Abstract:We consider the Riemann-Hilbert factorization approach to solving the field equations of dimensionally reduced gravity theories. First we prove that functions belonging to a certain class possess a canonical factorization due to properties of the underlying spectral curve. Then we use this result, together with appropriate matricial decompositions, to study the canonical factorization of non-meromorphic monodromy matrices that describe deformations of seed monodromy matrices associated with known solutions. Th… Show more
“…As a result one finds, in particular, that from rational n × n monodromy matrices M, whose canonical Wiener-Hopf factorization can be constructed explicitly and in a computationally simple manner, one obtains explicit exact solutions that would be very difficult to obtain through other approaches. This is the case of the novel solutions presented in [6], whose construction, based on the Riemann-Hilbert approach of [5], is hereby rigorously justified. Using our improved understanding of the role of the factorization contour, we return to one of the new solutions obtained in [6], which was restricted to a certain domain in space-time.…”
Section: Jhep05(2020)124 Introductionmentioning
confidence: 99%
“…This is the case of the novel solutions presented in [6], whose construction, based on the Riemann-Hilbert approach of [5], is hereby rigorously justified. Using our improved understanding of the role of the factorization contour, we return to one of the new solutions obtained in [6], which was restricted to a certain domain in space-time. Here we complete its analysis, discuss its meaning and properties, and we also consider other ranges of parameters.…”
Section: Jhep05(2020)124 Introductionmentioning
confidence: 99%
“…By restricting to the subspace of solutions that only depend on two of the D spacetime coordinates, various approaches to solving the field equations become available (see for instance [1] for a recent survey thereof). In this paper, we focus on the Riemann-Hilbert approach, which can be applied to gravitational theories that satisfy certain requirements, see for instance [2][3][4][5][6] and references therein. This approach is remarkable in that it allows us to obtain explicit solutions to the reduced field equations through the appropriate factorization of a matrix function which depends on a complex variable τ that does not appear in the original problem.…”
We consider the Riemann-Hilbert factorization approach to the construction of Weyl metrics in four space-time dimensions. We present, for the first time, a rigorous proof of the remarkable fact that the canonical Wiener-Hopf factorization of a matrix obtained from a general (possibly unbounded) monodromy matrix, with respect to an appropriately chosen contour, yields a solution to the non-linear gravitational field equations. This holds regardless of whether the dimensionally reduced metric in two dimensions has Minkowski or Euclidean signature. We show moreover that, by taking advantage of a certain degree of freedom in the choice of the contour, the same monodromy matrix generally yields various distinct solutions to the field equations. Our proof, which fills various gaps in the existing literature, is based on the solution of a second Riemann-Hilbert problem and highlights the deep role of the spectral curve, the normalization condition in the factorization and the choice of the contour. This approach allows us to construct explicit solutions, including new ones, to the non-linear gravitational field equations, using simple complex analytic results.
