Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi Approximation

Self-gravitating Bose-Einstein condensates (BEC) have been proposed in various astrophysical contexts, including Bose-stars and BEC dark matter halos. These systems are described by a combination of the Gross-Pitaevskii and Poisson equations (the GPP system). In the analysis of these hypothetical ob...

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Main Author: Viktor T. Toth
Format: Article
Language:English
Published: MDPI AG 2016-08-01
Series:Galaxies
Subjects:
Online Access:http://www.mdpi.com/2075-4434/4/3/9
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author Viktor T. Toth
author_facet Viktor T. Toth
author_sort Viktor T. Toth
collection DOAJ
description Self-gravitating Bose-Einstein condensates (BEC) have been proposed in various astrophysical contexts, including Bose-stars and BEC dark matter halos. These systems are described by a combination of the Gross-Pitaevskii and Poisson equations (the GPP system). In the analysis of these hypothetical objects, the Thomas-Fermi (TF) approximation is widely used. This approximation is based on the assumption that in the presence of a large number of particles, the kinetic term in the Gross-Pitaevskii energy functional can be neglected, yet it is well known that this assumption is violated near the condensate surface. We also show that the total energy of the self-gravitating condensate in the TF-approximation is positive. The stability of a self-gravitating system is dependent on the total energy being negative. Therefore, the TF-approximation is ill suited to formulate initial conditions in numerical simulations. As an alternative, we offer an approximate solution of the full GPP system.
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spelling doaj.art-2e0cff58d3d945a892bd0cf7db375ef62022-12-21T21:45:59ZengMDPI AGGalaxies2075-44342016-08-0143910.3390/galaxies4030009galaxies4030009Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi ApproximationViktor T. Toth0Ottawa, ON K1N 9H5, CanadaSelf-gravitating Bose-Einstein condensates (BEC) have been proposed in various astrophysical contexts, including Bose-stars and BEC dark matter halos. These systems are described by a combination of the Gross-Pitaevskii and Poisson equations (the GPP system). In the analysis of these hypothetical objects, the Thomas-Fermi (TF) approximation is widely used. This approximation is based on the assumption that in the presence of a large number of particles, the kinetic term in the Gross-Pitaevskii energy functional can be neglected, yet it is well known that this assumption is violated near the condensate surface. We also show that the total energy of the self-gravitating condensate in the TF-approximation is positive. The stability of a self-gravitating system is dependent on the total energy being negative. Therefore, the TF-approximation is ill suited to formulate initial conditions in numerical simulations. As an alternative, we offer an approximate solution of the full GPP system.http://www.mdpi.com/2075-4434/4/3/9Bose-Einstein condensatesdark matter halos
spellingShingle Viktor T. Toth
Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi Approximation
Galaxies
Bose-Einstein condensates
dark matter halos
title Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi Approximation
title_full Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi Approximation
title_fullStr Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi Approximation
title_full_unstemmed Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi Approximation
title_short Self-Gravitating Bose-Einstein Condensates and the Thomas-Fermi Approximation
title_sort self gravitating bose einstein condensates and the thomas fermi approximation
topic Bose-Einstein condensates
dark matter halos
url http://www.mdpi.com/2075-4434/4/3/9
work_keys_str_mv AT viktorttoth selfgravitatingboseeinsteincondensatesandthethomasfermiapproximation