2003
DOI: 10.1117/12.485953
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Quantum lattice gas representation for vector solitons

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Cited by 4 publications
(10 citation statements)
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“…Turbulent soliton interactions are also considered using a potential of the form V2A[JQi 2 + 1Q21 2 ] in the evolution of the Q 2 -mode, while the Qi-mode satisfies the standard cubic NLS potential. We have presented some preliminary results on the elastic Manakov soliton collisions at a SPIE conference (Vahala et al 2003a). Here, we concentrate on those soliton parameters that permit inelastic Manakov soliton collisions, and consider the effect of the cross-phase modulation coefficient and turbulence on the soliton/solitary waves.…”
Section: Ta2119/3mentioning
confidence: 99%
See 1 more Smart Citation
“…Turbulent soliton interactions are also considered using a potential of the form V2A[JQi 2 + 1Q21 2 ] in the evolution of the Q 2 -mode, while the Qi-mode satisfies the standard cubic NLS potential. We have presented some preliminary results on the elastic Manakov soliton collisions at a SPIE conference (Vahala et al 2003a). Here, we concentrate on those soliton parameters that permit inelastic Manakov soliton collisions, and consider the effect of the cross-phase modulation coefficient and turbulence on the soliton/solitary waves.…”
Section: Ta2119/3mentioning
confidence: 99%
“…Here we generalize our QLG algorithm for the scalar NLS equation (Vahala et al 2003a) to the coupled vector NLS system for arbitrary coupling potentials V1, and V2,…”
Section: Quantum Lattice Gas Representation For Coupled-nlsmentioning
confidence: 99%
“…The appropriate collide-stream sequence of unitary operators needed to recover the dispersive part of NLS is dictated by the fact thatC 4…”
Section: Quantum Lattice Representation For Nlsmentioning
confidence: 99%
“…These ID equations are derived from the full MHD equations when the fluid density length scales are much longer than those of the B field. '17"1 8 To leading order, this results in a constant density so that (1) forms a closed set of equations for v and B. Adding a y-component of the magnetic field gives a 1D model for solar flares.1 9 In Elsasser variables z± = v ± B, (1) can be written in symmetric form…”
Section: Introductionmentioning
confidence: 99%
“…We address actual quantum control and Von Neuman projective shot noise in our papers on experimental parallel quantum computing with NMR. After some algebra for the special case where f3 = • and 0 =2, and with the encoding formulae (4) and the mesoscopic transport equation (1) and the asignment formula(7), and then also with the encoding formulae (8) and the quantum Boltzmann equation (1) and the asignment formulae (1), it follows that the dynamics of the v(x) and B(x) fields can be written directly as a finite difference equation:…”
mentioning
confidence: 99%