Saved in:
Bibliographic Details
Main Authors: Ayon, Amanda Castillo, Pérez, Gabriel Gil, Martinez, Aurora Pérez, Rojas, H. Pérez, Bocchi, Gabriella Piccinelli, Concepcion, Adriel Rodriguez, Sanchez, Angel
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2508.16799
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866912558589411328
author Ayon, Amanda Castillo
Pérez, Gabriel Gil
Martinez, Aurora Pérez
Rojas, H. Pérez
Bocchi, Gabriella Piccinelli
Concepcion, Adriel Rodriguez
Sanchez, Angel
author_facet Ayon, Amanda Castillo
Pérez, Gabriel Gil
Martinez, Aurora Pérez
Rojas, H. Pérez
Bocchi, Gabriella Piccinelli
Concepcion, Adriel Rodriguez
Sanchez, Angel
contents We study the thermodynamic properties of a non-interacting, relativistic gas of charged scalar bosons in a uniform magnetic field, including both statistical and vacuum contributions at arbitrary field strengths. Focusing on the low-temperature regime and separating the Lowest Landau Level (LLL) from excited states provides a clearer view of the magnetic field's impact on thermodynamic quantities. We revisit Bose Einstein condensation (BEC), specific heat, magnetization, and the equation of state (EoS). A central result is the diffuse character of BEC induced by the magnetic field, reflected in the specific heat, which exhibits two plateaus: the first appears when the system becomes effectively one-dimensional through magnetic confinement, while the second-associated with the true one-particle ground state-is suppressed by the field. Consequently, no critical condensation temperature arises. For magnetization, the LLL contribution shifts from diamagnetic to paramagnetic As the field strengthen with the inclusion of the excited states, the statistical magnetization remains negative. In contrast, the vacuum contribution dominates at strong fields, driving paramagnetic. We also show that antiparticles enhance specific heat, magnetization, and total pressure. These effects are illustrated for a pion gas under neutron star conditions and compared with previous results for a neutral vector boson system.
format Preprint
id arxiv_https___arxiv_org_abs_2508_16799
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Two-Step Bose-Einstein Condensation of an ideal Magnetized Charged Bosonic gas under neutron star-like conditions
Ayon, Amanda Castillo
Pérez, Gabriel Gil
Martinez, Aurora Pérez
Rojas, H. Pérez
Bocchi, Gabriella Piccinelli
Concepcion, Adriel Rodriguez
Sanchez, Angel
High Energy Astrophysical Phenomena
Quantum Gases
Statistical Mechanics
We study the thermodynamic properties of a non-interacting, relativistic gas of charged scalar bosons in a uniform magnetic field, including both statistical and vacuum contributions at arbitrary field strengths. Focusing on the low-temperature regime and separating the Lowest Landau Level (LLL) from excited states provides a clearer view of the magnetic field's impact on thermodynamic quantities. We revisit Bose Einstein condensation (BEC), specific heat, magnetization, and the equation of state (EoS). A central result is the diffuse character of BEC induced by the magnetic field, reflected in the specific heat, which exhibits two plateaus: the first appears when the system becomes effectively one-dimensional through magnetic confinement, while the second-associated with the true one-particle ground state-is suppressed by the field. Consequently, no critical condensation temperature arises. For magnetization, the LLL contribution shifts from diamagnetic to paramagnetic As the field strengthen with the inclusion of the excited states, the statistical magnetization remains negative. In contrast, the vacuum contribution dominates at strong fields, driving paramagnetic. We also show that antiparticles enhance specific heat, magnetization, and total pressure. These effects are illustrated for a pion gas under neutron star conditions and compared with previous results for a neutral vector boson system.
title Two-Step Bose-Einstein Condensation of an ideal Magnetized Charged Bosonic gas under neutron star-like conditions
topic High Energy Astrophysical Phenomena
Quantum Gases
Statistical Mechanics
url https://arxiv.org/abs/2508.16799