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Quantum FRW cosmological solutions in the presence of Chaplygin gas and perfect fluid

机译:Chaplygin 气体和完美流体存在下的量子 FRW 宇宙学解决方案

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We present a Friedmann-Robertson-Walker quantum cosmological model in the presence of Chaplygin gas and perfect fluid for early and late time epochs. In this work, we consider perfect fluid as an effective potential and apply Schutz's variational formalism to the Chaplygin gas which recovers the notion of time. These give rise to Schrodinger-Wheeler-DeWitt equation for the scale factor. We use the eigenfunctions in order to construct wave packets and study the time dependent behavior of the expectation value of the scale factor using the many-worlds interpretation of quantum mechanics. We show that contrary to the classical case, the expectation value of the scale factor avoids singularity at quantum level. Moreover, this model predicts that the expansion of Universe is accelerating for the late times. (c) 2007 Elsevier B.V. All rights reserved.
机译:我们提出了一个弗里德曼-罗伯逊-沃克量子宇宙学模型,该模型在早期和晚期存在Chaplygin气体和完美流体的情况下。在这项工作中,我们将完美流体视为一种有效势能,并将舒茨的变分形式主义应用于恢复时间概念的 Chaplygin 气体。这些产生了比例因子的薛定谔-惠勒-德威特方程。我们使用特征函数来构造波包,并使用量子力学的多世界解释研究比例因子期望值的瞬态行为。我们表明,与经典情况相反,比例因子的期望值避免了量子水平上的奇异性。此外,该模型预测宇宙的膨胀在后期正在加速。(c) 2007年Elsevier B.V.保留所有权利。

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