Order Stars
Chapter
Abstract
Order stars, discovered by searching for a better understanding of the stability properties of the Padé approximations to e z (Wanner, Hairer & Nørsett 1978), offered nice and unexpected access to many other results: the “second barrier” of Dahlquist, the Daniel & Moore conjecture, highest possible order with real poles, comparison of stability domains (Jeltsch & Nevanlinna 1981, 1982), order bounds for hyperbolic or parabolic difference schemes (e.g., Iserles & Strang 1983, Iserles & Williamson 1983, Jeltsch 1988).
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© Springer-Verlag Berlin Heidelberg 1996