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- W2049525169 abstract "Both the truncated and the full version of the causal thermodynamic theory of nonequilibrium phenomena are used to study the evolution of a Bianchi type-III cosmological model. The initial anisotropy dies away rapidly and the de Sitter solutions are stable while the Friedmann ones are not." @default.
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- W2049525169 title "Dissipative effects in Bianchi type-III cosmologies" @default.
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- W2049525169 doi "https://doi.org/10.1103/physrevd.50.2572" @default.
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