Pages that link to "Item:Q1164871"

The following pages link to Insufficiency of Karmarkar's condition (Q1164871):

Displaying 19 items.

• Some new similarity solutions of Einstein field equations for spherical symmetric metric of class two (Q298833) (← links)
• Anisotropic compact stellar model of embedding class-I satisfying Karmarkar's condition in Vaidya and Tikekar spheroidal geometry (Q2226072) (← links)
• Gravastars in \((3+1)\) dimensions admitting Karmarkar condition (Q2281046) (← links)
• Anisotropic charged compact star of embedding class I (Q4976099) (← links)
• All conformally flat Einstein–Gauss–Bonnet static metrics (Q5163308) (← links)
• A study on charged compact stars (Q5218280) (← links)
• A new class of relativistic model of compact stars of embedding class I (Q5363936) (← links)
• A charged anisotropic well-behaved Adler–Finch–Skea solution satisfying Karmarkar condition (Q5363953) (← links)
• f(R)$f(R)$ Wormholes Embedded in a Pseudo–Euclidean Space <i>E</i>⁵ (Q6091885) (← links)
• Embedding class-1 anisotropic solution in \(f(\mathcal{G})\) gravity (Q6204906) (← links)
• Anisotropic stars in Brans-Dicke gravity (Q6489931) (← links)
• Stellar modeling with the Einstein-Maxwell field equations via gravitational decoupling (Q6490588) (← links)
• Anisotropic stars of class one space-time in \(f(R, \mathcal{T})\) gravity under the simplest linear functional of the matter-geometry coupling (Q6542173) (← links)
• Physical behavior of anisotropic quark stars in modified \(f(R, T)\) gravity (Q6548505) (← links)
• Possibility of stable thin-shell around wormholes within string cloud and quintessential field via the van der Waals and polytropic EOS (Q6549016) (← links)
• Role of complexity on the minimal deformation of black holes (Q6584887) (← links)
• Stellar modeling with quintessence field via embedding approach in Rastall teleparallel gravity (Q6625056) (← links)
• Relativistic model for anisotropic compact stars in embedding class-I spacetime (Q6649801) (← links)
• Role of \(\mathscr{F}(\mathcal{Q}, \mathscr{T})\) gravity with class one space-time in constructing new spherically symmetric stellar solutions (Q6670819) (← links)