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Asymptotic solutions for the Clairaut equation in the theory of rotating fluid masses

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Abstract

A procedure has been devised to construct a solution of the Clairaut equation in the form of an asymptotic expansion in terms of descending powers of\(\lambda = j + \tfrac{1}{2}\), wherej denotes the order of spherical-harmonic distortion. It has been shown that asj and, therefore λ increases, the foregoing series approaches asymptotically a solution of our equation. The procedure is similar to the WKB-method of theoretical physics.

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References

  • Birkhoff, G. D.: 1908,Trans. Am. Math. Soc. 9, 219–231.

    Google Scholar 

  • Cesari, L.: 1963,Asymptotic Behavior and Stability Problems in Ordinary Differential Equations, Academic Press, New York.

    Google Scholar 

  • Kopal, Z.: 1960,Figures of Equilibrium of Celestial Bodies, Univ. of Wisconsin Press, Madison.

    Google Scholar 

  • Langer, R. E.: 1934,Bull. Am. Math. Soc. 40, 545–582.

    Google Scholar 

  • Lanzano, P.: 1973, ‘Certain Particular Solutions of the Clairaut Equation’,Astrophys. Space Sci. 20, 71–83.

    Google Scholar 

  • Wentzel, G.: 1926,Z. Phys. 38, 518–529.

    Google Scholar 

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Kopal, Z., Lanzano, P. Asymptotic solutions for the Clairaut equation in the theory of rotating fluid masses. Astrophys Space Sci 23, 425–429 (1973). https://doi.org/10.1007/BF00645169

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  • DOI: https://doi.org/10.1007/BF00645169

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