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Unitary evolution of the quantum Universe with a Brown-Kuchar dust

机译:带有布朗-库恰粉尘的量子宇宙的ary变

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摘要

We study the time evolution of a wave function for the spatially flat Friedmann-Lemaitre-Robertson-Walker Universe governed by the Wheeler-DeWitt equation in both analytical and numerical methods. We consider a Brown-Kuchar dust as a matter field in order to introduce a 'clock' in quantum cosmology and adopt the Laplace-Beltrami operator-ordering. The Hamiltonian operator admits an infinite number of self-adjoint extensions corresponding to a one-parameter family of boundary conditions at the origin in the minisuperspace. For any value of the extension parameter in the boundary condition, the evolution of a wave function is unitary and the classical initial singularity is avoided and replaced by the big bounce in the quantum system. Exact wave functions show that the expectation value of the spatial volume of the Universe obeys the classical-time evolution in the late time but its variance diverges.
机译:我们用解析和数值方法研究了由Wheeler-DeWitt方程控制的空间平坦的Friedmann-Lemaitre-Robertson-Walker宇宙的波动函数的时间演化。为了将量子宇宙学引入“时钟”并采用Laplace-Beltrami算子排序,我们将Brown-Kuchar尘视为物质场。哈密​​顿算子允许无限数量的自伴随扩展,对应于超超空间原点处的一参数族边界条件。对于边界条件下扩展参数的任何值,波动函数的演化都是统一的,并且避免了经典的初始奇异性,并由量子系统中的大反弹代替。精确的波动函数表明,宇宙空间体积的期望值在后期服从古典时间的演化,但其方差却有所不同。

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