Abstract
We revisit the coupled-channel \(K\bar{K}\) interactions and dynamically generate the resonances \(f_0(980)\) and \(a_0(980)\) within both the isospin and the physical bases. The \(f_0(980)\)–\(a_0(980)\) mixing effects are generated in the scattering amplitudes of the coupled channels with the physical basis, which exploits the important role of the \(K\bar{K}\) channel in the dynamical nature of these resonances. With the scattering amplitudes obtained, we investigate the \(f_0(980)\) and \(a_0(980)\) contributions to the \(J/\psi \rightarrow \gamma \eta \pi ^0\), \(J/\psi \rightarrow \gamma \pi ^+\pi ^-\) and \(J/\psi \rightarrow \gamma \pi ^0\pi ^0\) radiative decays through the final-state interactions. We obtain the corresponding branching fractions \(\mathrm{Br}(J/\psi \rightarrow \gamma a_0(980) \rightarrow \gamma \eta \pi ^0) = (0.48\pm 0.03) \times 10^{-7}\), \(\mathrm{Br}(J/\psi \rightarrow \gamma f_0(980) \rightarrow \gamma \pi ^+\pi ^-) = (0.52-2.08) \times 10^{-7}\), \(\mathrm{Br}(J/\psi \rightarrow \gamma f_0(980) \rightarrow \gamma \pi ^0\pi ^0) = (0.26-1.04) \times 10^{-7}\), and predict \(\mathrm{Br}(J/\psi \rightarrow \gamma a_0(980)) = (1.24 - 1.61) \times 10^{-7}\) and \(\mathrm{Br}(J/\psi \rightarrow \gamma f_0(980)) = (0.69 - 4.00) \times 10^{-7}\). These fractions are within the upper limits of the experimental measurements.
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Data Availability Statement
This manuscript has no associated data or the data will not be deposited. [Authors’ comment: This is a theoretical investigation.]
Notes
Given the exploratory aim of our study on the mixing between the \(f_0(980)\) and \(a_0(980)\) resonances in \(J/\psi \) radiative decays, and since the experimental data can be well reproduced by unitarizing the leading-order V matrix (as shown below), we do not take into account in this work the contributions from the next-to-leading-order chiral perturbation theory amplitudes. The latter were already applied in the study of the scalar meson–meson scattering and its spectroscopy in several places in the literature, e.g., in [33, 40, 47,48,49, 51, 82, 83].
If the lightest vector and axial-vector resonances already provide total small contributions we think that is then sensitive to neglect heavier ones as they are expected to be even smaller because of the mass squared suppression of heavier-state propagators.
Reference [87] concludes that the unitarity-loop function \(G(M_{\mathrm{inv}}^ 2)\) used in Eq. (19) could actually differ by a constant of its counterpart in the evaluation of the partial-wave amplitudes, cf. Eq. (2). However, here we use a cutoff regularization for this function and insist on having a natural value for the cutoff around \(1{\text { GeV}}\) in all the cases.
An extra factor of \(\sqrt{2}\) is introduced in the Clebsch–Gordan coefficients for the \(\pi \pi \) states because of the unitarity normalization for the \(I=0\)\(\pi \pi \) state [31].
The \(J/\psi \) is a \(c\bar{c}\) and its decay into light-quark hadrons is an isoscalar OZI violating process rich in intermediate gluons that we also take as a scalar source following Ref. [95]. This is similar to the well-known \(^3P_0\) decay model in the quark model [96] where a \(q\bar{q}\) is produced from the vacuum and having its same quantum numbers. In this way, the isoscalar part of the electromagnetic current is selected because the radiative coupling of the photon to the charge kaons is already accounted for by the diagrams (a) and (b) of Fig. 8.
