Structure scalars and super-Poynting vector of tilted Szekeres geometry

DOI10.1142/S0218271815500145zbMath1311.83020OpenAlexW2086793200MaRDI QIDQ5249978

M. Zaeem Ul Haq Bhatti, Muhammad Sharif

Publication date: 13 May 2015

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271815500145

zbMATH Keywords

relativistic fluidsSzekeres modeltilted observer

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (2)

Shear and expansion evolution for dissipative fluids ⋮ Binding energy in self-gravitating charged plane symmetric systems

Cites Work

• Modelling inhomogeneity in Szekeres spacetime
• Radiation states and the problem of energy in general relativity
• Radiation and vorticity: the missing link
• Über Lösungen der Einsteinschen Feldgleichungen, die sich in einen fünfdimensionalen flachen Raum einbetten lassen
• Dynamics and stability of charged spherical star with tilted and non-tilted congruences
• Inhomogeneous cosmologies: New exact solutions and their evolution
• PHYSICAL CAUSES OF ENERGY DENSITY INHOMOGENIZATION AND STABILITY OF ENERGY DENSITY HOMOGENEITY IN RELATIVISTIC SELF-GRAVITATING FLUIDS
• General relativistic density perturbations

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