2003
DOI: 10.1016/s0370-2693(02)03189-1
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Effective matter superpotentials from Wishart random matrices

Abstract: We show how within the Dijkgraaf-Vafa prescription one can derive superpotentials for matter fields. The ingredients forming the non-perturbative Affleck-Dine-Seiberg superpotentials arise from constrained matrix integrals, which are equivalent to classical complex Wishart random matrices. The mechanism is similar to the way the Veneziano-Yankielowicz superpotential arises from the matrix model measure.Comment: 9 pages; v2: published versio

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Cited by 52 publications
(73 citation statements)
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“…Thus, its contribution to the superpotential is its derivative multiplied by the rank of the gauge group (the unbroken as well as the broken part!). The equation (58) recovers the suggestion [24] for the inclusion of massless quarks in the matrix model, and is also equivalent [39] with the suggestion of [30] that one first deforms the matrix model by mass terms and then takes the massless limit. This can be easily seen by using an integral representation for the δ-function in equation (58) and noticing that the new variable plays the role of mass parameter for the quarks Q M andQ M .…”
Section: Massive and Massless Matrix Modelssupporting
confidence: 60%
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“…Thus, its contribution to the superpotential is its derivative multiplied by the rank of the gauge group (the unbroken as well as the broken part!). The equation (58) recovers the suggestion [24] for the inclusion of massless quarks in the matrix model, and is also equivalent [39] with the suggestion of [30] that one first deforms the matrix model by mass terms and then takes the massless limit. This can be easily seen by using an integral representation for the δ-function in equation (58) and noticing that the new variable plays the role of mass parameter for the quarks Q M andQ M .…”
Section: Massive and Massless Matrix Modelssupporting
confidence: 60%
“…While the inclusion of massive quarks in this framework was easily achieved without reference to geometry, certain difficulties were encountered in dealing with massless ones. The two solutions to this problem, proposed in [24] and [30] on a field-theoretic basis only, were shown to be equivalent in [39]. From our analysis we see that this identification appears naturally from the geometrical picture and its relation to brane configurations.…”
Section: Discussionmentioning
confidence: 51%
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