Constraining the mass and width of the N*(1685) resonance

T. Mart
Phys. Rev. D 88, 057501 – Published 30 September 2013

Abstract

We have examined the existence of the N*(1685) resonance, which is recently listed by the Particle Data Group as a one-star nucleon resonance, by using a covariant isobar model for kaon photoproduction and assuming that the resonance has Jp=1/2+, in accordance with our previous finding. After the inclusion of this resonance, the changes in the total χ2 show two clear minima at MN*=1650 and 1696 MeV, which correspond to two different resonance states. The former corresponds to the narrow nucleon resonance found in our previous investigation, whereas the latter corresponds to a new resonance found as we increase the resonance width. From the latter we derive the mass and width relation of the N*(1685) resonance. We observe that the properties of both the N*(1685) and N*(1710)P11 resonances are strongly correlated. Although the best fit of the present work yields MN*=1696MeV and ΓN*=76MeV, the apparently small N*(1710)P11 coupling constant to the K+Λ channel found in previous investigations suggests that ΓN*35MeV, which, according to the mass and width relation, corresponds to MN*1680MeV.

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  • Received 12 August 2013

DOI:https://doi.org/10.1103/PhysRevD.88.057501

© 2013 American Physical Society

Authors & Affiliations

T. Mart

  • Departemen Fisika, FMIPA, Universitas Indonesia, Depok 16424, Indonesia

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Issue

Vol. 88, Iss. 5 — 1 September 2013

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