Condensed Matter

K. Binder, A. Muramatsu, D. Wolf
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引用次数: 0

Abstract

Condensed matter physics provides an understanding of macroscopic properties of solid or liquid matter in terms of the properties of nuclei and electrons of the constituting atoms. While in principle the problem is well understood - quantum mechanics of interacting many-body systems together with statistical mechanics provides the appropriate framework - in practice the problem is extremely complicated. Thus, a full first princi-ples approach, where one would solve the Dirac or Schr¨odinger equation for a system of N ≈ 10 22 nuclei (as contained in 1 cm 3 of condensed matter at typical conditions) plus the appropriate number of electrons, and then uses this information within the formalism of statistical thermodynamics, is by no means feasible. This will not become feasible dur-ing the next decades, even if the exponential increase of the computational power of the available hardware with time continues.
凝聚态
凝聚态物理根据构成原子的原子核和电子的性质,提供了对固体或液体物质的宏观性质的理解。虽然原则上这个问题很好理解——多体系统相互作用的量子力学与统计力学一起提供了适当的框架——但实际上这个问题极其复杂。因此,一个完整的第一原理方法,一个人将解决狄拉克或薛定谔方程的N≈10 22个原子核(在典型条件下包含在1厘米3的凝聚态物质中)加上适当数量的电子的系统,然后在统计热力学的形式体系中使用这些信息,是不可行的。即使现有硬件的计算能力随着时间的推移呈指数级增长,这在未来几十年里也不可能实现。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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