References
R. Aaij et al., [LHCb Collaboration], Phys. Rev. Lett. 115, 072001 (2015). arXiv:1507.03414 [hep-ex]
R. Aaij et al. [LHCb Collaboration], arXiv:1904.03947 [hep-ex]
H.X. Chen, W. Chen, X. Liu, S.L. Zhu, Phys. Rep. 639, 1 (2016). arXiv:1601.02092 [hep-ph]
A. Hosaka, T. Iijima, K. Miyabayashi, Y. Sakai, S. Yasui, PTEP 2016(6), 062C01 (2016). arXiv:1603.09229 [hep-ph]
H.X. Chen, W. Chen, X. Liu, Y.R. Liu, S.L. Zhu, Rep. Prog. Phys. 80(7), 076201 (2017). arXiv:1609.08928 [hep-ph]
R.F. Lebed, R.E. Mitchell, E.S. Swanson, Prog. Part. Nucl. Phys. 93, 143 (2017). arXiv:1610.04528 [hep-ph]
A. Esposito, A. Pilloni, A.D. Polosa, Phys. Rep. 668, 1 (2016). arXiv:1611.07920 [hep-ph]
F.K. Guo, C. Hanhart, U.-G. Meißner, Q. Wang, Q. Zhao, B.S. Zou, Rev. Mod. Phys. 90(1), 015004 (2018). arXiv:1705.00141 [hep-ph]
A. Ali, J.S. Lange, S. Stone, Prog. Part. Nucl. Phys. 97, 123 (2017). arXiv:1706.00610 [hep-ph]
S.L. Olsen, T. Skwarnicki, D. Zieminska, Rev. Mod. Phys. 90(1), 015003 (2018). arXiv:1708.04012 [hep-ph]
M. Karliner, J.L. Rosner, T. Skwarnicki, Ann. Rev. Nucl. Part. Sci. 68, 17 (2018). arXiv:1711.10626 [hep-ph]
C.Z. Yuan, Int. J. Mod. Phys. A 33(21), 1830018 (2018). arXiv:1808.01570 [hep-ex]
A. Astier, L. Montanet, M. Baubillier, J. Duboc, Phys. Lett. B 25, 294 (1967)
R. Ammar et al., Phys. Rev. Lett. 21, 1832 (1968)
C. Defoix, P. Rivet, J. Siaud, B. Conforto, M. Widgoff, F. Shively, Phys. Lett. B 28, 353 (1968)
S.D. Protopopescu et al., Phys. Rev. D 7, 1279 (1973)
B. Hyams et al., Nucl. Phys. B 64, 134 (1973)
S. Godfrey, N. Isgur, Phys. Rev. D 32, 189 (1985)
D. Morgan, M.R. Pennington, Z. Phys. C 48, 623 (1990)
D. Morgan, M.R. Pennington, Phys. Rev. D 48, 1185 (1993)
R.L. Jaffe, Phys. Rev. D 15, 267 (1977)
R.L. Jaffe, Phys. Rev. D 15, 281 (1977)
N.N. Achasov, S.A. Devyanin, G.N. Shestakov, Phys. Lett. B 96, 168 (1980)
K.L. Au, M.R. Pennington, D. Morgan, Phys. Lett. B 167, 229 (1986)
S.M. Flatté, Phys. Lett. B 63, 224 (1976)
J.D. Weinstein, N. Isgur, Phys. Rev. Lett. 48, 659 (1982)
J.D. Weinstein, N. Isgur, Phys. Rev. D 41, 2236 (1990)
B.S. Zou, D.V. Bugg, Phys. Rev. D 50, 591 (1994)
G. Janssen, B.C. Pearce, K. Holinde, J. Speth, Phys. Rev. D 52, 2690 (1995). arXiv:nucl-th/9411021
N.A. Tornqvist, M. Roos, Phys. Rev. Lett. 76, 1575 (1996). arXiv:hep-ph/9511210
J.A. Oller, E. Oset, Nucl. Phys. A 620, 438 (1997). Erratum: [Nucl. Phys. A 652, 407 (1999)]. arXiv:hep-ph/9702314
M.P. Locher, V.E. Markushin, H.Q. Zheng, Eur. Phys. J. C 4, 317 (1998). arXiv:hep-ph/9705230
