https://doi.org/10.1140/epjp/s13360-025-06556-x
Regular Article
Thermodynamic properties of harmonically trapped sodium 23Na gas in one dimension
1
Department of Physics, Faculty of Science, The Hashemite University, 13133, Zarqa, Jordan
2
Department of Applied Physics, Tafila Technical University, 66110, Tafila, Jordan
3
Department of Physics, School of Science, The University of Jordan, 11942, Amman, Jordan
Received:
12
January
2025
Accepted:
16
June
2025
Published online:
1
July
2025
The static fluctuation approximation (SFA) is used to calculate the condensate fraction and thermodynamic properties of a harmonically trapped, one-dimensional interacting, 23Na gas. The interatomic interaction is a repulsive contact potential. A closed set of coupled nonlinear integral equations is derived and solved numerically as a first step for calculating the following thermodynamic properties: energy spectrum, particle distribution, correlations, and fluctuations. Based on these quantities, the condensate fraction , chemical potential
, energy per particle U/N (N being the total number of particles in the system), specific heat capacity cv, pressure P, and entropy S are calculated. The effects of the temperature T, longitudinal frequency
, and transverse frequency
on these properties are explored. Our findings indicate that at very low T,
is close to 0.55; at a specific T, it increases with
, but decreases with
. The
results show that the system is in the quantum regime at ‘low’ T and in the classical regime above the transition temperature Tc. The behavior of
with
and
shows that both
and Tc increase with
and
. U/N is parabolic with T and
, but is nearly linear with respect to
. P reaches saturation above Tc; it is parabolic with T and decreases with
, but shows linear behavior at ‘high’ values of
[(
Hz]. S increases with T and behaves more like P with
and
.
Copyright comment Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2025
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.