2015
DOI: 10.1063/1.4922887
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A new class of ensemble conserving algorithms for approximate quantum dynamics: Theoretical formulation and model problems

Abstract: We develop two classes of quasi-classical dynamics that are shown to conserve the initial quantum ensemble when used in combination with the Feynman-Kleinert approximation of the density operator. These dynamics are used to improve the Feynman-Kleinert implementation of the classical Wigner approximation for the evaluation of quantum time correlation functions known as Feynman-Kleinert linearized path-integral. As shown, both classes of dynamics are able to recover the exact classical and high temperature limi… Show more

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Cited by 27 publications
(28 citation statements)
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References 26 publications
(66 reference statements)
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“…As a result of Eq. (33), the entire quantum Boltzmann distribution is conserved, provided the dynamics of Q 0,t is generated by a quantum-Boltzmann-conserving method such as (T)RPMD or CMD (as in the planetary model 18 ). From this it follows that the planetary model gives the same result as CMD (within the FK approximation) for linear Kubo TCFs.…”
Section: The Planetary Modelmentioning
confidence: 99%
See 1 more Smart Citation
“…As a result of Eq. (33), the entire quantum Boltzmann distribution is conserved, provided the dynamics of Q 0,t is generated by a quantum-Boltzmann-conserving method such as (T)RPMD or CMD (as in the planetary model 18 ). From this it follows that the planetary model gives the same result as CMD (within the FK approximation) for linear Kubo TCFs.…”
Section: The Planetary Modelmentioning
confidence: 99%
“…4 In this article, we examine the relation to Matsubara dynamics of another heuristically-obtained method-the Feynman-Kleinert (FK) quasi-classical Wigner method, or 'planetary model'. 18,19 This model is exact in the harmonic limit, not just for the dynamics of the centroid (as is true also for (T)RPMD and CMD), but also for the dynamics of fluctuations about the centroid. The planetary model describes these fluctuations by means of a single particle ('the planet') which follows locally harmonic motion, with a centroid-dependent frequency (see Fig.…”
Section: Introductionmentioning
confidence: 98%
“…30 Furthermore, the linearized SC-IVR (LSC-IVR) approach, 31 obtained as the linearized approximation of the SC-IVR, 32 has been used for simulations of infrared spectroscopy, 33,34 although the method neglects interference effects and does not in general preserve quantum statistics. Methods based on the path-integral formalism that preserve the quantum Boltzmann distribution, such as Centroid Molecular Dynamics (CMD), 35,36 Ring Polymer Molecular Dynamics (RPMD), 37 or the planetary model, 38 provide a balance between accuracy and computational overhead. 23,27,28,[39][40][41] Very recently, it has been shown that these methods are approximations of the general Boltzmann conserving Matsubara dynamics.…”
Section: Introductionmentioning
confidence: 99%
“…These range from the simple replacement of the quantum Boltzmann operator with its classical counterpart, an approximation that is only appropriate at sufficiently high temperatures where the zero-point energy is negligible, to sophisticated path integral-based techniques. [42][43][44][45][46][47][48][49][50][51][52][53][54][55][56][57] These approaches have proven useful in the investigation of, for instance, vibrational spectra and relaxation rates, 43,[58][59][60] proton transfer problems, 56 and quantum diffusion in parahydrogen 61 and liquid neon. 49 The benefits of these approximations notwithstanding, the general accuracy of approximate Wigner transformed density operators in complex systems has been difficult to assess, especially when used in conjunction with dynamical calculations.…”
Section: Introductionmentioning
confidence: 99%