Is the BKL map an intrinsic feature of the Quantum Mixmaster Universe?

IF 10.5 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Simone Lo Franco , Giovanni Montani
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引用次数: 0

Abstract

We study the quantum Mixmaster dynamics by constructing the corresponding Wheeler-DeWitt equation as a relativistic quantum theory in a pseudo-Riemannian Mini-superspace. The transition amplitude from a Kasner regime to the next one is built via the standard S-matrix of a relativistic scattering, and mediated by a single wall potential. We provide a coherent and convincing representation of the original Misner's idea that quasi-classical states can survive arbitrarily close to the cosmological singularity. By constructing a complete set of states, we demonstrate that the quasi-classical BKL map is preserved by the resulting transition amplitude to a new state when their mean total momentum is high enough (exactly coinciding with Misner's high occupation numbers). This scheme is naturally iterated to the initial singularity without appreciable shape changes. We also clarify the role played by the state localization, and, in particular, we outline that when the incoming state is spread, the possibility of violating the Kasner map is no longer negligible. Thus, Kasner-like wave packets can approach the initial singularity.
BKL映射是量子Mixmaster宇宙的内在特征吗?
我们通过在伪黎曼迷你超空间中构造相应的Wheeler-DeWitt方程作为相对论量子理论来研究量子Mixmaster动力学。从卡斯纳状态到下一个状态的过渡振幅是通过相对论散射的标准s矩阵建立的,并由单个壁势介导。我们提供了一个连贯的和令人信服的原始米斯纳的想法,准经典状态可以生存任意接近宇宙奇点。通过构造一个完整的状态集,我们证明了当它们的平均总动量足够高(与Misner的高占用数完全吻合)时,得到的新状态的过渡幅度保留了准经典BKL映射。该方案可以自然地迭代到初始奇点,没有明显的形状变化。我们还澄清了状态局域化所起的作用,特别是,我们概述了当传入状态传播时,违反卡斯纳图的可能性不再是可以忽略不计的。因此,类卡斯纳波包可以接近初始奇点。
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来源期刊
Journal of High Energy Astrophysics
Journal of High Energy Astrophysics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
9.70
自引率
5.30%
发文量
38
审稿时长
65 days
期刊介绍: The journal welcomes manuscripts on theoretical models, simulations, and observations of highly energetic astrophysical objects both in our Galaxy and beyond. Among those, black holes at all scales, neutron stars, pulsars and their nebula, binaries, novae and supernovae, their remnants, active galaxies, and clusters are just a few examples. The journal will consider research across the whole electromagnetic spectrum, as well as research using various messengers, such as gravitational waves or neutrinos. Effects of high-energy phenomena on cosmology and star-formation, results from dedicated surveys expanding the knowledge of extreme environments, and astrophysical implications of dark matter are also welcomed topics.
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