Non-Markovian dynamics in a spin star system: Exact solution and approximation techniques

Heinz-Peter Breuer, Daniel Burgarth, and Francesco Petruccione
Phys. Rev. B 70, 045323 – Published 30 July 2004

Abstract

The reduced dynamics of a central spin coupled to a bath of N spin-12 particles arranged in a spin star configuration is investigated. The exact time evolution of the reduced density operator is derived, and an analytical solution is obtained in the limit N of an infinite number of bath spins, where the model shows complete relaxation and partial decoherence. It is demonstrated that the dynamics of the central spin cannot be treated within the Born-Markov approximation. The Nakajima-Zwanzig and the time-convolutionless projection operator technique are applied to the spin star system. The performance of the corresponding perturbation expansions of the non-Markovian equations of motion is examined through a comparison with the exact solution.

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  • Received 9 January 2004

DOI:https://doi.org/10.1103/PhysRevB.70.045323

©2004 American Physical Society

Authors & Affiliations

Heinz-Peter Breuer1, Daniel Burgarth1, and Francesco Petruccione1,2

  • 1Physikalisches Institut, Universität Freiburg, Hermann-Herder-Str. 3, D-79104 Freiburg, Germany
  • 2School of Pure and Applied Physics, University of KwaZulu-Natal, 4041 Durban, South Africa

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Issue

Vol. 70, Iss. 4 — 15 July 2004

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