Spherically symmetric perturbation of an ultrarelativistic fluid in a homogeneous and isotropic universe

DOI10.1016/0375-9601(96)00524-5zbMath0972.83559arXivgr-qc/9604028OpenAlexW3100773420WikidataQ127293320 ScholiaQ127293320MaRDI QIDQ1967946

Yanyan Li

Publication date: 7 March 2000

Published in: Physics Letters. A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9604028

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (5)

A dynamic model of spherical perturbations in the Friedmann universe. II: Retarded solutions to an ultrarelativistic equation of state ⋮ Evolution of spherical perturbations in the cosmological environment of degenerate scalar-charged fermions with a scalar Higgs coupling ⋮ A dynamic model of spherical perturbations in the Friedmann universe. I ⋮ Spherically symmetric perturbations of spatially flat Friedmann models with imperfect fluid ⋮ A dynamic model of spherical perturbations in the Friedmann universe. III. Self-similar solutions

Cites Work

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• The Mass-Particle in an Expanding Universe

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