Nonlinear equations in radiating stellar structures
From MaRDI portal
Publication:5354898
DOI10.1063/1.4995394zbMath1370.85002OpenAlexW2739630794MaRDI QIDQ5354898
R. Narain, R. Mohanlal, Sunil D. Maharaj
Publication date: 5 September 2017
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.4995394
Relativistic cosmology (83F05) Galactic and stellar structure (85A15) Radiative transfer in astronomy and astrophysics (85A25) PDEs in connection with astronomy and astrophysics (35Q85)
Related Items (3)
Transformation method for generating periodic solutions of Abel's differential equation ⋮ A generating function and new exact solutions for geodesic matter ⋮ Bifurcations of the Riccati Quadratic Polynomial Differential Systems
Cites Work
- Unnamed Item
- Unnamed Item
- New shear-free relativistic models with heat flow
- A general class of Euclidean stars
- Collapsing spheres satisfying an ``Euclidean condition
- Radiating stars with exponential Lie symmetries
- Generalized Euclidean stars with equation of state
- Geodesic models generated by Lie symmetries
- A different approach to anisotropic spherical collapse with shear and heat radiation
- Riccati equations for bounded radiating systems
- Shearing radiative collapse with expansion and acceleration
- Noether and Lie symmetries for charged perfect fluids
- Collapse of a radiating star
- More about collapse of a radiating star
- Inhomogeneous Cosmological Models
- The influence of an equation-of-state during radiative collapse
- Gravitational Collapse and Spacetime Singularities
- Symmetries and differential equations
This page was built for publication: Nonlinear equations in radiating stellar structures
