The concept of reduced variables is revisited with regard to van der Waals’ theory and an application is made to polytropic spheres, where the reduced radial coordinate is , R radius, and the reduced density is , central density. Reduced density profiles are plotted for several polytropic indexes within the range, 0≤n≤5, disclosing two noticeable features. First, any point of coordinates, (w, v), 0≤w≤1, 0≤v≤1, belongs to a reduced density profile of the kind considered. Second, sufficiently steep i.e. large reduced density profiles exhibit an oblique inflection point, where the threshold is found to be located at n=nth=0.888715. Reduced pressure profiles,, central pressure, Lane-Emden fucntions, , and polytropic curves,?q=q(v), are also plotted. The method can be extended to nonspherical polytropes with regard to a selected direction,.?The results can be extended to polytropic spheres made of collisionless particles, for polytropic index within a more restricted range,?1/2≤n≤5 .
References
[1]
Jeans, J. (1929) Astronomy and Cosmogony. Dover Publications, New York.
[2]
Chandrasekhar, S. (1939) An Introduction to the Study of the Stellar Structure. University of Chicago Press, Chicago.
[3]
Horedt, G.P. (2004) Polytropes: Applications in Astrophysics and Related Fields. Kluver Academic Publishers, Dordrecht.
[4]
Plummer, H.C. (1911) On the Problem of Distribution in Globular Star Clusters. Monthly Notices of the Royal Astronomical Society, 71, 460-470. http://dx.doi.org/10.1093/mnras/71.5.460
[5]
Caimmi, R. (2010) A Principle of Corresponding States for Two-Component, Self-Gravitating Fluids. Serbian Astronomical Journal, 180, 19-55. http://dx.doi.org/10.2298/SAJ1080019C
[6]
Caimmi, R. (2012) Tidal Interactions and Principle of Corresponding States: From Micro to Macro Cosmos. A Century after van der Waals’ Nobel Prize. http://arxiv.org/pdf/1210.3688.pdf
[7]
Rostagni, A. (1957) Meccanica e Termodinamica. Ed. Libreria Universitaria di G. Randi, Padova.
[8]
Landau, L.D. and Lifshitz, E.M. (1967) Physique Statistique. Mir, Moscow.
[9]
van der Waals, J.D. (1873) Over de Continuited van den Gas-en Vloeistoftoestand. Doctoral Thesis, University of Leiden, Leiden.
[10]
Caimmi, R. (1980) Emden-Chandrasekhar Axisymmetric, Solid-Body Rotating Polytropes. I—Exact Solutions for the Special Cases N Equals 0, 1 and 5. Astrophysics and Space Science, 71, 415-457.
[11]
Caimmi, R. (1983) Emden-Chandrasekhar Axisymmetric, Solid-Body Rotating Polytropes. II—Power Series Solutions to EC Associated Equations of Degree 0 and 2. Astrophysics and Space Science, 89, 255-277. http://dx.doi.org/10.1007/BF00655979
[12]
Horedt, G.P. (1986) Seven-Digit Tables of Lane-Emden Functions. Astrophysics and Space Science, 126, 357-408. http://dx.doi.org/10.1007/BF00639386
[13]
Caimmi, R. (1985) Emden-Chandrasekhar Axisymmetric, Rigidly Rotating Polytropes. III—Determination of Equilibrium Configurations by an Improvement of Chandrasekhar’s Method. Astrophysics and Space Science, 113, 125-142. http://dx.doi.org/10.1007/BF00650276
[14]
Vandervoort, P.O. (1980) The Nonaxisymmetric Configurations of Uniformly Rotating Polytropes. The Astrophysical Journal, 241, 316-333. http://dx.doi.org/10.1086/158344