Maclaurin spheroid in disguise: New figures of equilibrium with external magnetic support

We show that a rigidly rotating, homogeneous ellipsoid of revolution threaded by a uniform, coaxial magnetic field is a possible figure of equilibrium. While the spheroidal shape is fully preserved, the rotation rate is modified. Accordingly, we extend the fundamental formula by Maclaurin. In contrast with the nonmagnetic case, prolate shapes are permitted, but there are critical states in the form of maximum elongations, depending on ionization fraction, ion/electron drift, magnetic field, and mass density. As checked from numerical simulations based on the self-consistent-field method, prolate states survive to gas compressibility. The relevance to interstellar clouds is outlined.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-09-10
DOI
https://doi.org/10.1103/physrevd.110.063017
Citations
1
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.33
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article

Maclaurin spheroid in disguise: New figures of equilibrium with external magnetic support

J.-M. Huré, Clément Staelen
1 citations
Physical review. D/Physical review. D.
Stellar, planetary, and galactic studies
0.33
article

Maclaurin spheroid in disguise: New figures of equilibrium with external magnetic support

J.-M. Huré, Clément Staelen
article en
1 citations

Abstract

We show that a rigidly rotating, homogeneous ellipsoid of revolution threaded by a uniform, coaxial magnetic field is a possible figure of equilibrium. While the spheroidal shape is fully preserved, the rotation rate is modified. Accordingly, we extend the fundamental formula by Maclaurin. In contrast with the nonmagnetic case, prolate shapes are permitted, but there are critical states in the form of maximum elongations, depending on ionization fraction, ion/electron drift, magnetic field, and mass density. As checked from numerical simulations based on the self-consistent-field method, prolate states survive to gas compressibility. The relevance to interstellar clouds is outlined.

Physical review. D/Physical review. D.Vol. 110(6)
Université de Bordeaux (FR), Laboratoire d'Astrophysique de Bordeaux (FR), Centre Émile Durkheim (FR)
Openalex Percentile: Top 35%
Stellar, planetary, and galactic studies
0.33
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