宇宙背景玻色凝聚（CBBC）
Cosmic Background Bose Condensation (CBBC)
摘要：
粒子质量越小、温度越低、数密度越高，玻色子的简并效应越重要。玻色凝聚要求粒子处于相同的最低能量量子态。我们提出了一个宇宙背景玻色凝聚，无处不在，其粒子具有最低的量子能态，$\hbar c / λ$，与$λ$的可见宇宙的大小，因此非定域。这一点我们等同于任何粒子的自引力势能的量子，等同于能量最小的信息位。宇宙熵（$\sim 10^{122} \ bits$）是可见宇宙中粒子数密度（$ \sim 10^{36} \ bits / cm^3$）最高、质量（$\sim 10^{-66} g$）最小、温度（$\sim 10^{-29} K$）最低的。因此，它是宇宙背景玻色凝聚（CBBC）的最佳候选者，CBBC是一种完全平静的流体，没有粘度，处于超流状态，可能是宇宙膨胀的原因。
英文摘要：
Degeneracy effects for bosons are more important for smaller particle mass, smaller temperature and higher number density. Bose condensation requires that particles be in the same lowest energy quantum state. We propose a cosmic background Bose condensation, present everywhere, whith its particles having the lowest quantum energy state, $\hbar c / λ$, with $λ$ about the size of the visible universe, and therefore unlocalized. This we identify with the quantum of the self gravitational potential energy of any particle, and with the bit of information of minimum energy. The entropy of the universe ($\sim 10^{122} \ bits$) has the highest number density ($ \sim 10^{36} \ bits / cm^3$) of particles inside the visible universe, the smallest mass, $\sim 10^{-66} g$, and the smallest temperature, $\sim 10^{-29} K$. Therefore it is the best candidate for a Cosmic Background Bose Condensation (CBBC), a completely calmed fluid, with no viscosity, in a superfluidity state, and possibly responsible for the expansion of the universe.
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