J.A. Oller, E. Oset, J.R. Peláez, Phys. Rev. D 59, 074001 (1999). Erratum: [Phys. Rev. D 60, 099906 (1999)]. Erratum: [Phys. Rev. D 75, 099903 (2007)]. arXiv:hep-ph/9804209
J.A. Oller, E. Oset, Phys. Rev. D 60, 074023 (1999). arXiv:hep-ph/9809337
V. Baru, J. Haidenbauer, C. Hanhart, Y. Kalashnikova, A.E. Kudryavtsev, Phys. Lett. B 586, 53 (2004). arXiv:hep-ph/0308129
V. Baru, J. Haidenbauer, C. Hanhart, A.E. Kudryavtsev, U.-G. Meißner, Eur. Phys. J. A 23, 523 (2005). arXiv:nucl-th/0410099
V. Baru, C. Hanhart, Y.S. Kalashnikova, A.E. Kudryavtsev, A.V. Nefediev, Eur. Phys. J. A 44, 93 (2010). arXiv:1001.0369 [hep-ph]
D.V. Bugg, V.V. Anisovich, A. Sarantsev, B.S. Zou, Phys. Rev. D 50, 4412 (1994)
J.J. Dudek et al. [Hadron Spectrum Collaboration], Phys. Rev. D 93(9), 094506 (2016). arXiv:1602.05122 [hep-ph]
Z.H. Guo, L. Liu, U.-G. Meißner, J.A. Oller, A. Rusetsky, Phys. Rev. D 95(5), 054004 (2017). arXiv:1609.08096 [hep-ph]
R. Garcia-Martin, R. Kaminski, J.R. Peláez, J. Ruiz de Elvira, Phys. Rev. Lett. 107, 072001 (2011). arXiv:1107.1635 [hep-ph]
G. Colangelo, J. Gasser, H. Leutwyler, Nucl. Phys. B 603, 125 (2001). arXiv:hep-ph/0103088
B. Ananthanarayan, G. Colangelo, J. Gasser, H. Leutwyler, Phys. Rep. 353, 207 (2001). arXiv:hep-ph/0005297
I. Caprini, G. Colangelo, H. Leutwyler, Phys. Rev. Lett. 96, 132001 (2006). arXiv:hep-ph/0512364
M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, 030001 (2018)
M. Albaladejo, J.A. Oller, Phys. Rev. Lett. 101, 252002 (2008). arXiv:0801.4929 [hep-ph]
M. Albaladejo, J.A. Oller, Phys. Rev. D 86, 034003 (2012). arXiv:1205.6606 [hep-ph]
Z.H. Guo, J.A. Oller, J. Ruiz de Elvira, Phys. Lett. B 712, 407 (2012). arXiv:1203.4381 [hep-ph]
Z.H. Guo, J.A. Oller, J. Ruiz de Elvira, Phys. Rev. D 86, 054006 (2012). arXiv:1206.4163 [hep-ph]
A Gomez Nicola, J .R. Peláez, Phys. Rev. D 65, 054009 (2002). arXiv:hep-ph/0109056
Z.H. Guo, J.A. Oller, Phys. Rev. D 84, 034005 (2011). arXiv:1104.2849 [hep-ph]
N.N. Achasov, S.A. Devyanin, G.N. Shestakov, Phys. Lett. B 88, 367 (1979)
B. Kerbikov, F. Tabakin, Phys. Rev. C 62, 064601 (2000). arXiv:nucl-th/0006017
F.E. Close, A. Kirk, Phys. Lett. B 489, 24 (2000). arXiv:hep-ph/0008066
V.Y. Grishina, L.A. Kondratyuk, M. Buescher, W. Cassing, H. Stroher, Phys. Lett. B 521, 217 (2001). arXiv:nucl-th/0103081
F.E. Close, A. Kirk, Phys. Lett. B 515, 13 (2001). arXiv:hep-ph/0106108
N.N. Achasov, A.V. Kiselev, Phys. Lett. B 534, 83 (2002). arXiv:hep-ph/0203042
A.E. Kudryavtsev, V.E. Tarasov, J. Haidenbauer, C. Hanhart, J. Speth, Phys. Rev. C 66, 015207 (2002). arXiv:nucl-th/0203034
