1992
DOI: 10.1063/1.529991
|View full text |Cite
|
Sign up to set email alerts
|

Exact solutions of SL(N,R)-invariant chiral equations one- and two-dimensional subspaces

Abstract: A methodology for integrating the chiral equation (pg,&-I),,-+ (pg,g-') ,= = 0 is developed, when g is a matrix of the SL(N,R) groug. In this work the ansatze g=g(A) where A satisfy the Laplace equation and g=g(&r) are made, where A and T are geodesic parameters of an arbitrary Riemannian space. This reduces the chiral equation to an algebraic problem and g can be obtained by integrating a homogeneous linear system of differential equations. As an example of the first ansatz, all the matrices for N=3 and one e… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
8
0

Year Published

1993
1993
2023
2023

Publication Types

Select...
6

Relationship

1
5

Authors

Journals

citations
Cited by 10 publications
(8 citation statements)
references
References 5 publications
0
8
0
Order By: Relevance
“…This is possible because the corresponding potential space, defined bellow, is a symmetric Riemannian space only for α = 0 and α = √ 3, but this is not the case for the low energy limit in super strings or the Maxwell-phantom theories. In [12] we extended this method [31][32][33][34][35][36][37][38][39][40][41][42][43][44][45] to the Einstein-Maxwell-Dilaton fields with arbitrary α and in this work I have extended this techniques for the Einstein-Maxwell-Phantom fields. In this work I have given a method from which we can derive a set of formulas that can be integrated in order to find exact solutions of the Einstein-Maxell phantom fields.…”
Section: Discussionmentioning
confidence: 99%
“…This is possible because the corresponding potential space, defined bellow, is a symmetric Riemannian space only for α = 0 and α = √ 3, but this is not the case for the low energy limit in super strings or the Maxwell-phantom theories. In [12] we extended this method [31][32][33][34][35][36][37][38][39][40][41][42][43][44][45] to the Einstein-Maxwell-Dilaton fields with arbitrary α and in this work I have extended this techniques for the Einstein-Maxwell-Phantom fields. In this work I have given a method from which we can derive a set of formulas that can be integrated in order to find exact solutions of the Einstein-Maxell phantom fields.…”
Section: Discussionmentioning
confidence: 99%
“…the KK theory obtains a chiral form. This form allowed to obtain wide classes of the three-dimensional solutions defined by a set of harmonic functions (see [17]), etc. Moreover, in two dimensions the inverse scattering transform technique leads to construction of the 2N-soliton solution (see [18] for the d = 1 and d = 2 cases).…”
Section: Generation Techniquementioning
confidence: 99%
“…A general integration algorithm that applies even to the Lie algebra sl(N, R), is given in [8]. An explicitly solvable example for SL(4, R) can be found in [91.…”
Section: (~6)mentioning
confidence: 99%