Isospin splittings of doubly heavy baryons

Brodsky, S. J.; Guo, F.-K.; Hanhart, C.; Meißner, U.-G.

doi:10.1016/j.physletb.2011.03.014

Journal Article

PreJuSER-18592

Isospin splittings of doubly heavy baryons

Brodsky, S. J. ; Guo, F.-K. ; Hanhart, C.FZJ* ; Meißner, U.-G.FZJ*

2011
North-Holland Publ. Amsterdam

Physics letters / B 698, 251 - 255 (2011) [10.1016/j.physletb.2011.03.014]

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Please use a persistent id in citations: http://hdl.handle.net/2128/10293 doi:10.1016/j.physletb.2011.03.014

Abstract: The SELEX Collaboration has reported a very large isospin splitting of doubly charmed baryons. We show that this effect would imply that the doubly charmed baryons are very compact. One intriguing possibility is that such baryons have a linear geometry Q-q-Q where the light quark q oscillates between the two heavy quarks Q, analogous to a linear molecule such as carbon dioxide. However, using conventional arguments, the size of a heavy-light hadron is expected to be around 0.5 fm, much larger than the size needed to explain the observed large isospin splitting. Assuming the distance between two heavy quarks is much smaller than that between the light quark and a heavy one, the doubly heavy baryons are related to the heavy mesons via heavy quark-diquark symmetry. Based on this symmetry, we predict the isospin splittings for doubly heavy baryons including Xi(cc), Xi(bb) and Xi(bc). The prediction for the Xi(cc) is much smaller than the SELEX value. On the other hand, the Xi(bb) baryons are predicted to have an isospin splitting as large as (6.3 +/- 1.7) MeV. An experimental study of doubly bottomed baryons is therefore very important to better understand the structure of baryons with heavy quarks. (C) 2011 Elsevier B.V. All rights reserved.

Keyword(s): baryon: heavy ; isospin ; charmed baryon: bottom baryon ; charm: 2 ; bottom: 2 ; baryon: mass difference ; pentaquark ; Doubly heavy baryons (auto) ; Isospin splitting (auto) ; Heavy quark-diquark symmetry (auto)

Classification:

Physics, Multidisciplinary

Note: We want to thank J. Gasser for helpful discussions and U.-G.M. acknowledges a useful communication from H. Leutwyler. S.J.B. is indebted to M. Karliner and H. Lipkin for very helpful discussions on effective diquark models. We also thank J. Engelfried, J.-P. Lansberg, A. Goldhaber and J. Russ for comments. F.-K.G., C.H. and U.-G.M. would like to thank the DFG (SFB/TR 16, "Subnuclear Structure of Matter"), the HGF (Virtual Institute "Spin and Strong QCD", VH-VI-231), and the European Community-Research Infrastructure Integrating Activity "Study of Strongly Interacting Matter" (acronym HadronPhysics2, Grant Agreement No. 227431) under the Seventh Framework Programme of EU for support. U.-G.M. also thanks the BMBF for support (grant 06BN9006). This research was also supported by the Department of Energy, contract DE-AC02-76SF00515.

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