2015
DOI: 10.1142/s2010326315500161
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Symmetries of the Feinberg–Zee random hopping matrix

Abstract: We study the symmetries of the spectrum of the Feinberg-Zee Random Hopping Matrix introduced in [6] and studied in various papers therafter (e.g.[1], [2], [3], [7], [9]). In [3], Chandler-Wilde and Davies proved that the spectrum of the Feinberg-Zee Random Hopping Matrix is invariant under taking square roots, which implied that the unit disk is contained in the spectrum (a result already obtained slightly earlier in [1]). In a similar approach we show that there is an infinite sequence of symmetries at least … Show more

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Cited by 9 publications
(33 citation statements)
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“…Moreover, it was shown in [5] that π ∞ is dense in the unit disk D := {z ∈ C : |z| ≤ 1}, i.e. clos(π ∞ ) ∩ D = D. This result was improved to a larger set in [10]. Our new result here implies that σ ∞ is dense in this particular set as well.…”
Section: Introductionmentioning
confidence: 50%
See 2 more Smart Citations
“…Moreover, it was shown in [5] that π ∞ is dense in the unit disk D := {z ∈ C : |z| ≤ 1}, i.e. clos(π ∞ ) ∩ D = D. This result was improved to a larger set in [10]. Our new result here implies that σ ∞ is dense in this particular set as well.…”
Section: Introductionmentioning
confidence: 50%
“…Thus the assertion follows. Alternatively one could also apply Laplace's formula twice to get the same result (see [10] for details). 2…”
Section: Three Lemmas and A Theoremmentioning
confidence: 99%
See 1 more Smart Citation
“…We here use a random-sign model, also known as the Feinberg-Zee (FZ) random-hopping model [27,39,[56][57][58][59][60][61][62][63], defined by the Hamiltonian…”
Section: Demonstrationmentioning
confidence: 99%
“…(1.7) (Here p −2 (S) := p −1 (p −1 (S)), p −3 (S) := p −1 (p −2 (S)), etc.) Hagger [17] observes that, as a consequence of (1.5) and (1.6), U (p) ⊂ Σ π . He also notes that standard results of complex dynamics (e.g., [11,Corollary 14.8]) imply that J(p) ⊂ U (p), so that J(p) ⊂ Σ π ; here J(p) denotes the Julia set of the polynomial p. (Where p 2 (λ) := p(p(λ)), p 3 (λ) := p(p 2 (λ)), etc., we recall [11] that the filled Julia set K(p) of a polynomial p of degree ≥ 2 is the compact set of those λ ∈ C for which the sequence (p n (λ)) n∈N , the orbit of λ, is bounded.…”
Section: Introductionmentioning
confidence: 99%