Effects of external field and potential on non-relativistic quantum particles in disclinations background

TL;DR

This paper analyzes how external fields and potentials influence non-relativistic quantum particles in a cosmic string background, deriving eigenvalues, exploring thermodynamic properties, and examining particle localization through entropy.

Contribution

It provides analytical solutions for quantum particles in a cosmic string background considering various potentials and fields, including thermodynamic and entropy analysis at finite temperatures.

Findings

Eigenvalue solutions for quantum particles in cosmic string space-time

Thermodynamic properties and partition functions at non-zero temperature

Insights into particle localization via entropic measures

Abstract

In this work, we investigate the behavior of non-relativistic quantum particles immersed in a cosmic string space-time background. Our study involves the examination of these particles as they interact with a range of influences, including potential, magnetic, and quantum flux fields. We employ analytical methods to solve the associated wave equation, leading to the derivation of eigenvalue solutions for this quantum system. Subsequently, we leverage these eigenvalue solutions to scrutinize several potential models. For each model, we present and engage in a thorough discussion of the corresponding eigenvalue solutions. In an extension of our investigation, we explore the thermodynamic and magnetic properties of the quantum system when it is exposed to non-zero temperature conditions, denoted by $T \neq 0$. Our analysis encompasses the calculation of essential parameters such as the partition function for the system and other pertinent functions. Following these calculations, we meticulously examine and interpret the outcomes, shedding light on the system's behavior and characteristics in the presence of temperature variations. Furthermore, we calculate entropic information to investigate the location of particles in the system.