“…Note that κ 2,0 κ 0,2 = 1/4 is the minimal value which comes from the uncertainty principle (i.e., we assume a coherent state initially). Note also that κ 2,0 κ 0,2 −κ 2 1,1 is a constant [32,33]. In Fig.…”
Section: Modelmentioning
confidence: 79%
“…Since we know that p ≈ y − y 0 evolves linearly in time in the classical system, we illustrate evolutions of variables as functions of p. Note that κ 2,0 κ 0,2 = 1/4 is the minimal value which comes from the uncertainty principle (i.e., we assume a coherent state initially). Note also that κ 2,0 κ 0,2 −κ 2 1,1 is a constant [32,33]. In Fig.…”
Section: Modelmentioning
confidence: 79%
“…It is well-known that the Ehrenfest's theorem tells Recently, Shigeta et al [32,33] defined an expression for the expectation value by means of cumulants among the canonical pair of the variables q and p. That is defined as…”
Section: Modelmentioning
confidence: 99%
“…Then, the following simultaneous equations are derived from the Ehrenfest's theorem: [32,33] q =H (0,1) , (4.5) p = −H (1,0) , (4.6) κ 2,0 = 2κ 2,0H (1,1) + 2κ 1,1H (0,2) , (4.7)…”
Section: Modelmentioning
confidence: 99%
“…Then, the following simultaneous equations are derived from the Ehrenfest's theorem: [32,33] q = H(0,1) , (4.5)…”
We propose an approach to quantum cosmology of integrable models. To analyze the models with two dynamical variables, we introduce equivalent Hamiltonians in reduced phase spaces, which are obtained with the aid of the Faddeev-Jackiw method. Quantum dynamics of the models can be studied by using the equivalent Hamiltonians with various techniques.
“…Note that κ 2,0 κ 0,2 = 1/4 is the minimal value which comes from the uncertainty principle (i.e., we assume a coherent state initially). Note also that κ 2,0 κ 0,2 −κ 2 1,1 is a constant [32,33]. In Fig.…”
Section: Modelmentioning
confidence: 79%
“…Since we know that p ≈ y − y 0 evolves linearly in time in the classical system, we illustrate evolutions of variables as functions of p. Note that κ 2,0 κ 0,2 = 1/4 is the minimal value which comes from the uncertainty principle (i.e., we assume a coherent state initially). Note also that κ 2,0 κ 0,2 −κ 2 1,1 is a constant [32,33]. In Fig.…”
Section: Modelmentioning
confidence: 79%
“…It is well-known that the Ehrenfest's theorem tells Recently, Shigeta et al [32,33] defined an expression for the expectation value by means of cumulants among the canonical pair of the variables q and p. That is defined as…”
Section: Modelmentioning
confidence: 99%
“…Then, the following simultaneous equations are derived from the Ehrenfest's theorem: [32,33] q =H (0,1) , (4.5) p = −H (1,0) , (4.6) κ 2,0 = 2κ 2,0H (1,1) + 2κ 1,1H (0,2) , (4.7)…”
Section: Modelmentioning
confidence: 99%
“…Then, the following simultaneous equations are derived from the Ehrenfest's theorem: [32,33] q = H(0,1) , (4.5)…”
We propose an approach to quantum cosmology of integrable models. To analyze the models with two dynamical variables, we introduce equivalent Hamiltonians in reduced phase spaces, which are obtained with the aid of the Faddeev-Jackiw method. Quantum dynamics of the models can be studied by using the equivalent Hamiltonians with various techniques.
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