Why Ξ(1690) and Ξ(2120) are so narrow

K. P. Khemchandani, A. Martínez Torres, A. Hosaka, H. Nagahiro, F. S. Navarra, and M. Nielsen
Phys. Rev. D 97, 034005 – Published 7 February 2018

Abstract

The Ξ baryons are expected to be naturally narrower as compared to their nonstrange and strange counterparts since they have only one light quark and, thus, their decay involves producing either a light meson and doubly strange baryon or both meson and baryon with strangeness which involves, relatively, more energy. In fact, some Ξ’s have full widths of the order of even 10–20 MeV when, in principle, they have a large phase space to decay to some open channels. Such is the case of Ξ(1690), for which the width has been found to be of the order of 10 MeV in the latest BABAR and BELLE data. In this manuscript we study why some Ξ’s are so narrow. Based on a coupled channel calculation of the pseudoscalar meson-baryon and vector meson-baryon systems with chiral and hidden local symmetry Lagrangians, we find that the answer lies in the intricate hadron dynamics. We find that the known mass, width, spin-parity, and branching ratios of Ξ(1690) can be naturally explained in terms of coupled channel meson-baryon dynamics. We find another narrow resonance which can be related to Ξ(2120). We also look for exotic states Ξ+ and Ξ but find none. In addition we provide the cross sections for K¯Λ,K¯ΣπΞ which can be useful for understanding the enhanced yield of Ξ reported in recent studies of heavy ion collisions.

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  • Received 23 September 2016
  • Revised 21 December 2017

DOI:https://doi.org/10.1103/PhysRevD.97.034005

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

K. P. Khemchandani1,2,*, A. Martínez Torres3, A. Hosaka4, H. Nagahiro4,5, F. S. Navarra3, and M. Nielsen3

  • 1Departamento de Ciências Exatas e da Terra, Universidade Federal de São Paulo, Campus Diadema, Rua Prof. Artur Riedel, 275, Jardim Eldorado, Diadema, 09972-270 São Paulo, Brazil
  • 2Faculdade de Tecnologia, Universidade do Estado do Rio de Janeiro, Rodovia Presidente Dutra Km 298, Pólo Industrial, Resende, 27537-000 Rio de Janeiro, Brazil
  • 3Instituto de Física, Universidade de São Paulo, C.P 66318, São Paulo, 05314-970 São Paulo, Brazil
  • 4Research Center for Nuclear Physics (RCNP), Mihogaoka 10-1, Ibaraki 567-0047, Japan
  • 5Department of Physics, Nara Women’s University, Nara 630-8506, Japan

  • *kanchan.khemchandani@unifesp.br

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Issue

Vol. 97, Iss. 3 — 1 February 2018

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