@Article{Nieves+Pavao2020,
author="Nieves, J.
and Pavao, R.",
title="Nature of the lowest-lying odd parity charmed baryon Lambda(c)(2595) and Lambda(c)(2625) resonances",
journal="Physical Review D",
year="2020",
publisher="Amer Physical Soc",
volume="101",
number="1",
pages="014018--17pp",
abstract="We study the structure of the Lambda(c) (2595) and Lambda(c) (2625) resonances in the framework of an effective field theory consistent with heavy quark spin and chiral symmetries, which incorporates the interplay between Sigma(()(c)*() )pi -- ND(*()) baryon-meson degrees of freedom (d.o.f.) and bare P-wave c (u) over bard quark-model states. We show that these two resonances are not heavy quark spin symmetry partners. The J(P) = 3/2(-) Lambda(c) (2625) should be viewed mostly as a dressed three-quark state, whose origin is determined by a bare state, predicted to lie very close to the mass of the resonance. The J(P) = 1/2(-) Lambda(c) (2595) seems to have, however, a predominant molecular structure. This is because it is either the result of the chiral Sigma(c)pi interaction, whose threshold is located much closer than the mass of the bare three-quark state, or because the light d.o.f. in its inner structure are coupled to the unnatural 0(-) quantum numbers. We show that both situations can occur depending on the renormalization procedure used. We find some additional states, but the classification of the spectrum in terms of heavy quark spin symmetry is difficult, despite having used interactions that respect this symmetry. This is because the bare quark-model state and the Sigma(c)pi threshold are located extraordinarily close to the Lambda(c) (2625) and Lambda(c) (2595), respectively, and hence they play totally different roles in each sector.",
optnote="WOS:000509494900007",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=4272), last updated on Sun, 16 Feb 2020 16:58:13 +0000",
issn="2470-0010",
doi="10.1103/PhysRevD.101.014018",
opturl="https://arxiv.org/abs/1907.05747",
opturl="https://doi.org/10.1103/PhysRevD.101.014018",
language="English"
}