Curved Witten-Dijkgraaf-Verlinde-Verlinde equation and N=4 mechanics

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  • Yerevan State University
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Original languageEnglish
Article number101702
JournalPhysical Review D
Volume96
Issue number10
Publication statusPublished - 2017

Abstract

We propose a generalization of the Witten-Dijkgraaf-Verlinde-Verlinde (WDVV) equation from Rn to an arbitrary Riemannian manifold. Its form is obtained by extending the relation of the WDVV equation with N=4 supersymmetric n-dimensional mechanics from flat to curved space. The resulting "curved WDVV equation" is written in terms of a third-rank Codazzi tensor. For every flat-space WDVV solution subject to a simple constraint, we provide a curved-space solution on any isotropic space, in terms of the rotationally invariant conformal factor of the metric.

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Curved Witten-Dijkgraaf-Verlinde-Verlinde equation and N=4 mechanics. / Kozyrev, Nikolay; Krivonos, Sergey; Lechtenfeld, Olaf et al.
In: Physical Review D, Vol. 96, No. 10, 101702, 2017.

Research output: Contribution to journalArticleResearchpeer review

Kozyrev N, Krivonos S, Lechtenfeld O, Nersessian A, Sutulin A. Curved Witten-Dijkgraaf-Verlinde-Verlinde equation and N=4 mechanics. Physical Review D. 2017;96(10):101702. doi: 10.1103/PhysRevD.96.101702
Kozyrev, Nikolay ; Krivonos, Sergey ; Lechtenfeld, Olaf et al. / Curved Witten-Dijkgraaf-Verlinde-Verlinde equation and N=4 mechanics. In: Physical Review D. 2017 ; Vol. 96, No. 10.
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abstract = "We propose a generalization of the Witten-Dijkgraaf-Verlinde-Verlinde (WDVV) equation from Rn to an arbitrary Riemannian manifold. Its form is obtained by extending the relation of the WDVV equation with N=4 supersymmetric n-dimensional mechanics from flat to curved space. The resulting {"}curved WDVV equation{"} is written in terms of a third-rank Codazzi tensor. For every flat-space WDVV solution subject to a simple constraint, we provide a curved-space solution on any isotropic space, in terms of the rotationally invariant conformal factor of the metric.",
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note = "Funding Information: We are grateful to M. Feigin and A. Veselov for stimulating discussions. A. S. also thanks S. Kuzenko, A. Sagnotti, and D. Sorokin for valuable comments and discussions during the Ginzburg conference in Moscow. This work was partially supported by the Heisenberg-Landau program. The work of N. K. and S. K. was partially supported by RSCF Grant No. 14-11-00598, and that of A. S. was partially supported by RFBR Grant No. 15-02-06670. The work of A. N. was partially supported by the Armenian State Committee of Science Grant No. 15T-1C367. This article is based upon work from COST Action MP1405 QSPACE, supported by COST (European Cooperation in Science and Technology). Publisher Copyright: {\textcopyright} 2017 American Physical Society. Copyright: Copyright 2017 Elsevier B.V., All rights reserved.",
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AU - Krivonos, Sergey

AU - Lechtenfeld, Olaf

AU - Nersessian, Armen

AU - Sutulin, Anton

N1 - Funding Information: We are grateful to M. Feigin and A. Veselov for stimulating discussions. A. S. also thanks S. Kuzenko, A. Sagnotti, and D. Sorokin for valuable comments and discussions during the Ginzburg conference in Moscow. This work was partially supported by the Heisenberg-Landau program. The work of N. K. and S. K. was partially supported by RSCF Grant No. 14-11-00598, and that of A. S. was partially supported by RFBR Grant No. 15-02-06670. The work of A. N. was partially supported by the Armenian State Committee of Science Grant No. 15T-1C367. This article is based upon work from COST Action MP1405 QSPACE, supported by COST (European Cooperation in Science and Technology). Publisher Copyright: © 2017 American Physical Society. Copyright: Copyright 2017 Elsevier B.V., All rights reserved.

PY - 2017

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