1992
DOI: 10.1016/0550-3213(92)90067-l
|View full text |Cite
|
Sign up to set email alerts
|

symmetry of quantum W∞ gravity

Abstract: Two-dimensional gravity in the light-cone gauge was shown by Polyakov to exhibit an underlying SL(2, R) Kac-Moody symmetry, which may be used to express the energy-momentum tensor for the metric component h ++ in terms of the SL(2, R) currents via the Sugawara construction. We review some recent results which show that in a similar manner, W ∞ and W 1+∞ gravities have underlying SL(∞, R) and GL(∞, R) Kac-Moody symmetries respectively.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
21
0

Year Published

1992
1992
2024
2024

Publication Types

Select...
6

Relationship

1
5

Authors

Journals

citations
Cited by 10 publications
(21 citation statements)
references
References 24 publications
0
21
0
Order By: Relevance
“…The quantization procedure deforms the classical algebra w to the quantum algebra W due to the presence of anomalies -deformations of Moyal type of Poisson and symplecticdiffeomorphism algebras caused essentially by normal order ambiguities (see bellow). Also, generalizing the SL(2, R) Kac-Moody hidden symmetry of Polyakov's induced gravity, there are SL(∞, R) and GL(∞, R) Kac-Moody hidden symmetries for W ∞ and W 1+∞ gravities, respectively [33]. Moreover, as already mentioned, the symmetry W 1+∞ appears to be useful in the classification of universality classes in the fractional quantum Hall effect.…”
Section: Tensor Operator Algebras Of Su(2) and Large-n Matrix Modelsmentioning
confidence: 87%
“…The quantization procedure deforms the classical algebra w to the quantum algebra W due to the presence of anomalies -deformations of Moyal type of Poisson and symplecticdiffeomorphism algebras caused essentially by normal order ambiguities (see bellow). Also, generalizing the SL(2, R) Kac-Moody hidden symmetry of Polyakov's induced gravity, there are SL(∞, R) and GL(∞, R) Kac-Moody hidden symmetries for W ∞ and W 1+∞ gravities, respectively [33]. Moreover, as already mentioned, the symmetry W 1+∞ appears to be useful in the classification of universality classes in the fractional quantum Hall effect.…”
Section: Tensor Operator Algebras Of Su(2) and Large-n Matrix Modelsmentioning
confidence: 87%
“…A Killing symmetry reduction of 4D SD Gravity furnishes the 3D continuous SL(∞, R) Toda theory [1] which exhibits a w ∞ symmetry (a Killing symmetry reduction of a CP 1 loop algebra over w ∞ ). Conversely, the induced 2D quantum W ∞ gravity action in the light-cone gauge has a hidden SL(∞, R) Kac-Moody symmetry [27]. The classical geometry of 2D w ∞ gravity is linked to the 4D Self-Dual gravity associated with the 4D cotangent space of 2D Riemann surfaces [38] and admits a Fedosov deformation quantization.…”
Section: Non-critical W ∞ (Super) Strings and The Critical (Super) Mementioning
confidence: 99%
“…One should notice that one is adding the weights as vectors in a Hilbert space and not the values of λ, λ * . Going back to eq-(6.24), the n th mode component associated with the function f (t) = a n cos(nt) leads tô 27) and similarly for the other generatorŝ…”
Section: Correspondence Between Highest Weight Representations and Thmentioning
confidence: 99%
“…The second approach is to extract the anomalous quantum dynamics directly from the the anomalous Ward identities of the worldsheet symmetries. In this latter approach, non-trivial correlation functions arise at the quantum level, revealing in some cases hidden quantum symmetries such as the SL(2, IR) symmetry found by Polyakov for the bosonic string [4], or the SL(∞, IR) symmetry found in worldsheet W ∞ gravity [5,6] (which becomes a GL(∞, IR) symmetry for W 1+∞ gravity [6].) Because it reveals hidden symmetries, the approach of extracting dynamics from anomalous Ward identities is clearly of great importance for the non-critical theories.…”
Section: Introductionmentioning
confidence: 99%
“…Attempts in [7] to extend the approach of [4][5][6] to the W N gravity case ran into the difficulty that a consistent set of conditions to impose on the background gauge fields to eliminate the anomalies could not be derived owing to their off-diagonal structure. These difficulties are presumably related to our imperfect understanding of W 3 geometry.…”
Section: Introductionmentioning
confidence: 99%