$Ξ_c(2790)^{+/0}$ and $Ξ_c(2815)^{+/0}$ radiative decays

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Hauptverfasser: García-Tecocoatzi, H., Ramirez-Morales, A., Rivero-Acosta, A., Santopinto, E., Vaquera-Araujo, C. A.
Format: Preprint
Veröffentlicht: 2025
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author García-Tecocoatzi, H.
Ramirez-Morales, A.
Rivero-Acosta, A.
Santopinto, E.
Vaquera-Araujo, C. A.
author_facet García-Tecocoatzi, H.
Ramirez-Morales, A.
Rivero-Acosta, A.
Santopinto, E.
Vaquera-Araujo, C. A.
contents In this work, we study the $Ξ_c$ baryon electromagnetic decay widths within the constituent quark model formalism through an analysis of the transitions from $P-$wave states to ground states. We use the non-relativistic limit of the Hamiltonian of the electromagnetic interaction on keeping all the terms up to the order $m_j^{-1}$. We calculate the electromagnetic decay widths analytically, for the first time, without any further approximation. Specifically, our theoretical results for the $Ξ_c(2790)^{+/0}$ and $Ξ_c(2815)^{+/0}$ radiative decay widths, without the introduction of any additional parameters, display a significant agreement with the recent experimental values obtained by the Belle experiment. The agreement is due to the fact that we have not introduced further approximation to simplify the calculation of the difficult convective term, unlike what was done in previous studies. Our predictions may be useful for future experiments at the Belle, BABAR, and LHC experiments.
format Preprint
id arxiv_https___arxiv_org_abs_2501_08798
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle $Ξ_c(2790)^{+/0}$ and $Ξ_c(2815)^{+/0}$ radiative decays
García-Tecocoatzi, H.
Ramirez-Morales, A.
Rivero-Acosta, A.
Santopinto, E.
Vaquera-Araujo, C. A.
High Energy Physics - Phenomenology
In this work, we study the $Ξ_c$ baryon electromagnetic decay widths within the constituent quark model formalism through an analysis of the transitions from $P-$wave states to ground states. We use the non-relativistic limit of the Hamiltonian of the electromagnetic interaction on keeping all the terms up to the order $m_j^{-1}$. We calculate the electromagnetic decay widths analytically, for the first time, without any further approximation. Specifically, our theoretical results for the $Ξ_c(2790)^{+/0}$ and $Ξ_c(2815)^{+/0}$ radiative decay widths, without the introduction of any additional parameters, display a significant agreement with the recent experimental values obtained by the Belle experiment. The agreement is due to the fact that we have not introduced further approximation to simplify the calculation of the difficult convective term, unlike what was done in previous studies. Our predictions may be useful for future experiments at the Belle, BABAR, and LHC experiments.
title $Ξ_c(2790)^{+/0}$ and $Ξ_c(2815)^{+/0}$ radiative decays
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2501.08798