宇宙的状态

J. Hartle
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引用次数: 1

摘要

宇宙的量子态是什么?这是量子宇宙学的核心问题。本文描述了该量子态在支配宇宙中所有物理系统普遍表现出的规律的最终理论中的位置。这个最终理论有可能由两部分组成:(1)动力理论,如超弦理论;(2)宇宙状态,如霍金的无边界波函数。两者都是必要的,因为量子力学中的预测既需要哈密顿量,也需要状态。对状态的完全无知导致预测与观察不一致。在早期宇宙中观察到的简单性给人们带来了希望,即存在一种简单的、可发现的宇宙量子态。也许,就像动力学理论一样,对晚时间、低能量观测的量子态的预测可以用一个有效的宇宙学理论来总结。这不应掩盖为这种有效的理论提供基本基础的必要性,这种理论对其特点作出统一的解释,并且在没有限制性假设的情况下适用。可能有一个原理既决定了动力学理论又决定了量子态。这将是一个真正统一的终极理论。(在“理论物理和宇宙学的未来:霍金60岁生日研讨会”上的演讲)
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The State of the Universe
What is the quantum state of the universe? That is the central question of quantum cosmology. This essay describes the place of that quantum state in a final theory governing the regularities exhibited universally by all physical systems in the universe. It is possible that this final theory consists of two parts: (1) a dynamical theory such as superstring theory, and (2) a state of the universe such as Hawking's no-boundary wave function. Both are necessary because prediction in quantum mechanics requires both a Hamiltonian and a state. Complete ignorance of the state leads to predictions inconsistent with observation. The simplicity observed in the early universe gives hope that there is a simple, discoverable quantum state of the universe. It may be that, like the dynamical theory, the predictions of the quantum state for late time, low energy observations can be summarized by an effective cosmological theory. That should not obscure the need to provide a fundamental basis for such an effective theory which gives a a unified explanation of its features and is applicable without restrictive assumptions. It could be that there is one principle that determines both the dynamical theory and the quantum state. That would be a truly unified final theory. (talk given The Future of Theoretical Physics and Cosmology: Stephen Hawking 60th Birthday Symposium)
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FRONT MATTER Are We Typical? The Physics of ‘Now’ BACK MATTER The Impact of Cosmology on Quantum Mechanics
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