The Positive Solutions of the Matukuma Equation and the Problem of Finite Radius and Finite Mass |
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Authors: | Jürgen Batt Yi Li |
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Institution: | 1. Mathematisches Institut, der Universit?t München, Theresienstr. 39, 80333, München, Germany 2. Department of Mathematics, University of Iowa, Iowa City, Iowa, 52242, USA 3. Department of Mathematics, Xian Jiaotong University, Xian, Shannxi, China
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Abstract: | This work is an extensive study of the 3 different types of positive solutions of the Matukuma equation ${\frac{1}{r^{2}}\left( r^{2}\phi^{\prime}\right) ^{\prime}=-{\frac{r^{\lambda-2}}{\left( 1+r^{2}\right)^{\lambda /2}}}\phi^{p},p >1 ,\lambda >0 }${\frac{1}{r^{2}}\left( r^{2}\phi^{\prime}\right) ^{\prime}=-{\frac{r^{\lambda-2}}{\left( 1+r^{2}\right)^{\lambda /2}}}\phi^{p},p >1 ,\lambda >0 }: the E-solutions (regular at r = 0), the M-solutions (singular at r = 0) and the F-solutions (whose existence begins away from r = 0). An essential tool is a transformation of the equation into a 2-dimensional asymptotically autonomous system, whose
limit sets (by a theorem of H. R. Thieme) are the limit sets of Emden–Fowler systems, and serve as to characterizate the different
solutions. The emphasis lies on the study of the M-solutions. The asymptotic expansions obtained make it possible to apply the results to the important question of stellar
dynamics, solutions to which lead to galactic models (stationary solutions of the Vlasov–Poisson system) of finite radius
and/or finite mass for different p, λ. |
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