Chandrasekhar, S. (1962) On the point of bifurcation along the sequence of the Jacobi ellipsoids Astrophysical Journal, 136 . pp. 1048-1068. ISSN 0004-637X
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Official URL: http://adsabs.harvard.edu/doi/10.1086/147457
Related URL: http://dx.doi.org/10.1086/147457
Abstract
In this paper, the known point of bifurcation along the sequence of the Jacobi ellipsoids is isolated by a new method based on equilibrium considerations only. The method consists in finding an integral property (or, more generally, a functional) of the configuration which vanishes as a condition of equilibnum. The first variation of such a functional will vamsh at a point of bifurcation (and only at a point of bifurcation) for a Lagrangian displacement which deforms the body from the shape it has along an equilibrium sequence to the shape it will have in the sequence following bifurcation. For finding a func tional J with the requisite properties, an equation for the third-order virial (namely, ∫ρuixixkdx) is first established, And from an examination of the conditions, which follow from this equation, for equilibrium, it is found that J = ∫vρ [x3 B13+ x2Bl2+ xl (B33 - B22)] dx (where Bij is the tensor potential of the gravitational field) has all the necessary properties The first variation of J, for the Lagrangian displacement which deforms a Jacobi ellipsoid into a pear-shaped object, is then evaluated, and it is shown that its vanishing determines the point of bifurcation along the Jacobian sequence, in agreement with Darwin's result.
Item Type: | Article |
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Source: | Copyright of this article belongs to American Astronomical Society. |
ID Code: | 73402 |
Deposited On: | 03 Dec 2011 12:23 |
Last Modified: | 18 May 2016 18:15 |
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