Irene Kyza
University of Dundee
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Publication
Featured researches published by Irene Kyza.
Numerische Mathematik | 2013
Andrea Bonito; Irene Kyza; Ricardo H. Nochetto
We derive optimal a priori error estimates for discontinuous Galerkin (dG) time discrete schemes of any order applied to an advection–diffusion model defined on moving domains and written in the Arbitrary Lagrangian Eulerian (ALE) framework. Our estimates hold without any restrictions on the time steps for dG with exact integration or Reynolds’ quadrature. They involve a mild restriction on the time steps for the practical Runge–Kutta–Radau methods of any order. The key ingredients are the stability results shown earlier in Bonito et al. (Time-discrete higher order ALE formulations: stability, 2013) along with a novel ALE projection. Numerical experiments illustrate and complement our theoretical results.
SIAM Journal on Numerical Analysis | 2011
Irene Kyza; Charalambos Makridakis
We prove a posteriori error estimates for time discrete approximations, for semilinear parabolic equations with solutions that might blow up in finite time. In particular we consider the backward Euler and the Crank-Nicolson methods. The main tools that are used in the analysis are the reconstruction technique and energy methods combined with appropriate fixed point arguments. The final estimates we derive are conditional and lead to error control near the blow up time.
SIAM Journal on Scientific Computing | 2016
Andrea Cangiani; Emmanuil H. Georgoulis; Irene Kyza; Stephen Metcalfe
This work is concerned with the development of a space-time adaptive numerical method, based on a rigorous a posteriori error bound, for a semilinear convection-diffusion problem which may exhibit blow-up in finite time. More specifically, a posteriori error bounds are derived in the
Numerische Mathematik | 2015
Theodoros Katsaounis; Irene Kyza
L^{\infty}(L^2)+L^2(H^1)
Journal of Scientific Computing | 2018
Irene Kyza; Stephen Arthur Metcalfe; Thomas P. Wihler
-type norm for a first order in time implicit-explicit interior penalty discontinuous Galerkin in space discretization of the problem, although the theory presented is directly applicable to the case of conforming finite element approximations in space. The choice of the discretization in time is made based on a careful analysis of adaptive time-stepping methods for ODEs that exhibit finite time blow-up. The new adaptive algorithm is shown to accurately estimate the blow-up time of a number of problems, including one which exhibits regional blow-up.
Archive | 2014
Andrea Bonito; Irene Kyza; Ricardo H. Nochetto
We derive optimal order a posteriori error estimates for fully discrete approximations of linear Schrödinger-type equations, in the
SIAM Journal on Numerical Analysis | 2013
Andrea Bonito; Irene Kyza; Ricardo H. Nochetto
Ima Journal of Numerical Analysis | 2011
Irene Kyza; Charalambos Makridakis; Michael Plexousakis
L^\infty (L^2)
Mathematical Modelling and Numerical Analysis | 2011
Irene Kyza
SIAM Journal on Numerical Analysis | 2018
Theodoros Katsaounis; Irene Kyza
L∞(L2)-norm. For the discretization in time we use the Crank–Nicolson method, while for the space discretization we use finite element spaces that are allowed to change in time. The derivation of the estimators is based on a novel elliptic reconstruction that leads to estimates which reflect the physical properties of Schrödinger equations. The final estimates are obtained using energy techniques and residual-type estimators. Various numerical experiments for the one-dimensional linear Schrödinger equation in the semiclassical regime, verify and complement our theoretical results. The numerical implementations are performed with both uniform partitions and adaptivity in time and space. For adaptivity, we further develop and analyze an existing time-space adaptive algorithm to the cases of Schrödinger equations. The adaptive algorithm reduces the computational cost substantially and provides efficient error control for the solution and the observables of the problem, especially for small values of the Planck constant.