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Classical analogous of quantum cosmological perfect fluid models
General Relativity and Quantum Cosmology · Submitted 28 Nov 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We show that such models are equivalent to a classical system where, besides the perfect fluid, a repulsive fluid with an equation of state $p_Q = \rho_Q$ is present.
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The abstract, sentence by sentence
Quantization in the mini-superspace of a gravity system coupled to a perfect fluid, leads to a solvable model which implies singularity free solutions through the construction of a superposition of the wavefunctions. We show that such models are equivalent to a classical system where, besides the perfect fluid, a repulsive fluid with an equation of state $p_Q = \rho_Q$ is present. This leads to speculate on the true nature of this quantization procedure. A perturbative analysis of the classical system reveals the condition for the stability of the classical system in terms of the existence of an anti-gravity phase.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Quantization in the mini-superspace of a gravity system coupled to a perfect fluid, leads to a solvable model which implies singularity free solutions through the construction of a superposition of the wavefunctions. | result 0.51 | 0.46 | 0.25 | asserted 1.00 |
| s1 | We show that such models are equivalent to a classical system where, besides the perfect fluid, a repulsive fluid with an equation of state $p_Q = \rho_Q$ is present. | result 0.92 | 0.89 | 0.68 | asserted 1.00 |
| s2 | This leads to speculate on the true nature of this quantization procedure. | interpretation 1.00 | 0.19 | 0.07 | speculative 0.94 |
| s3 | A perturbative analysis of the classical system reveals the condition for the stability of the classical system in terms of the existence of an anti-gravity phase. | result 0.78 | 0.87 | 0.16 | asserted 0.97 |
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The paper
Original abstract
Quantization in the mini-superspace of a gravity system coupled to a perfect fluid, leads to a solvable model which implies singularity free solutions through the construction of a superposition of the wavefunctions. We show that such models are equivalent to a classical system where, besides the perfect fluid, a repulsive fluid with an equation of state $p_Q = \rho_Q$ is present. This leads to speculate on the true nature of this quantization procedure. A perturbative analysis of the classical system reveals the condition for the stability of the classical system in terms of the existence of an anti-gravity phase.
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How the literature uses it
4 arXiv papers cite this in 5 sentences
Papers whose main result relates to this one's
States the same result 1 paper
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We show that such quantum cosmological perfect fluid models admit a universal classical analogue, represented by the addition, to the ordinary classical model, of a repulsive stiff matter fluid.
Quantum cosmological perfect fluid model and its classical analogue · 0.92
Papers citing it · 3 sentences without a confident label
Uses its method or tool 2 papers
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According to Schutz's representation for the perfect fluid [ref] , its Hamiltonian can be viewed as (see [ref] for details) [equation] where $T$ is a dynamical variable related to the thermodynamical parameters of the perfect fluid and $P_T$ is its conjugate momentum.
Classical and quantum Ho\v{r}ava-Lifshitz cosmology in a minisuperspace perspective · The model · 0.97
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According to Schutz's representation for the perfect fluid [ref] , its Hamiltonian can be viewed as (see [ref] for details) [equation] where $T$ is a dynamical variable related to the thermodynamical parameters of the perfect fluid and $P_T$ is its conjugate momentum.
Classical and quantum massive cosmology for the open FRW universe · Preliminary set-up · 0.94
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