2012
DOI: 10.1016/j.na.2011.05.064
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The Denjoy–Wolff theorem in

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Cited by 23 publications
(15 citation statements)
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“…Busemann sequences have been introduced (under the name horosphere sequences) in balanced bounded convex domains in [28], and later studied in bounded convex domains in [14]. The proof of the following result is an adaptation of the ideas contained in those papers.…”
Section: Admissible Sequences Busemann Sequences and Horosphere Bounmentioning
confidence: 99%
See 1 more Smart Citation
“…Busemann sequences have been introduced (under the name horosphere sequences) in balanced bounded convex domains in [28], and later studied in bounded convex domains in [14]. The proof of the following result is an adaptation of the ideas contained in those papers.…”
Section: Admissible Sequences Busemann Sequences and Horosphere Bounmentioning
confidence: 99%
“…In this paper we introduce a completely new prime ends theory defined via horospheres related to sequences. Horospheres have been used pretty much in geometric function theory in one and several variables, especially for studying iteration theory, Julia's Lemma, Denjoy-Wolff theorems (see, e.g., [1,3,4,14,15,37,21] and references therein), and they are a particular instance of a general notion of horospheres in locally complete metric spaces, see [17,6]. In complex geometry, horospheres defined by using complex geodesics are sometimes called Busemann horospheres.…”
Section: Introductionmentioning
confidence: 99%
“…In a Hilbert space ellipsoids replace the internally tangent discs [18]. In strictly convex domains, in C n [1,2,7], or in Banach spaces [9,10], the internally tangent discs are replaced by horospheres defined in terms of the Kobayashi distance. Although these horospheres are defined for arbitrary Banach spaces [2,3,32], if the boundary of the ball is more complicated they are considerably less tractable, even in finite dimensions [17,4,16].…”
Section: Introductionmentioning
confidence: 99%
“…Although these horospheres are defined for arbitrary Banach spaces [2,3,32], if the boundary of the ball is more complicated they are considerably less tractable, even in finite dimensions [17,4,16]. While holomorphic iteration on both finite and infinite dimensional Banach spaces has recently continued apace [5,7,8,9,11,12,20,28,31,32,34], spaces whose balls have, for example, non-strictly convex boundaries, even classical spaces such as the C * -algebras or L(H, K), still require a Wolff theorem and concrete descriptions of invariant domains to facilitate progress on iteration.…”
Section: Introductionmentioning
confidence: 99%
“…Small horospheres might be too small; as shown by Frosini [F], there are holomorphic self-maps of the polydisk with no invariant small horospheres. We thus need another kind of horospheres, defined by Kapeluszny, Kuczumow and Reich [KKR2], and studied in detail by Budzyńska [Bu2]. To introduce them we begin with a definition:…”
mentioning
confidence: 99%