2020
DOI: 10.48550/arxiv.2003.10475
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Exact equivalences and phase discrepancies between random matrix ensembles

Leonardo Santilli,
Miguel Tierz

Abstract: We study two types of random matrix ensembles that emerge when considering the same probability measure on partitions. One is the Meixner ensemble with a hard wall and the other are two families of unitary matrix models, with weight functions that can be interpreted as characteristic polynomial insertions. We show that the models, while having the same exact evaluation for fixed values of the parameter, may present a different phase structure. We find phase transitions of the second and third order, depending … Show more

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Cited by 4 publications
(7 citation statements)
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“…The particular case with A = N was recently studied in section 3 of [30], where it originated from a family of unitary matrix models through the map to the unit circle. This case is special, as we shall discuss, and in the large N theory corresponds to the marginal case for stability of the model.…”
Section: The 3-parameter Deformed Cauchy Modelmentioning
confidence: 99%
See 2 more Smart Citations
“…The particular case with A = N was recently studied in section 3 of [30], where it originated from a family of unitary matrix models through the map to the unit circle. This case is special, as we shall discuss, and in the large N theory corresponds to the marginal case for stability of the model.…”
Section: The 3-parameter Deformed Cauchy Modelmentioning
confidence: 99%
“…This case is special, as we shall discuss, and in the large N theory corresponds to the marginal case for stability of the model. When = 0, the potential (3) describes a Cauchy ensemble, studied in [31,30].…”
Section: The 3-parameter Deformed Cauchy Modelmentioning
confidence: 99%
See 1 more Smart Citation
“…An interesting question is if all phases appearing in the whole (λ, τ ) parameter space have a counterpart in the Hermitian model of [11]. The correspondence in the phase structure of unitary and Hermitian matrix models in the large N limit involves subtle issues that have been recently discussed in [23]. In the present model, the main difference will occur in the τ < 0 region.…”
Section: Discussionmentioning
confidence: 87%
“…The term with coefficient A corresponds to the logarithmic term in (1) (taking into account a shift due to the Jacobian of the sterographic map), while the term with coefficient B gives rise to the GWW term. The model generalizes the Hermitian model appeared in [8], derived from the ν = 0 case (see [9,10] for earlier studies on related models). The logarithmic term appears in the mathematical literature in the study of Cauchy random matrix ensembles [11].…”
Section: Introductionmentioning
confidence: 81%