Theory of coupled parametric oscillators beyond coupled Ising spins

Marcello Calvanese Strinati, Leon Bello, Avi Pe'Er, Emanuele G. Dalla Torre

Research output: Contribution to journalArticlepeer-review

30 Scopus citations

Abstract

Periodically driven parametric oscillators offer a convenient way to simulate classical Ising spins. When many parametric oscillators are coupled dissipatively, they can be analogous to networks of Ising spins, forming an effective coherent Ising machine (CIM) that efficiently solves computationally hard optimization problems. In the companion paper, we studied experimentally the minimal realization of a CIM, i.e. two coupled parametric oscillators [L. Bello, M. Calvanese Strinati, E. G. Dalla Torre, and A. Pe'er, Phys. Rev. Lett. 123, 083901 (2019)10.1103/PhysRevLett.123.083901]. We found that the presence of an energy-conserving coupling between the oscillators can dramatically change the dynamics, leading to everlasting beats which transcend the Ising description. Here, we analyze this effect theoretically by solving numerically and, when possible, analytically the equations of motion of two parametric oscillators. Our main tools include (i) a Floquet analysis of the linear equations, (ii) a multiscale analysis based on a separation of timescales between the parametric oscillations and the beats, and (iii) the numerical identification of limit cycles and attractors. Using these tools, we fully determine the phase boundaries and critical exponents of the model, as a function of the intensity and the phase of the coupling and of the pump. Our study highlights the universal character of the phase diagram and its independence on the specific type of nonlinearity present in the system. Furthermore, we identify phases of the model with more than two attractors, possibly describing a larger spin algebra.

Original languageEnglish
Article number023835
JournalPhysical Review A
Volume100
Issue number2
DOIs
StatePublished - 22 Aug 2019

Bibliographical note

Publisher Copyright:
© 2019 American Physical Society. ©2019 American Physical Society.

Funding

We thank Joseph Avron, Ivan Bonamassa, Claudio Conti, Nir Davidson, Igor Gershenzon, Ron Lifshitz, Chene Tradonsky, and Yoshihisa Yamamoto for fruitful discussions. We are grateful to David A. Kessler for careful reading and invaluable comments on this paper. A.P. acknowledges support from ISF Grant No. 46/14. M.C.S. acknowledges support from the ISF Grants No. 231/14 and No. 1452/14.

FundersFunder number
Israel Science Foundation231/14, 46/14, 1452/14

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