Abstract

We extract the excitation energy scales of the hadron spectra in a less model-dependent method using Schottky anomaly. Schottky anomaly is a thermodynamical phenomenon that the specific heat of a system consisting of a finite number of energy levels has a peak at finite temperature due to the energy gaps. Using the masses of all hadrons that are experimentally established, we obtain the excitation energy scales of the hadron spectra and investigate their flavor dependence.

Highlights

  • Understanding the hadron structure is one of the important subjects in hadron physics

  • In the heavy meson systems, we have found two energy scales for hyperfine structure by spin-spin interaction and the orbital excitation by central potential

  • Comparing the results of charmonium and bottomonium, we find that the energy scale of the orbital excitation is about 440 MeV, and it is insensitive to the flavor of the heavy mesons

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Summary

INTRODUCTION

Understanding the hadron structure is one of the important subjects in hadron physics. To identify effective degrees of freedom in composite objects, it is good to investigate excitation modes We visualize the excitation energy scales in various hadronic spectra in a less model-dependent way by examining specific heats obtained by hadronic mass spectra. This method is used widely in different areas. Reference [7] first applied for hadron physics to extract the effective degrees of freedom of the constituent of a hadron This is based on the fact that the specific heat of a system is closely related to dynamical degrees of freedom in thermodynamics. IV is devoted to a summary of this work and future prospects

SCHOTTKY ANOMALY
Two-state system
N-state systems
Analysis of calculated data
APPLICATION TO HADRON
Heavy mesons
Heavy quarkonia
Open charm and open bottom mesons
Summary of heavy mesons
Light mesons
Baryons
Heavy baryons
Discussion for the baryon system
Findings
Excitation energy scales for positive and negative parity hadrons
SUMMARY
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