Refining radiative decay studies in singly heavy baryons

TL;DR

This paper improves the theoretical understanding of radiative decays in singly heavy baryons by employing numerical wave functions from the Gaussian expansion method, aiming to support high-precision hadron spectroscopy.

Contribution

It introduces a systematic study using numerical spatial wave functions for more accurate calculations of radiative decays in singly heavy baryons.

Findings

Enhanced accuracy in decay rate calculations

Provides detailed mass spectrum of singly heavy baryons

Supports high-precision spectroscopic analysis

Abstract

In this work, we systematically study the radiative decays of singly heavy baryons, a crucial aspect of their spectroscopic behavior. To enhance the accuracy of our calculations, we utilize numerical spatial wave functions for the singly heavy baryons obtained through the Gaussian expansion method, which also yields their mass spectrum. As hadron spectroscopy enters an era of high precision, we believe our study of the radiative decays of singly heavy baryons will provide valuable insights for further exploration of these particles.