New exact anisotropic static spherically symmetric stellar models satisfying the Eiesland condition

DOI10.1016/j.aop.2019.01.007zbMath1409.83031OpenAlexW2909505765WikidataQ128578893 ScholiaQ128578893MaRDI QIDQ1732559

Mohammad Hassan Murad, Saba Fatema, Ksh. Newton Singh

Publication date: 25 March 2019

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.aop.2019.01.007

zbMATH Keywords

stabilityrelativistic star: structure

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (2)

Description of the interior of the neutron star in EXO 1785-248 by mean of the Karmarkar condition ⋮ An analytical anisotropic compact stellar model of embedding class I

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• Unnamed Item
• Unnamed Item
• A new relativistic stellar model with anisotropic fluid in Karmarkar space-time
• Compact stars with specific mass function
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• The contraction of gravitating spheres

This page was built for publication: New exact anisotropic static spherically symmetric stellar models satisfying the Eiesland condition