A cosmological model of the universe, filled with perfect fluid with nonlinear, unhomogenous equation of state

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The square equation of state is applied to modeling of the cosmological parameters. Phantom and unphantom phases are found and investigated. There is an assessment of their dependence on the phenomenological coefficients in the equation of state.

Cosmological expansion with acceleration

Короткий адрес: https://sciup.org/14729891

IDR: 14729891

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