Cylindrically symmetric distributions of matter taking into account pressure

This paper considers a non-steady-state cosmological field for describing the distribution of matter with nonzero pressure; the assumption of cylindrical symmetry is taken into consideration. A new class of non-steady-state solutions to the Einstein equations is found. A homogeneous, anisotropic universe and an analog of the Schwarzschild solution are considered as particular cases. The obtained results can be used for describing cylindrical regions in the universe, especially in the vicinity of linear mass ejection from galaxies and quasars and linear super-large-scale structures