N.N. Achasov, G.N. Shestakov, Phys. Rev. Lett. 92, 182001 (2004). arXiv:hep-ph/0312214
N.N. Achasov, G.N. Shestakov, Phys. Rev. D 70, 074015 (2004). arXiv:hep-ph/0405129
J.J. Wu, Q. Zhao, B.S. Zou, Phys. Rev. D 75, 114012 (2007). arXiv:0704.3652 [hep-ph]
C. Hanhart, B. Kubis, J.R. Peláez, Phys. Rev. D 76, 074028 (2007). arXiv:0707.0262 [hep-ph]
J.J. Wu, B.S. Zou, Phys. Rev. D 78, 074017 (2008). arXiv:0808.2683 [hep-ph]
M. Ablikim et al. [BESIII Collaboration], Phys. Rev. D 83, 032003 (2011). arXiv:1012.5131 [hep-ex]
M. Ablikim et al. [BESIII Collaboration], Phys. Rev. Lett. 121(2), 022001 (2018). arXiv:1802.00583 [hep-ex]
E. Oset, A. Ramos, Nucl. Phys. A 635, 99 (1998). arXiv:nucl-th/9711022
J.A. Oller, U.-G. Meißner, Phys. Lett. B 500, 263 (2001). arXiv:hep-ph/0011146
L. Roca, Phys. Rev. D 88, 014045 (2013). arXiv:1210.4742 [hep-ph]
M. Bayar, V.R. Debastiani, Phys. Lett. B 775, 94 (2017). arXiv:1708.02764 [hep-ph]
T. Sekihara, S. Kumano, Phys. Rev. D 92(3), 034010 (2015). arXiv:1409.2213 [hep-ph]
S. Nussinov, T.N. Truong, Phys. Rev. Lett. 63, 1349 (1989). Erratum: [Phys. Rev. Lett. 63, 2002 (1989)]
N.N. Achasov, V.N. Ivanchenko, Nucl. Phys. B 315, 465 (1989)
J L Lucio Martinez, J. Pestieau, Phys. Rev. D 42, 3253 (1990)
F.E. Close, N. Isgur, S. Kumano, Nucl. Phys. B 389, 513 (1993). arXiv:hep-ph/9301253
A. Bramon, R. Escribano, J .L .M. Lucio, M. Napsuciale, G. Pancheri, Phys. Lett. B 494, 221 (2000). arXiv:hep-ph/0008188
A. Bramon, R. Escribano, J L Lucio Martinez, M. Napsuciale, Phys. Lett. B 517, 345 (2001). arXiv:hep-ph/0105179
A. Bramon, R. Escribano, J .L .M. Lucio, M. Napsuciale, G. Pancheri, Eur. Phys. J. C 26, 253 (2002). arXiv:hep-ph/0204339
J.A. Oller, Phys. Lett. B 426, 7 (1998). arXiv:hep-ph/9803214
E. Marco, S. Hirenzaki, E. Oset, H. Toki, Phys. Lett. B 470, 20 (1999). arXiv:hep-ph/9903217
J.E. Palomar, L. Roca, E. Oset, M J Vicente Vacas, Nucl. Phys. A 729, 743 (2003). arXiv:hep-ph/0306249
M. Ablikim et al. [BESIII Collaboration], Phys. Rev. D 94(7), 072005 (2016). arXiv:1608.07393 [hep-ex]
J.R. Peláez, G. Rios, Phys. Rev. Lett. 97, 242002 (2006). https://doi.org/10.1103/PhysRevLett.97.242002. arXiv:hep-ph/0610397
J.R. Peláez, G. Ríos, Phys. Rev. D 82, 114002 (2010). https://doi.org/10.1103/PhysRevD.82.114002. arXiv:1010.6008 [hep-ph]
F. Aceti, J.M. Dias, E. Oset, Eur. Phys. J. A 51(4), 48 (2015). arXiv:1501.06505 [hep-ph]
T.A. Armstrong et al. [WA76 and Athens-Bari-Birmingham-CERN-College de France Collaborations], Z. Phys. C 52, 389 (1991)
