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Fractional incompressible stars
Date
2015-10-01
Author
Bayin, Selcuk S.
Krisch, Jean P.
Metadata
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
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In this paper we investigate the fractional versions of the stellar structure equations for non radiating spherical objects. Using incompressible fluids as a comparison, we develop models for constant density Newtonian objects with fractional mass distributions and/or stress conditions. To better understand the fractional effects, we discuss effective values for the density and equation of state. The fractional objects are smaller and less massive than integer models. The fractional parameters are related to a polytropic index for the models considered.
Subject Keywords
Fractional stars
,
Compact objects
,
Incompressible matter
,
Dense matter
,
Equation of state
,
Gravitation
URI
https://hdl.handle.net/11511/65411
Journal
ASTROPHYSICS AND SPACE SCIENCE
DOI
https://doi.org/10.1007/s10509-015-2499-9
Collections
Graduate School of Applied Mathematics, Article
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S. S. Bayin and J. P. Krisch, “Fractional incompressible stars,”
ASTROPHYSICS AND SPACE SCIENCE
, pp. 0–0, 2015, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/65411.