Static solutions of Einstein's field equations for spheres of fluid.

DOI10.1103/PHYSREV.55.364zbMath65.1048.02WikidataQ21709331 ScholiaQ21709331MaRDI QIDQ2593686

Richard C. Tolman

Publication date: 1939

Published in: Physical Review, II. Series (Search for Journal in Brave)

Related Items (18)

Impact of polytropic fluid on a usual gravitational source ⋮ Study of physical properties of charged compact star model in \(f(T)\) gravity ⋮ Decoupled anisotropic spheres in self-interacting Brans-Dicke gravity ⋮ Study of anisotropic strange stars in Krori Barua metric under \(f(T, \mathcal{T})\) gravity ⋮ Charged anisotropic fluid sphere in comparison with its uncharged analogue through extended geometric deformation ⋮ The wormhole model with an exponential shape function in the Finslerian framework ⋮ Charged strange stars with dust and phantom regimes in Rastall gravity ⋮ Charged anisotropic fluid sphere in \(f(\mathcal{R}, T)\) gravity ⋮ Existence of compact anisotropic stars with Karmarkar-Tolman spacetime ⋮ Mathematical modeling approach for compact objects: a new metric potential in the spherically symmetric system with Schwarzschild's coordinates ⋮ A study of compact stars within Rastall gravity ⋮ Electrobaryonic axion: hair of neutron stars ⋮ Energetic interaction between Einstein's universe and a source like-Tolman IV complexity factor ⋮ Black hole solutions with constant Ricci scalar in a model of Finsler gravity ⋮ Anisotropic quark stars in modified \(f(R, T)\) gravity utilizing Tolman V potential ⋮ Energy exchange between charged relativistic fluids in \(f(T)\) gravity ⋮ Dark energy stars in \(f(R, G)\) gravity ⋮ Configurations and deformations in relativistic elasticity

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