Numerical simulations of Gowdy-symmetric perturbations of decelerated FLRW Einstein-Euler solutions indicate finite-time shock formation for every linear equation of state p=K rho with 0<=K<=1.
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Instability of Slowly Expanding FLRW Spacetimes
Numerical simulations of Gowdy-symmetric perturbations of decelerated FLRW Einstein-Euler solutions indicate finite-time shock formation for every linear equation of state p=K rho with 0<=K<=1.