J.B. Gay et al. [Amsterdam-CERN-Nijmegen-Oxford Collaboration], Phys. Lett. B 63, 220 (1976)
J.A. Oller, Nucl. Phys. A 714, 161 (2003). arXiv:hep-ph/0205121
F. Klingl, N. Kaiser, W. Weise, Z. Phys. A 356, 193 (1996). arXiv:hep-ph/9607431
U.-G. Meißner, Phys. Rep. 161, 213 (1988)
A. Bramon, A. Grau, G. Pancheri, Phys. Lett. B 289, 97 (1992)
L. Roca, J.E. Palomar, E. Oset, H.C. Chiang, Nucl. Phys. A 744, 127 (2004). arXiv:hep-ph/0405228
J.J. Sakurai, Currents and Mesons (University of Chicago Press, Chicago, 1969)
M. Bando, T. Kugo, S. Uehara, K. Yamawaki, T. Yanagida, Phys. Rev. Lett. 54, 1215 (1985)
C.W. Xiao, E. Oset, Eur. Phys. J. A 49, 52 (2013). arXiv:1211.1862 [hep-ph]
U.-G. Meißner, J.A. Oller, Nucl. Phys. A 679, 671 (2001). arXiv:hep-ph/0005253
L. Micu, Nucl. Phys. B 10, 521 (1969)
M. Ablikim et al. [BESIII Collaboration], Phys. Rev. D 92(5), 052003 (2015). Erratum: [Phys. Rev. D 93(3), 039906 (2016)]. arXiv:1506.00546 [hep-ex]
M. Ablikim et al., Phys. Lett. B 642, 441 (2006). arXiv:hep-ex/0603048
J. Becker et al. [Mark-III Collaboration], Phys. Rev. D 35, 2077 (1987)
J.E. Augustin et al. [DM2 Collaboration], Z. Phys. C 36, 369 (1987)
J.Z. Bai et al. [BES Collaboration], Phys. Rev. Lett. 76, 3502 (1996)
M. Ablikim et al. [BESIII Collaboration], arXiv:1808.06946 [hep-ex]
A. Martinez Torres, K.P. Khemchandani, F.S. Navarra, M. Nielsen, E. Oset, Phys. Lett. B 719, 388 (2013). arXiv:1210.6392 [hep-ph]
J.J. Xie, E. Oset, Phys. Lett. B 753, 591 (2016). arXiv:1509.08099 [hep-ph]
Acknowledgements
CWX thanks E. Oset and Q. Wang for the useful discussions. This work is supported in part by the DFG and the NSFC through funds provided to the Sino-German CRC 110 “Symmetries and the Emergence of Structure in QCD”. JAO would like to thank partial financial support by the MINECO (Spain) and FEDER (EU) grant FPA2016-77313-P. The work of UGM was also supported by the Chinese Academy of Sciences (CAS) President’s International Fellowship Initiative (PIFI) (Grant No. 2018DM0034) and by VolkswagenStiftung (Grant No. 93562).
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Xiao, C.W., Meißner, UG. & Oller, J.A. Investigation of \(J/\psi \rightarrow \gamma \, \pi ^0 \eta (\pi ^+\pi ^-, \pi ^0\pi ^0)\) radiative decays including final-state interactions. Eur. Phys. J. A 56, 23 (2020). https://doi.org/10.1140/epja/s10050-020-00025-y
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DOI: https://doi.org/10.1140/epja/s10050-020-00025-y