Holographic Fisher information metric in Schrödinger spacetime
In this paper, we study the Fisher information metric on the space of the coupling constants on both sides of the duality between non-relativistic dipole field theories and string theory in Schrödinger spacetime. We consider the following setup. In the gauge theory side one can deform a given confor...
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Veröffentlicht in: | European physical journal plus 2021-11, Vol.136 (11), p.1128, Article 1128 |
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Sprache: | eng |
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Zusammenfassung: | In this paper, we study the Fisher information metric on the space of the coupling constants on both sides of the duality between non-relativistic dipole field theories and string theory in Schrödinger spacetime. We consider the following setup. In the gauge theory side one can deform a given conformal field theory by a proper scalar operator and compute the quantum information metric via the two-point correlation function between two such operators. On the string side the deformation corresponds to a scalar field probing the background. In the large
N
limit of the theory the probing can be done without backreaction on the original spacetime, thus one can construct a perturbative scheme for the calculation of the dual holographic Fisher information metric as shown by [
1
]. Considering the asymptotic behaviour of the holographic Fisher information metric close to the boundary of the Schrödinger spacetime we show that its divergence structure exactly matches its dual quantum counterpart up to the leading order, thus extending the holographic setup up to the non-relativistic case. One should note that the existence of other terms is not seen from the boundary theory to this level of approximation. Their behaviour near the boundary, however, is pointing what kind of information from the boundary theory is missing to be able to reconstruct the bulk. Obviously, more work is needed to refine and elucidate their meaning and interrelations in holographic setup. |
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ISSN: | 2190-5444 2190-5444 |
DOI: | 10.1140/epjp/s13360-021-02109-0 |