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Main Authors: Gutiérrez-Guerrero, L. X., Raya, Alfredo, Albino, L., Hernández-Pinto, R. J.
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2409.06057
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author Gutiérrez-Guerrero, L. X.
Raya, Alfredo
Albino, L.
Hernández-Pinto, R. J.
author_facet Gutiérrez-Guerrero, L. X.
Raya, Alfredo
Albino, L.
Hernández-Pinto, R. J.
contents We compute masses of twenty positive parity first radial excitations of spin-$1/2$ and $3/2$ baryons composed of u,d,s,c and b quarks in a quark-diquark picture within a contact interaction model. These excitations comprise of two elements: one characterized by a zero in the Faddeev amplitude, representing a radial excitation of the quark-diquark system and the other marked by a zero in the diquark's Bethe-Salpeter amplitude, corresponding to an intrinsic excitation of the diquark correlation. Wherever possible, we compare our results with other models and/or experiment. We verify that the masses obtained through our model conform to the spacing rules for all the baryons studied, whether light or heavy and whether of spin 1/2 or 3/2. The computed masses do not just offer a guide to the future experimental searches but also compare well with the existing candidates for the possible radial excitations of some heavy baryons.
format Preprint
id arxiv_https___arxiv_org_abs_2409_06057
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle First Radial Excitations of Baryons in a Contact Interaction: Mass Spectrum
Gutiérrez-Guerrero, L. X.
Raya, Alfredo
Albino, L.
Hernández-Pinto, R. J.
High Energy Physics - Phenomenology
We compute masses of twenty positive parity first radial excitations of spin-$1/2$ and $3/2$ baryons composed of u,d,s,c and b quarks in a quark-diquark picture within a contact interaction model. These excitations comprise of two elements: one characterized by a zero in the Faddeev amplitude, representing a radial excitation of the quark-diquark system and the other marked by a zero in the diquark's Bethe-Salpeter amplitude, corresponding to an intrinsic excitation of the diquark correlation. Wherever possible, we compare our results with other models and/or experiment. We verify that the masses obtained through our model conform to the spacing rules for all the baryons studied, whether light or heavy and whether of spin 1/2 or 3/2. The computed masses do not just offer a guide to the future experimental searches but also compare well with the existing candidates for the possible radial excitations of some heavy baryons.
title First Radial Excitations of Baryons in a Contact Interaction: Mass Spectrum
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2409.06057