop calculation in xPT may also play an important role in reversing the signs of the 2-loop order results for these quantities. Acknowledgement We are very grateful to the organizers of the "Mini-Workshop Bled 2009: Problems in multi-quark states", for the kind invitation to present this work. This research is supported by the Polish Ministry of Science and Higher Education, grants N202 034 32/0918 and N202 249235, by Fundacao para a Ciencia e Tecnologia, grants FEDER, OE, POCI 2010, CERN/FP/83510/2008, and by the European Community-Research Infrastructure Integrating Activity Study of Strongly InteractingMatter (Grant Agreement 227431) under the Seventh Framework Programme of the EU. References 1. L. V. Fil'kov, V. L. Kashevarov, Phys. Rev. C 72 (2005) 035211. 2. L. V. Fil'kov, V. L. Kashevarov, Phys. Rev. C 73 (2006) 035210. 3. J. Gasser, M. A. Ivanov, M. E. Sainio, Nucl. Phys. B 728 (2005) 31. 4. J. Gasser, M. A. Ivanov, M. E. Sainio, Nucl. Phys. B 745 (2006) 84. 5. S. Bellucci, J. Gasser, M. E. Sainio, Nucl. Phys. B 423 (1994) 80; S. Bellucci, J. Gasser, M. E. Sainio, Nucl. Phys. B 431 (1994) 413, Erratum. 6. Y. Nambu, J. Jona-Lasinio, Phys. Rev. 122 (1961) 345; 124 (1961) 246. 7. B. Hiller, W. Broniowski, A. A. Osipov, A. H. Blin, arXiv:0908.0159 [hep-ph] 8. B. Bajc, A. H. Blin, B. Hiller, M. C. Nemes, A. A. Osipov, M. Rosina, Nucl. Phys. A 604 (1996) 406. 9. I. Guiasu, E. E. Radescu, Ann. Phys. 120 (1979) 145; I. Guiasu, E.E. Radescu, Ann. Phys. 122 (1979) 436. 10. V. Bernard, A. A. Osipov, U.-G. Meißner, Phys. Lett. B 285 (1992) 119. 11. J. Bijnens, F. Cornet, Nucl. Phys. B 296 (1988) 557. 12. J. F. Donoghue, B. R. Holstein, Y. C. Lin, Phys. Rev. D 37 (1988) 2423. 13. J. F. Donoghue, B. R. Holstein, Phys. Rev. D 48 (1993) 137.