Relationship between the transverse-field Ising model and the XY model via the rotating-wave approximation

Thomas G. Kiely and J. K. Freericks
Phys. Rev. A 97, 023611 – Published 6 February 2018

Abstract

In a large transverse field, there is an energy cost associated with flipping spins along the axis of the field. This penalty can be employed to relate the transverse-field Ising model in a large field to the XY model in no field (when measurements are performed at the proper stroboscopic times). We describe the details for how this relationship works and, in particular, we also show under what circumstances it fails. We examine wave-function overlap between the two models and observables, such as spin-spin Green's functions. In general, the mapping is quite robust at short times, but will ultimately fail if the run time becomes too long. There is also a tradeoff between the length of time one can run a simulation out to and the time jitter of the stroboscopic measurements that must be balanced when planning to employ this mapping.

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  • Received 12 November 2017

DOI:https://doi.org/10.1103/PhysRevA.97.023611

©2018 American Physical Society

Physics Subject Headings (PhySH)

Atomic, Molecular & OpticalQuantum Information, Science & Technology

Authors & Affiliations

Thomas G. Kiely and J. K. Freericks

  • Department of Physics, Georgetown University, 37th and O Streets NW, Washington, DC 20057, USA

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Issue

Vol. 97, Iss. 2 — February 2018

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