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In this paper, we obtain optimal first order error estimates for a fully discrete fractional-step scheme applied to the Navier-Stokes equations. This scheme uses decomposition
of the viscosity in time and finite elements (FE) in space.
In [15], optimal first order error estimates (for velocity and pressure) for the corresponding time-discrete scheme were obtained, using in particular $H^2 \times H^1$ estimates for the approximations of
the velocity and pressure. Now, we use this time-discrete scheme as an auxiliary problem to study
a fully discrete finite element scheme, obtaining optimal first order approximation for velocity and
pressure with respect to the max-norm in time and the $H^1 \times L^2$-norm in space.
The proof of these error estimates are based on three main points: a) provide some new estimates
for the time-discrete scheme (not proved in [15]) which must be now used, b) give a discrete version
of the $H^2 \times H^1$ estimates in FE spaces, using stability in the $W^{1,6} \times L^6$-norm of the FE Stokes
projector, and c) the use of a weight function vanishing at initial time will let to hold the error
estimates without imposing global compatibility for the exact solution.
In this paper, we obtain optimal first order error estimates for a fully discrete fractional-step scheme applied to the Navier-Stokes equations. This scheme uses decomposition
of the viscosity in time and finite elements (FE) in space.
In [15], optimal first order error estimates (for velocity and pressure) for the corresponding time-discrete scheme were obtained, using in particular $H^2 \times H^1$ estimates for the approximations of
the velocity and pressure. Now, we use this time-discrete scheme as an auxiliary problem to study
a fully discrete finite element scheme, obtaining optimal first order approximation for velocity and
pressure with respect to the max-norm in time and the $H^1 \times L^2$-norm in space.
The proof of these error estimates are based on three main points: a) provide some new estimates
for the time-discrete scheme (not proved in [15]) which must be now used, b) give a discrete version
of the $H^2 \times H^1$ estimates in FE spaces, using stability in the $W^{1,6} \times L^6$-norm of the FE Stokes
projector, and c) the use of a weight function vanishing at initial time will let to hold the error
estimates without imposing global compatibility for the exact solution.