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Volumn 79, Issue 4, 2009, Pages

Early time kinetics of systems with spatial symmetry breaking

Author keywords

[No Author keywords available]

Indexed keywords

ANTIFERROMAGNETIC ISING MODELS; CAHN HILLIARD COOKS; DIFFERENT TIME SCALE; FOURIER MODES; GENERALIZED THEORIES; INTERACTION RANGES; LINEAR COMBINATIONS; LINEAR THEORIES; NUMERICAL SIMULATIONS; SPATIAL SYMMETRIES; SYMMETRY-BREAKING; TIME-SCALE; UNSTABLE REGIONS; UNSTABLE STATE;

EID: 65549086186     PISSN: 15393755     EISSN: 15502376     Source Type: Journal    
DOI: 10.1103/PhysRevE.79.041121     Document Type: Article
Times cited : (3)

References (38)
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    • In analogy to the ferromagnetic case we refer to dynamics as conserving or not conserving the "order parameter" even though φ is not a well-defined order parameter for the antiferromagnetic Ising model which we will consider.
    • In analogy to the ferromagnetic case we refer to dynamics as conserving or not conserving the "order parameter" even though φ is not a well-defined order parameter for the antiferromagnetic Ising model which we will consider.
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    • We note that Corberi 10.1103/PhysRevE.51.5469
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    • The ratio L/R gives the approximate number of stripes (or clumps along one dimension) in the system. We have tested many values of L/R and found that the early stage two kinetics is unaffected by this value. We did find that stage two lasts longer for larger values of L/R. At any value of L/R larger interaction ranges extend the lifetime of stage two. We do not deal with the creation of defects in systems with large L/R because the defects do not form until after stage two breaks down.
    • The ratio L/R gives the approximate number of stripes (or clumps along one dimension) in the system. We have tested many values of L/R and found that the early stage two kinetics is unaffected by this value. We did find that stage two lasts longer for larger values of L/R. At any value of L/R larger interaction ranges extend the lifetime of stage two. We do not deal with the creation of defects in systems with large L/R because the defects do not form until after stage two breaks down.
  • 38
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    • That the contribution from the noise term has the same time dependence as the noiseless term can be shown to be true in the case where B=const [from Eq. 2] but is complicated by further couplings for a spatially dependent B.
    • That the contribution from the noise term has the same time dependence as the noiseless term can be shown to be true in the case where B=const [from Eq. 2] but is complicated by further couplings for a spatially dependent B.


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