Stellar structure via truncated M-fractional Lane–Emden solutions

Stellar structure via truncated M-fractional Lane–Emden solutions

Abstract The Lane–Emden equation (LEE) is essential for modeling the structure of self-gravitating, spherically symmetric polytropic stars in hydrostatic equilibrium. Astronomy commonly employs it to depict normal stars, white dwarfs, and other celestial systems. This paper presents a new formulatio...

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Bibliographic Details
Main Authors: Mohamed I. Nouh, Emad A.-B. Abdel-Salam, Abaker A. Hassaballa, A. M. Awad, M. S. Jazmati, M. S. M. Bahgat
Format: Article
Language:English
Published: Nature Portfolio 2025-04-01
Series:Scientific Reports
Subjects:
Polytropic gas sphere
Lane–Emden equation
Truncated M-fractional derivative
White dwarfs
Online Access:https://doi.org/10.1038/s41598-025-96734-9
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https://doi.org/10.1038/s41598-025-96734-9

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