2006
DOI: 10.1088/0305-4470/39/11/015
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Superstring theory on pp waves with ADE geometries

Abstract: We study the BMN correspondence between certain Penrose limits of type IIB superstrings on pp-wave orbifolds with ADE geometries, and the set of four-dimensional N = 2 superconformal field theories constructed as quiver gauge models classified by finite ADE Lie algebras and affine ADE Kac-Moody algebras. These models have 16 preserved supercharges and are based on systems of D3-branes and wrapped D5-and D7-branes. We derive explicitly the metrics of these pp-wave orbifolds and show that the BMN extension requi… Show more

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Cited by 6 publications
(8 citation statements)
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“…If u = f (x) is a function, then the manifold HΓ f can be expressed in terms of the invariants (8). So, we have:…”
Section: Partially Invariant Solutions Methodsmentioning
confidence: 99%
See 1 more Smart Citation
“…If u = f (x) is a function, then the manifold HΓ f can be expressed in terms of the invariants (8). So, we have:…”
Section: Partially Invariant Solutions Methodsmentioning
confidence: 99%
“…A Walker manifold is called Einstein Walker manifold if its Ricci tensor is a scaler multiple of the metric at each point. Four-dimensional Einstein Walker manifolds form the underling structure of many geometric and physical models such as; hh-space in general relativity, pp-wave model and other areas [6][7][8][9][10][11][12].…”
Section: Introductionmentioning
confidence: 99%
“…According to modern physics, we do not live in a Riemannian universe, but rather in a Lorentzian universe or even in the higher signature setting according to some string theories. Indefinite signatures also appears in supergravity theory (see, for example, Abounasr, Belhaj, Rasmussen, and Saidi [2]). Walker metrics have indefinite signatures and are important as well (see, for example, the discussion in Davidov, Diaz-Ramos, Garcia-Rio, Matsushita, Muskarov, and Vazquez-Lorenzo [7]).…”
Section: Higher Signature Geometrymentioning
confidence: 99%
“…Lorentzian Walker manifolds have been studied extensively in physics since they constitute the background metric of the pp-wave models. A pp-wave spacetime admits a covariantly constant null vector field U [1].…”
Section: Introductionmentioning
confidence: 99%