“…As a result one finds, in particular, that from rational n × n monodromy matrices M, whose canonical Wiener-Hopf factorization can be constructed explicitly and in a computationally simple manner, one obtains explicit exact solutions that would be very difficult to obtain through other approaches. This is the case of the novel solutions presented in [6], whose construction, based on the Riemann-Hilbert approach of [5], is hereby rigorously justified. Using our improved understanding of the role of the factorization contour, we return to one of the new solutions obtained in [6], which was restricted to a certain domain in space-time.…”
Section: Jhep05(2020)124 Introductionmentioning
confidence: 99%
“…This is the case of the novel solutions presented in [6], whose construction, based on the Riemann-Hilbert approach of [5], is hereby rigorously justified. Using our improved understanding of the role of the factorization contour, we return to one of the new solutions obtained in [6], which was restricted to a certain domain in space-time. Here we complete its analysis, discuss its meaning and properties, and we also consider other ranges of parameters.…”
Section: Jhep05(2020)124 Introductionmentioning
confidence: 99%
“…By restricting to the subspace of solutions that only depend on two of the D spacetime coordinates, various approaches to solving the field equations become available (see for instance [1] for a recent survey thereof). In this paper, we focus on the Riemann-Hilbert approach, which can be applied to gravitational theories that satisfy certain requirements, see for instance [2][3][4][5][6] and references therein. This approach is remarkable in that it allows us to obtain explicit solutions to the reduced field equations through the appropriate factorization of a matrix function which depends on a complex variable τ that does not appear in the original problem.…”
We consider the Riemann-Hilbert factorization approach to the construction of Weyl metrics in four space-time dimensions. We present, for the first time, a rigorous proof of the remarkable fact that the canonical Wiener-Hopf factorization of a matrix obtained from a general (possibly unbounded) monodromy matrix, with respect to an appropriately chosen contour, yields a solution to the non-linear gravitational field equations. This holds regardless of whether the dimensionally reduced metric in two dimensions has Minkowski or Euclidean signature. We show moreover that, by taking advantage of a certain degree of freedom in the choice of the contour, the same monodromy matrix generally yields various distinct solutions to the field equations. Our proof, which fills various gaps in the existing literature, is based on the solution of a second Riemann-Hilbert problem and highlights the deep role of the spectral curve, the normalization condition in the factorization and the choice of the contour. This approach allows us to construct explicit solutions, including new ones, to the non-linear gravitational field equations, using simple complex analytic results.
“…We expect the techniques of [13,14] to be applicable for their explicit factorisation. It will also be interesting to relate monodromy matrices to rod-structure [41] in some precise way.…”
Section: Many Supertubes In Taub-nut and The Related Bubbling Geometriesmentioning
confidence: 99%
“…In the first approach [9][10][11][12], the authors have focused on monodromy matrices with simple poles with suitable rank residues. In the second approach [13,14], the authors have converted the matrix valued factorisation problem into a vectorial RiemannHilbert problem and solved it using complex analysis. Several examples have been worked out in both these approaches.…”
The Riemann-Hilbert approach to studying solutions of supergravity theories allows us to associate spacetime independent monodromy matrices (matrices in the Geroch group) with solutions that effectively only depend on two spacetime coordinates. This offers insights into symmetries of supergravity theories, and in the classification of their solutions. In this paper, we initiate a systematic study of monodromy matrices for multicenter solutions of five-dimensional U(1) 3 supergravity. We obtain monodromy matrices for a class of collinear Bena-Warner bubbling geometries. We show that for this class of solutions, monodromy matrices in the vector representation of SO(4,4) have only simple poles with residues of rank two and nilpotency degree two. These properties strongly suggest that an inverse scattering construction along the lines of [arXiv:1311.7018 [hepth]] can be given for this class of solutions, though it is not attempted in this work. Along the way, we clarify a technical point in the existing literature: we show that the so-called "spectral flow transformations" of Bena, Bobev, and Warner are precisely a class of Harrison transformations when restricted to the situation of two commuting Killing symmetries in five-dimensions.
The Riemann-Hilbert approach, in conjunction with the canonical Wiener-Hopf factorisation of certain matrix functions called monodromy matrices, enables one to obtain explicit solutions to the non-linear field equations of some gravitational theories. These solutions are encoded in the elements of a matrix M depending on the Weyl coordinates ρ and v, determined by that factorisation. We address here, for the first time, the underlying question of what happens when a canonical Wiener-Hopf factorisation does not exist, using the close connection of Wiener-Hopf factorisation with Toeplitz operators to study this question. For the case of rational monodromy matrices, we prove that the non-existence of a canonical Wiener-Hopf factorisation determines curves in the (ρ, v) plane on which some elements of M(ρ, v) tend to infinity, but where the space-time metric may still be well behaved. In the case of uncharged rotating black holes in four space-time dimensions and, for certain choices of coordinates, in five space-time dimensions, we show that these curves correspond to their ergosurfaces.
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