1990
DOI: 10.1103/physrevlett.64.260
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Spacetime singularities in string theory

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Cited by 374 publications
(553 citation statements)
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“…It has been argued [29] that this leads to singular string propagation and therefore, naively, one might think that these solutions are unphysical. However, we believe that this is not the case.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…It has been argued [29] that this leads to singular string propagation and therefore, naively, one might think that these solutions are unphysical. However, we believe that this is not the case.…”
Section: Discussionmentioning
confidence: 99%
“…If the metric is of the form (1) the fluctuations of the eight transverse modes are governed by Schrödinger equations (see, for instance, [29])…”
Section: The Perturbative String Spectrummentioning
confidence: 99%
“…are solutions to all orders in α ′ for the bosonic/fermionic string in D = 26/10 provided A ij satisfies the condition [4] 4 m 2 (n − k) = A ij A ij .…”
Section: The Background As the Penrose Limit Of Ds N × S Nmentioning
confidence: 99%
“…This observation led in the sixties and seventies to a detailed study of the geometric properties of planewave metrics and of matter fields defined on them [2]. Already within string theory, it soon became clear that higher-dimensional plane waves give exact solutions to string theory, provided the Kalb-Ramond and dilaton fields satisfy certain conditions [3] [4]. The generalization of the Penrose limiting procedure relating higher dimensional plane waves with more complicated solutions to string theory [5] further triggered the interest in such space-times.…”
Section: Introductionmentioning
confidence: 99%
“…As we will see, now the lack of global hyperbolicity can be well understood, but Ehlers-Kundt conjecture still remains open. The applications to string theory have highlights as: (a) gravitational pp-waves are relevant spacetimes with vanishing scalar invariants (VSI, see [19,42] for a classification), and such spacetimes yield exact backgrounds for string theory (vanishing of α ′ corrections, [2,30]), (b) Berenstein, Maldacena and Nastase [5] have recently proposed and influential solvable model for string theory by taking the Penrose limit in AdS 5 × S 5 spacetimes, or (c) after realizing that Gödel like universes can be supersimetrically embedded in string theory, it was realized and emphasized that these solutions were T -dual to compactified plane wave backgrounds [13,28,35].…”
Section: Introductionmentioning
confidence: 99%