This investigation reveals new forms of instability defined by growth rates in Banach spaces, suggesting deeper understanding of dynamical systems.
In this paper, we investigate new forms of instability for linear discrete-time dynamical systems in Banach spaces, focusing on characterizations described by non-exponential growth rates. We introduce and analyze the concept of <a:math xmlns:a="http://www.w3.org/1998/Math/MathML"> <a:mi>h</a:mi> </a:math> -instability, where <b:math xmlns:b="http://www.w3.org/1998/Math/MathML"> <b:mi>h</b:mi> <b:mo>=</b:mo> <b:mo stretchy="false">(</b:mo> <b:msub> <b:mi>h</b:mi> <b:mi>n</b:mi> </b:msub> <b:msub> <b:mo stretchy="false">)</b:mo> <b:mrow class="MJX-TeXAtom-ORD"> <b:mi>n</b:mi> <b:mo> ∈ </b:mo> <b:mrow class="MJX-TeXAtom-ORD"> <b:mi mathvariant="double-struck">N</b:mi> </b:mrow> </b:mrow> </b:msub> </b:math> is a non-decreasing sequence that diverges to infinity. This formulation generalizes classical and nonuniform notions of exponential and polynomial instability by allowing for a variety of growth profiles. Our approach studies a linear system. We establish sufficient conditions for <h:math xmlns:h="http://www.w3.org/1998/Math/MathML"> <h:mi>h</h:mi> </h:math> -instability, investigate its connections with known instability concepts, and provide examples illustrating the sharpness of the results.
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C. Popa (2026) studied this question.
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